قائمة بأجرام النظام الشمسي حسب الحجم

تتضمن هذه المقالة قائمة بأضخم الأجسام المعروفة في النظام الشمسي، وقوائم جزئية للأجسام الأصغر حجماً مرتبة حسب متوسط نصف قطرها المرصود . ويمكن ترتيب هذه القوائم وفقاً لنصف قطر الجسم وكتلته، وبالنسبة لأضخم الأجسام، وفقاً لحجمها وكثافتها وجاذبيتها السطحية، إن توفرت هذه القيم.

تحتوي هذه القوائم على الشمس والكواكب والكواكب القزمة والعديد من الأجسام الصغيرة الأكبر حجماً في النظام الشمسي (والتي تشمل الكويكبات ) وجميع الأقمار الطبيعية المسماة وعدد من الأجسام الأصغر ذات الأهمية التاريخية أو العلمية، مثل المذنبات والأجسام القريبة من الأرض .

تم اكتشاف العديد من الأجسام العابرة لنبتون ؛ وفي كثير من الحالات، تكون مواقعها في هذه القائمة تقريبية، نظرًا لوجود هامش خطأ كبير في تقدير أقطارها بسبب بعدها عن الأرض. كما توجد شكوك في قيم الكتلة ونصف القطر، واختلافات في الشكل والكثافة، وتعتمد دقة التقدير غالبًا على مدى قرب الجسم من الأرض أو ما إذا كان قد تمت زيارته بواسطة مسبار.

من المعروف أو المتوقع أن تكون الأجسام الموجودة في النظام الشمسي والتي تزيد كتلتها عن 10 ^{^21}كيلوغرامًا كروية الشكل تقريبًا. وتتحول الأجرام الفلكية إلى أشكال كروية ( أجسام كروية جزئية )، محققةً التوازن الهيدروستاتيكي ، عندما تكون جاذبيتها كافية للتغلب على قوة بنيتها. كان يُعتقد أن الحد الفاصل للأجسام الكروية يتراوح بين 100 و200 كيلومتر في نصف القطر إذا كانت تحتوي على كمية كبيرة من الجليد؛ ^{[ 1 ]} ومع ذلك، كشفت دراسات لاحقة أن الأقمار الجليدية الكبيرة مثل إيابيتوس (قطره 1470 كيلومترًا) ليست في حالة توازن هيدروستاتيكي في الوقت الحالي، ^{[ 2 ]} ويشير تقييم أُجري عام 2019 إلى أن العديد من الأجسام العابرة لنبتون التي يتراوح حجمها بين 400 و1000 كيلومتر قد لا تكون حتى أجسامًا صلبة تمامًا، ناهيك عن كونها كروية بفعل الجاذبية. ^{[ 3 ]} تُشار إلى الأجسام التي تكون بيضاوية الشكل بسبب جاذبيتها الخاصة هنا بشكل عام على أنها "مستديرة"، سواء كانت في حالة توازن اليوم أم لا، في حين أن الأجسام التي من الواضح أنها ليست بيضاوية الشكل تُشار إليها على أنها "غير منتظمة".

تتميز الأجسام الكروية عادةً بتسطح قطبي نتيجةً لقوة الطرد المركزي الناتجة عن دورانها، وقد يكون لها أحيانًا أقطار استوائية مختلفة تمامًا ( مثل الأجسام الإهليلجية المختلفة الأضلاع كجسم هاوميا ). وعلى عكس أجسام مثل هاوميا، تتميز الأجسام غير المنتظمة بشكل غير إهليلجي واضح، وغالبًا ما تكون حوافها حادة.

قد يصعب تحديد قطر الأجسام النموذجية الواقعة وراء كوكب زحل (ضمن هامش خطأ يبلغ حوالي الضعف). أما بالنسبة للأجسام العابرة لنبتون، فهناك قدر من الثقة في تحديد أقطارها، ولكن بالنسبة للأجسام العابرة لنبتون غير الثنائية، فلا توجد ثقة حقيقية في كتلها/كثافتها. يُفترض عادةً أن العديد من الأجسام العابرة لنبتون لها كثافة بلوتو البالغة 2.0 غ/سم³ ^، ولكن من المحتمل بنفس القدر أن تكون كثافتها شبيهة بكثافة المذنبات، أي 0.5 غ/سم³ ^فقط . ^{[ 4 ]}

على سبيل المثال، إذا افترضنا خطأً أن كتلة جرم عابر لنبتون تبلغ 3.59 × 10بناءً على نصف قطر يبلغ 350^كم وكثافة 2 جم/سم³^، ولكن تبين لاحقًا أن نصف قطره 175 كم فقط وكثافته 0.5 جم/سم³^، فإن كتلته الحقيقية ستكون 1.12 × 10⁻⁶ كجم فقط.¹⁹ كجم.

تُعرف أحجام وكتل العديد من أقمار المشتري وزحل بشكل جيد نسبيًا بفضل عمليات الرصد والتفاعلات العديدة التي أجرتها المركبتان الفضائيتان غاليليو وكاسيني ؛ ومع ذلك، فإن كتل العديد من الأقمار التي يقل نصف قطرها عن 100 كيلومتر تقريبًا، مثل قمر هيماليا التابع للمشتري ، غير مؤكدة إلى حد كبير. ^{[ 5 ]} أما في المناطق الأبعد عن زحل، فإن أحجام وكتل الأجرام أقل وضوحًا. ولم تُرسل مركبة فضائية حتى الآن لدراسة أقمار أورانوس أو نبتون على المدى الطويل. وبالنسبة للأقمار الخارجية الصغيرة غير المنتظمة لأورانوس، مثل سيكوراكس ، التي لم تكتشفها المركبة فوياجر 2 ، فإن صفحات الويب المختلفة التابعة لناسا، مثل المركز الوطني لبيانات علوم الفضاء ^{[ 6 ]} وموقع ديناميكيات النظام الشمسي التابع لمختبر الدفع النفاث ^{[ 5 ]،} تُقدم تقديرات متضاربة إلى حد ما لأحجامها وانعكاساتها، وذلك بحسب البحث العلمي المُستشهد به.

نظرة عامة بيانية

الأقطار النسبية لأكبر خمسين جسماً تم قياسها في النظام الشمسي، مُلوّنة حسب المنطقة المدارية. القيم هي الأقطار بالكيلومترات. كلا المقياسين خطيان.

الكتل النسبية لأجرام النظام الشمسي. الأجرام الأصغر من زحل غير مرئية بهذا المقياس.
الكتل النسبية للكواكب الشمسية. يهيمن كوكب المشتري بنسبة 71% من المجموع الكلي، بينما يهيمن كوكب زحل بنسبة 21% على النظام.
الكتل النسبية للأجرام الصلبة في النظام الشمسي. تهيمن الأرض بنسبة 48% والزهرة بنسبة 39%. أما الأجرام الأقل كتلة من بلوتو فلا يمكن رؤيتها بهذا المقياس.
مخططان دائريان، أحدهما متداخل داخل الآخر، يوضحان الكتل النسبية لأقمار النظام الشمسي الرئيسية ^{[ 7 ]}

الأجسام التي يزيد نصف قطرها عن 400 كيلومتر

يبلغ نصف القطر الحجمي الاسمي للأجسام التالية 400 كيلومتر أو أكثر. كان يُعتقد سابقًا أن أي جسم جليدي يزيد نصف قطره عن 200 كيلومتر تقريبًا يكون في حالة توازن هيدروستاتيكي . ^{[ 8 ]} ومع ذلك، يُعد سيريس (نصف قطره 470 كيلومترًا) أصغر جسم تتوافق قياساته التفصيلية مع حالة التوازن الهيدروستاتيكي، ^{[ 9 ]} بينما يُعد إيابيتوس (نصف قطره 735 كيلومترًا) أكبر جسم جليدي وُجد أنه ليس في حالة توازن هيدروستاتيكي. ^{[ 10 ]} جميع الأقمار الجليدية المعروفة في هذا النطاق بيضاوية الشكل (باستثناء بروتيوس )، ولكن قد تكون الأجسام العابرة لنبتون التي يصل نصف قطرها إلى 450-500 كيلومتر مسامية للغاية. ^{[ 11 ]}

لتبسيط الحسابات ولأغراض المقارنة، تُحسب القيم يدويًا بافتراض أن جميع الأجسام كروية الشكل. ولا يشمل حجم الأجسام الصلبة غلافها الجوي. فعلى سبيل المثال، يبدو تيتان أكبر من غانيميد، لكن جسمه الصلب أصغر. أما بالنسبة للكواكب العملاقة ، فيُعرَّف "نصف القطر" بأنه المسافة من المركز التي يصل عندها ضغط الغلاف الجوي إلى 1 بار. ^{[ 12 ]}

لأن سدنا ليس لها أقمار معروفة، فإن تحديد كتلتها بشكل مباشر أمر مستحيل دون إرسال مسبار.

الجسم ^{[ ملاحظة 1 ]}	صورة	نصف القطر ^{[ ملاحظة 2 ]}		مقدار		كتلة		مساحة السطح		كثافة	الجاذبية ^{[ ملاحظة 3 ]}		يكتب	اكتشاف
الجسم ^{[ ملاحظة 1 ]}	صورة	( كم )	( R _🜨 )	( 109 كم ³ )	( V _🜨 )	( 10 ²¹ كجم)	( م _🜨 )	( ¹⁰⁶كم ² )	🜨	(جم/ ^سم³ )	(م/ ^ث² )	( 🜨 )	يكتب	اكتشاف
شمس		695 700 ± ؟ ^{[ 13 ]}	109.2 ^{[ 14 ]}	1,409,300,000 ^{[ 14 ]}	1,301,000 ^{[ 14 ]}	1 988 475 000 ± 92 000 ^{[ 15 ]}	333,000 ^{[ 14 ]}	6,078,700 ^{[ 14 ]}	11918 ^{[ 14 ]}	1.409 ^{[ 14 ]}	274.0 ^{[ 14 ]}	27.94 ^{[ 14 ]}	نجم من فئة G2V	ما قبل التاريخ
كوكب المشتري		69886 ± 0.4 ^[¹⁶^]	10.97	1,431,280	1321	1 898 125 ± 88 ^{[ 17 ]}	317.83	61,419 ^{[ 18 ]}	120.41	1.3262 ± 0.0003 ^{[ 17 ]}	24.79 ^{[ 17 ]}	2.528	كوكب غازي عملاق ؛ له حلقات	ما قبل التاريخ
زحل		58232 ± 6 ^{[ 17 ]} (136775 لخاتم أ )	9.140	827,130	764	568 317 ± 26 ^{[ 17 ]}	95.162	42,612 ^{[ 19 ]}	83.54	0.6871 ± 0.0002 ^{[ 17 ]}	10.44 ^{[ 17 ]}	1.065	كوكب غازي عملاق ؛ له حلقات	ما قبل التاريخ
أورانوس		25362 ± 7 ^[¹⁷^]	3.981	68,340	63.1	86809.9 ± 4.0 ^[¹⁷^]	14.536	8083.1 ^{[ 20 ]}	15.85	1.270 ± 0.001 ^{[ 17 ]}	8.69 ^{[ 17 ]}	0.886	كوكب عملاق جليدي ؛ له حلقات	1781
نبتون		24622 ± 19 ^[¹⁷^]	3.865	62,540	57.7	102 409 .2 ± 4.8 ^{[ 17 ]}	17.147	7618.3 ^{[ 21 ]}	14.94	1.638 ± 0.004 ^{[ 17 ]}	11.15 ^{[ 17 ]}	1.137	كوكب عملاق جليدي ؛ له حلقات	1846
أرض		6371.0084 ± 0.0001 ^[¹⁷^]	1	1,083.21	1	5972.17 ± 0.28 ^[¹⁷^]	1	510.06447 ^{[ 22 ]}	1	5.5134 ± 0.0003 ^{[ 17 ]}	9.81 ^{[ 17 ]}	1	كوكب أرضي	ما قبل التاريخ
الزهرة		6051.8 ± 1.0 ^[¹⁷^]	0.9499	928.43	0.857	4867.31 ± 0.23 ^[¹⁷^]	0.815	460.2 ^{[ 23 ]}	0.903	5.243 ± 0.003 ^{[ 17 ]}	8.87 ^{[ 17 ]}	0.905	كوكب أرضي	ما قبل التاريخ
المريخ		3389.5 ± 0.2 ^[¹⁷^]	0.5320	163.18	0.151	641.691 ± 0.030 ^{[ 17 ]}	0.107	144.37 ^{[ 24 ]}	0.283	3.9340 ± 0.0007 ^{[ 17 ]}	3.71 ^{[ 17 ]}	0.379	كوكب أرضي	ما قبل التاريخ
غانيميد جوبيتر الثالث		2634.1 ± 0.3 ^[²⁵^]	0.4135	76.30	0.0704	148.19	0.0248	86.999 ^{[ 26 ]}	0.171	1.936 ^{[ 25 ]}	1.428	0.146	قمر المشتري (جليدي)	1610
تيتان زحل السادس		2574.73 ± 0.09 ^[²⁷^]	0.4037 ^{[ أ ]}	71.50	0.0658	134.518 ± 0.003 ^{[ 28 ]}	0.0225	83.3054 ^{[ 29 ]}	0.163	1.880 ± 0.004 ^{[ 30 ]}	1.354	0.138	قمر زحل (جليدي)	1655
الزئبق		2439.4 ± 0.1 ^[¹⁷^]	0.3829	60.83	0.0562	330.103 ± 0.021 ^{[ 17 ]}	0.0553	74.797 ^{[ 31 ]}	0.147	5.4289 ± 0.0007 ^{[ 17 ]}	3.70 ^{[ 17 ]}	0.377	كوكب أرضي	ما قبل التاريخ
كاليستو جوبيتر الرابع		2 410 .3 ± 1.5 ^{[ 32 ]}	0.3783	58.65	0.0541	107.594	0.018	73.005 ^{[ 33 ]}	0.143	1.834 ± 0.003 ^{[ 32 ]}	1.23603	0.126	قمر المشتري (جليدي)	1610
قمر آيو كوكب المشتري الأول		1821.6 ± 0.5 ^[⁵^]	0.2859	25.32	0.0234	89.32	0.015	41.698 ^{[ 34 ]}	0.082	3.528 ± 0.006 ^{[ 35 ]}	1.797	0.183	قمر تابع لكوكب المشتري (أرضي)	1610
القمر الأرض ١		1737.4 ± 0.1 ^[³⁶^]	0.2727	21.958	0.0203	73.46 ^{[ 37 ]}	0.0123	37.937 ^{[ 38 ]}	0.074	3.344 ± 0.005 ^{[ 36 ]}	1.625	0.166	قمر الأرض (الأرضي)	ما قبل التاريخ
أوروبا جوبيتر 2		1 560 .8 ± 0.5 ^{[ 5 ]}	0.2450	15.93	0.0147	48.00	0.008035	30.613 ^{[ 39 ]}	0.06	3.013 ± 0.005	1.316	0.134	قمر تابع لكوكب المشتري (أرضي)	1610
تريتون نبتون الأول		1 353 .4 ± 0.9 ^{[ أ ]}^{[ 27 ]}	0.2124 ^{[ أ ]}	10.38	0.0096	21.39 ± 0.03	0.003599	23.018 ^{[ 40 ]}	0.045	2.061	0.782	0.0797	قمر نبتون (جليدي)	1846
بلوتو 134340		1 188 .3 ± 0.8 ^{[ 41 ]}	0.187	7.057	0.00651	13.03 ± 0.03	0.0022	17.79	0.034	1.853 ± 0.004 ^{[ 42 ]}	0.620	0.063	كوكب قزم ؛ بلوتينو ؛ متعدد	1930
إيريس 136199		1 163 ± 6 ^{[ ب ]}^{[ 43 ]}	0.1825 ^{[ ب ]}	6.59	0.0061	16.38 ± 0.2 ^{[ ج ]}	0.0028	17	0.033	2.43 ± 0.05	0.824	0.083	كوكب قزم ؛ مرصد ديناميكا الشمس ؛ نظام ثنائي	2003
تيتانيا أورانوس الثالث		788.4 ± 0.6 ^{[ 46 ]}	0.1237 ^{[ د ]}	2.06	0.0019	3.4550 ± 0.0509 ^{[ 47 ]}	0.00059	7.82 ^{[ 48 ]}	0.015	1.683	0.378	0.0385	قمر أورانوس	1787
هاوميا 136108		772 +20 −19 ^{[ 49 ]}	0.12	1.98 ^{[ هـ ]}	0.0018	3.952 44 +0.011 09 −0.011 03 ^{[ 51 ]}	0.00066	8.14	0.016	2.050 +0.157 −0.152 ^{[ 49 ]}^{[ f ]}	0.401	0.0409	كوكب قزم ؛ جرم سماوي رنيني في حزام كايبر (7:12)؛ ثلاثي النجوم ؛ له حلقات	2004
ريا زحل الخامس		763.5 ± 0.5 ^{[ 52 ]}	0.1199 ^{[ د ]}	1.87	0.0017	2.307	0.00039	7.34 ^{[ 53 ]}	0.014	1.2372 ± 0.0029 ^{[ 52 ]}	0.26	0.027	قمر زحل	1672
أوبرون أورانوس الرابع		761.4 ± 2.6 ^{[ أ ]}^{[ 27 ]}	0.1195 ^{[ أ ]}	1.85	0.0017	3.1104 ± 0.0749 ^{[ 47 ]}	0.0005	7.285 ^{[ 54 ]}	0.014	1.682	0.347	0.035	قمر أورانوس	1787
إيابيتوس زحل الثامن		734.4 ± 2.8 ^{[ 55 ]}^{[ 52 ]}	0.1153	1.66	0.0015	1.806	0.00033	6.8	0.013	1.0887 ± 0.0127 ^{[ 52 ]}	0.223	0.0227	قمر زحل	1671
ماكيماكي 136472		715 ± 7 ^{[ 56 ]}	0.112	1.53	0.0014	2.69 ± 0.20 ^{[ 57 ]}^{[ g ]}	0.00045	6.4	0.013	1.76 ± 0.17	0.35	0.0357	كوكب قزم ؛ كيوبوانو	2005
غونغ غونغ 225088		615 ± 25 ^{[ 58 ]}^{[ غرام ]}	0.0983	1.03	0.0009	1.75 ± 0.07 ^{[ 58 ]}	0.00029	4.753	0.009	1.74 ± 0.16 ^{[ 58 ]}	0.3	0.0306	كوكب قزم ؛ مرصد ديناميكا الشمس الرنان (3:10)	2007
شارون بلوتو الأول		606.0 ± 0.5 ^{[ 41 ]}	0.0951	0.932	0.0009	1.5897 ± 0.0045 ^{[ 42 ]}	0.00025	4.578 ^{[ 59 ]}	0.009	1.705 ± 0.006 ^{[ 42 ]}	0.288	0.0294	قمر بلوتو	1978
أومبريل أورانوس الثاني		584.7 ± 2.8 ^{[ 27 ]}	0.0918	0.837	0.0008	1.2885 ± 0.0225 ^{[ 47 ]}	0.00020	4.3 ^{[ 60 ]}	0.008	1.539	0.234	0.024	قمر أورانوس	1851
أرييل أورانوس الأول		578.9 ± 0.6 ^{[ 27 ]}	0.0909	0.813	0.0007	1.2331 ± 0.0180 ^{[ 47 ]}	0.000226	4.211 ^{[ 61 ]}	0.008	1.517	0.269	0.027	قمر أورانوس	1851
ديون زحل الرابع		561.4 ± 0.4 ^{[ 55 ]}^{[ 52 ]}	0.0881	0.741	0.0007	1.095 4868 ± 0.000 0246 ^{[ 52 ]}	0.000183	3.965 ^{[ 62 ]}	0.008	1.478 ± 0.003	0.232	0.0237	قمر زحل	1684
كواوار 50000		548.8 ± 1.1 ^{[ 63 ]}	0.0879	0.737	0.0007	1.212 ± 0.005 ^{[ 63 ]}	0.0002	3.83	0.008	1.751 ± 0.013 ^{[ 63 ]}	0.3	0.0306	كوكب قزم ؛ مكعب الشكل ؛ ثنائي ؛ له حلقات	2002
تيثيس زحل الثالث		531.1 ± 0.6 ^{[ 64 ]}^{[ 52 ]}	0.0834	0.624	0.0006	0.617 4959 ± 0.000 0146 ^{[ 65 ]}	0.000103	3.57 ^{[ 66 ]}	0.007	0.984 ± 0.003 ^{[ 64 ]}	0.145	0.015	قمر زحل	1684
سيريس 1		469.7 ± 0.1 ^{[ 67 ]}	0.0742	0.433	0.0004	0.938 392 ± 0.000 005 ^{[ 68 ]}	0.000157	2.85 ^{[ 69 ]}	0.006 ^{[ 69 ]}	2.1616 ± 0.0025 ^{[ 68 ]}	0.28	0.029	كوكب قزم ؛ كويكب حزام	1801
أوركس 90482		455 +25 −20 ^{[ 70 ]}	0.0719	0.404	0.0004	0.548 ± 0.010 ^{[ 45 ]}	0.000092			1.4 ± 0.2 ^{[ 45 ]}	0.2	0.0204	كوكب قزم ؛ بلوتينو ؛ ثنائي	2004
سيدنا 90377		450 +160 −130 ^{[ 71 ]}	0.0711	0.516	0.0005								كوكب قزم ؛ جسم منفصل ؛ جسم منفصل	2003
سالاسيا 120347		419 ± 22 ^{[ 72 ]}	0.0664	0.373	0.0003	0.4861 +0.0076 −0.0074 ^{[ 73 ]}^{[ g ]}	0.000082			1.5 ± 0.1 ^{[ 74 ]}	0.185	0.0168	كيوبوانو ؛ ثنائي	2004
نجم عملاق، كوكب أرضي، كوكب قزم، كوكب قزم محتمل، قمر الأرض ، قمر المشتري ، قمر زحل، قمر أورانوس ، قمر نبتون ، قمر بلوتو

الأجسام الأصغر حجماً حسب متوسط نصف القطر

من 200 إلى 399 كم

جميع الأقمار الجليدية المصورة التي يزيد نصف قطرها عن 200 كم، باستثناء بروتيوس، تبدو كروية بوضوح، على الرغم من أن تلك التي يقل نصف قطرها عن 400 كم والتي تم قياس أشكالها بدقة ليست في حالة توازن هيدروستاتيكي. ^{[ 75 ]} الكثافة المعروفة للأجرام العابرة لنبتون في هذا النطاق الحجمي منخفضة بشكل ملحوظ (تتراوح كثافتها بين 1 و1.2 غ/سم³ ^، مما يشير إلى احتفاظ هذه الأجسام بمسامية داخلية كبيرة منذ تكوينها، وأنها لم تتعرض أبدًا لضغط جاذبي لتصبح أجسامًا صلبة تمامًا. ^{[ 11 ]} العديد من الأجسام العابرة لنبتون الساطعة بطبيعتها، مثل 2018 VG 18 و 2017 OF 201، لا تتوفر لها أحجام مُقاسة مباشرة (على سبيل المثال، عبر الاحتجاب النجمي وقياس الإشعاع الحراري )، لذا تُقدّر أحجامها بناءً على قيمة البياض المفترضة . ^[⁷⁶^] في القائمة أدناه، تُدرج الأجسام العابرة لنبتون ذات الأحجام غير المُقاسة فقط إذا ذُكرت في البيانات الصحفية والمراجع العلمية.

الجسم ^{[ ملاحظة 1 ]}	نصف القطر ^{[ ملاحظة 2 ]} ( كم )	الكتلة (10 ¹⁸ كجم)	الكثافة (جم/ ^سم³ )	اكتب ^{[ ملاحظة 4 ]}	المراجع ^{[ ملاحظة 5 ]} ر · م
ماني 307261	398 ± 12	–	–	كيوبوانو	^{[ 77 ]}
أخليس 208996	386 ± 6 ( ما يعادل المساحة )	≈ 200 ^{[ ساعة ]}	0.87 ± 0.01 (بافتراض HE) ^{[ 80 ]}	بلوتينو ؛ ثنائي	^{[ 80 ]}
آيا 55565	384 +20 −19	–	–	كيوبوانو	^{[ 81 ]}
2010 JO ₁₇₉ 574372	≈ 375 ± 75 ^{[ i ]}	–	–	SDO	^{[ 82 ]}
تشيمينيغاوا 532037	371 +39 −42	–	–	SDO ؛ ثنائي	^{[ 83 ]}
فاردا 174567	370 ± 7	244 ± 6 ^{[ j ]}	1.23 ± 0.04 أو1.78 ± 0.06 ^{[ 85 ]}	كيوبوانو؛ ثنائي	^{[ 85 ]} ·^[⁸⁵^]
2017 من 201	≈ 350 ^{[ i ]}	–	–	إيتنو	^{[ 86 ]}
إكسيون 28978	348.4 +5.4 −4.4 ( ما يعادل المساحة )	–	–	بلوتينو	^{[ 87 ]}
2021 DR 15	345 ± 80 ^{[ i ]}	–	–	SDO	^{[ 88 ]}
غويبنيو 90568	340 ± 17	–	–	كيوبوانو	^{[ 89 ]}
ريتونا 145452	340 +28 −36	–	–	كيوبوانو	^{[ 89 ]}
2015 RR 245 523794	≈ 335 ^{[ i ]}	–	–	رنين KBO (2:9)	^{[ 90 ]}
Uni 55637	330 ± 19	125 ± 3 ^{[ غرام ]}	0.82 ± 0.11	كيوبوانو؛ ثنائي	^{[ 91 ]} ·^[⁹²^]
فارونا 20000	327 +77 −51	≈ 160	0.992 +0.086 −0.015 ^{[ 93 ]}	كيوبوانو	^{[ 94 ]}
2003 UZ ₄₁₃ 455502	325 +0.5 −88	≈ 300 ^{[ k ]}	2.64	بلوتينو	^{[ 95 ]}
رومينا 145451	≈ 322	–	–	SDO	^{[ 96 ]}^{[ 97 ]}
2014 UZ 224 (DeeDee)	318 +28 −30	–	–	SDO	^{[ 98 ]}
Gǃkúnǁʼhòmdímà 229762	317 +5 −4	136.1 ± 3.3	1.007 +0.050 −0.049 ^{[ 49 ]}	SDO؛ ثنائي	^{[ 49 ]} ·^[⁹⁹^]
2008 OG ₁₉ 470599	310 +28 −56 ^{[ i ]}	–	0.609 ± 0.004	SDO	^{[ 100 ]} ·^[¹⁰⁰^]
عسر التسمية إيريس ١	308 +60 −50	82 ± 57	0.7 ± 0.5	قمر إيريس	^{[ 45 ]}
2007 JJ ₄₃ 278361	305 +85 −70 ^{[ i ]}	–	–	كيوبوانو	^{[ 101 ]}
2004 XR ₁₉₀ (بافي) 612911	300 ± 85	–	–	SDO	^{[ 102 ]}
2005 QU ₁₈₂ 303775	292 +78 −72	–	–	SDO	^{[ 95 ]}
2014 EZ ₅₁ 523692	> 288	–	–	SDO	^{[ 103 ]}
Xewioso 78799	283 +36 −37	–	–	كيوبوانو	^{[ 104 ]}
2015 BP ₅₁₉ (كاجو) 768325	275 ± 75 ^{[ i ]}			إيتنو	^{[ 105 ]}
فيستا 4	262.7 ± 0.1	259.0271 ± 0.0058	3.456 ± 0.035 ^{[ 106 ]}	كويكبات الحزام من النوع الخامس	^{[ 106 ]} ·^[¹⁰⁷^]
2003 مقابل ₂ 84922	262 ± 4	–	–	بلوتينو	^{[ 108 ]}
بالاس 2	256 ± 2	204 ± 3	2.92 ± 0.08	كويكبات الحزام من النوع ب	^{[ 109 ]}^{[ 110 ]}
2004 TY ₃₆₄ 120348	256 +19 −20	–	–	كيوبوانو	^{[ 111 ]}
2005 TB ₁₉₀ 145480	254 +64 −58	–	–	جسم منفصل	^{[ 111 ]}^{[ 112 ]}
إنسيلادوس زحل الثاني	252.1 ± 0.2	108.0 ± 0.1	1.609 ± 0.005	قمر زحل	^{[ 55 ]} ·^[¹¹³^]
2002 TC ₃₀₂ 84522	250 ± 7	–	–	SDO الرنيني (2:5)	^{[ 114 ]}
2018 VG 18 (Farout)	≈ 250 ^{[ i ]}	–	–	الرنين SDO (2:9)	^{[ 115 ]}
2005 UQ ₅₁₃ 202421	249 +32 −38	–	–	كيوبوانو	^{[ 81 ]}
ميراندا أورانوس الخامس	235.8 ± 0.7	62.93 ± 3.00	1.148	قمر أورانوس	^{[ 116 ]} ·^[⁴⁷^]
دزيوانا 471143	235 +18 −5	–	–	SDO	^{[ 117 ]}
2002 XV ₉₃ 612533	235 +22 −15	–	–	بلوتينو	^{[ 118 ]}
1999 DE ₉ 26375	231 ± 23	–	–	SDO الرنيني (2:5)	^{[ 119 ]}
2003 السنة المالية ₁₂₈ 120132	230 ± 11	–	–	SDO	^{[ 112 ]}
2012 VP 113 (بايدن)	≈ 225 ^{[ i ]}	–	–	سدنويد	^{[ 120 ]}
2002 VR ₁₂₈ 84719	224 +24 −22	–	–	بلوتينو	^{[ 121 ]}
فانث أوركس الأول	221 ± 5	87 ± 8	1.5 +1.0 −0.5	قمر أوركس 90482	^{[ 122 ]} ·^[⁴⁵^]
هيجيا 10	216 ± 4	87.4 ± 6.9	2.06 ± 0.20	كويكبات الحزام من النوع ج	^{[ 123 ]} ·^[¹¹⁰^]
2004 NT ₃₃ 444030	212 +44 −40	–	–	كيوبوانو	^{[ 81 ]}
بروتيوس نبتون الثامن	210 ± 7	15.5–31 ^{[ ل ]}	≈ 0.46–0.91 ^{[ 125 ]}	قمر نبتون	^{[ 5 ]} ·^[⁵^]
الفوضى 19521	208 +42 −15 مكافئ	–	–	كيوبوانو	^{[ 126 ]}
2001 QF ₂₉₈ 469372	204 +20 −22	–	–	بلوتينو	^{[ 121 ]}
هويا 38628	203 ± 8	40.1	1.073 ± 0.066	بلوتينو ؛ ثنائي	^{[ 127 ]} ·^[¹²⁸^]
2004 PF ₁₁₅ 175113	203 +49 −38	–	–	بلوتينو	^{[ 121 ]}
إلماري فاردا 1	202 ± 20	22	–	قمر عام 174567 فاردا	^{[ 72 ]}
أسطورة: SDO – جسم القرص المتناثر كيوبوانو - جسم كلاسيكي من حزام كويبر بلوتينو – رنين مداري بنسبة 2:3 مع نبتون

من 100 إلى 199 كم

تحتوي هذه القائمة على مجموعة مختارة من الأجرام التي يُقدّر نصف قطرها بين 100 و199 كيلومترًا ( قطرها بين 200 و399 كيلومترًا)، ويُطلق علماء الفلك على الأجرام التي يبلغ نصف قطرها 200 ^{كيلومتر} اسم " نصف قطر حبة البطاطا ". قد يكون لأكبر هذه الأجرام شكل متوازن هيدروستاتيكيًا، لكن معظمها غير منتظم (أي على شكل حبة بطاطا). تتراوح كتلتها بين 10²¹ ^و10¹⁸ كيلوغرام . تُحدّد العناصر المدارية لكويكبات الحزام الرئيسي وفقًا لبيانات مختبر الدفع النفاث (JPLSSD) بالنطاق (2.0 وحدة فلكية < a < 3.2 وحدة فلكية؛ q > 1.666 وحدة فلكية). ^[¹²⁹^] تم استبعاد العديد من الأجرام العابرة لنبتون من هذه القائمة نظرًا لقلة المعلومات المتوفرة عن أحجامها. ^[⁷⁶^]

الجسم ^{[ ملاحظة 1 ]}	نصف القطر ^{[ ملاحظة 2 ]} ( كم )	الكتلة ( 10 ¹⁸ كجم )	يكتب	المراجع ^{[ ملاحظة 5 ]} ر · م
2004 UX ₁₀ 144897	199 +16 −20	≳ 30	بلوتينو	^{[ 121 ]} ·^[¹³⁰^]
1993 SC 15789	199 +55 −86	≈ 47	بلوتينو	^{[ 131 ]}
ميماس زحل 1	198.2 ± 0.3	37.49 ± 0.03	قمر زحل	^{[ 55 ]} ·^[¹¹³^]^[²⁷^]
أكتيا سالاسيا 1	196 ± 16	20	قمر عام 120347 سالاسيا	^{[ 72 ]}
1998 SN ₁₆₅ 35671	196 ± 20		كيوبوانو	^{[ 81 ]}
2002 KX ₁₄ 119951	194.6 ± 4.4		كيوبوانو	^{[ 132 ]}
مرحباً ʻ iaka Haumea I	185 ± 10	16 ± 2	قمر هاوميا	^{[ 133 ]} ·^[¹³³^]
2001 UR ₁₆₃ 42301	176 ± 42		رنين KBO (4:9)	^{[ 134 ]}
نيريد نبتون الثاني	170 ± 25	35.7	قمر نبتون	^{[ 27 ]}
1996 TL ₆₆ 15874	170 ± 10		SDO	^{[ 112 ]}
2004 XA ₁₉₂ 230965	170 +60 −48		SDO	^{[ 121 ]}
إنترامنيا 704	166 ± 3	35.2 ± 5.1	كويكبات الحزام من النوع F	^{[ 135 ]} ·^[¹¹⁰^]
يوروبا 52	160 ± 2	23.9 ± 3.8	كويكبات الحزام من النوع ج	^{[ 110 ]}
1999 CD ₁₅₈ 469306	< 155	≈ 48	رنين KBO (4:7)	^{[ 136 ]}
2007 OC ₁₀ 470316	165 ± 28	≈ 30	SDO	^{[ 137 ]}
2023 KQ 14 (أمونايت)	150 ± 40 ^{[ i ]}		سدنويد	^{[ 138 ]}
دافيدا 511	149 ± 2	26.6 ± 7.3	كويكبات الحزام من النوع ج	^{[ 110 ]}
2002 TX ₃₀₀ 55636	143 ± 5	≈ 11	عائلة كوبيوانو ، هاوميا	^{[ 139 ]} ·^[¹³⁹^]
2003 OP ₃₂ 120178	137 +24 −12.	≈ 45	عائلة كوبيوانو، هاوميا	^{[ 136 ]}
سيلفيا 87	137 ± 2	14.3 ± 0.5	كويكب من النوع X في الحزام الخارجي ؛ ثلاثي	^{[ 110 ]}
ليمبو 47171	136 ± 9	6.71	بلوتينو ؛ ثلاثي	^{[ 140 ]}
يونوميا 15	135 ± 2	30.5 ± 1.9	كويكبات الحزام من النوع S	^{[ 110 ]}
هايبريون زحل السابع	135 ± 4	5.62 ± 0.05	قمر زحل	^{[ 75 ]} ·^[⁷⁵^]^[²⁷^]
يوفروزين 31	134 ± 2	16.5 ± 2.6	كويكب حزام من النوع C ؛ ثنائي	^{[ 110 ]}
1998 SM ₁₆₅ 26308	134 ± 14	6.87 ± 1.8	رنين KBO (1:2)	^{[ 141 ]} ·^[¹⁴¹^]
سيبيل 65	131.5 ± 1.5	14.8 ± 1.8	كويكبات الحزام الخارجي من النوع ج	^{[ 142 ]}
جونو 3	127 ± 1	27.0 ± 2.4	كويكبات الحزام من النوع S	^{[ 110 ]}
هيسي ليمبو 2	126 ± 8	5.273	فرعي من 47171 ليمبو	^{[ 140 ]}
هيكتور 624	125 ± 13	7.9 ± 1.4	_حصان طروادة جوبيتر ( L4 ) من النوع D ؛ ثنائي	^{[ 143 ]} ·^[¹⁴³^]
Chariklo 10199	124.8 +3.0 −2.3	6.4 ± 0.5	قنطور ؛ له حلقات	^{[ 144 ]}
سيلا 79360	124 ± 15	5.89	كيوبوانو ؛ ثنائي	^{[ 145 ]}^{[ 146 ]}
2007 RW ₁₀ 309239	124 ± 15		شبه قمر تابع لكوكب نبتون	^{[ 112 ]}
ألتجيرا 148780	123 +19 −70	2.388	كيوبوانو ؛ ثنائي	^{[ 81 ]}^{[ 147 ]}
نونام 79360	118 ± 15	4.892	ثانوي من 79360 سيلا	^{[ 145 ]}^{[ 148 ]}
بامبرغا 324	114 ± 2	10.2 ± 0.9	كويكبات الحزام من النوع ج	^{[ 110 ]}
المريض 451	112.9 ± 2.3	10.9 ± 5.3	كويكبات الحزام من النوع ج	^{[ 149 ]} ·^[¹⁵⁰^]
سايكي 16	112 ± 2	26.2 ± 2.9	كويكبات الحزام من النوع M	^{[ 110 ]}
سيتو 65489	112 ± 5	5.4 ± 0.4	قنطور ممتد ؛ ثنائي	^{[ 112 ]} ·^[¹⁵¹^]
هيركولينا 532	111.2 ± 2.4	10	كويكبات الحزام من النوع S	^{[ 152 ]}
قمر عام 148780 ألتجيرا	110 +17 −62	1.695	ثانوي من 148780 ألتجيرا	^{[ 81 ]}^{[ 153 ]}
ليلياكوهونوا 541132	110 +14 −10		سدنويد	^{[ 154 ]}
ثيسبي 88	109 ± 2	11.6 ± 2.2	كويكبات الحزام من النوع ب	^{[ 110 ]}
دوريس 48	108 ± 2	6.9 ± 2.9	كويكبات الحزام من النوع ج	^{[ 110 ]}
فيبي زحل التاسع	106.5 ± 0.7	8.29 ± 0.01	قمر زحل	^{[ 75 ]} ·^[⁷⁵^]^[²⁷^]
قمر هويا 38628	106 ± 15	5.1	قمر عام 38628 هويا	^{[ 127 ]}
فورتونا 19	105.5 ± 1.0	8.8 ± 1.4	كويكبات الحزام من النوع G	^{[ 110 ]}
كاميلا 107	105 ± 4	11.2 ± 0.3	كويكب من النوع ج في الحزام الخارجي ؛ ثلاثي	^{[ 149 ]} ·^[¹⁵⁰^]
ثيميس 24	104 ± 2	6.2 ± 2.9	كويكبات الحزام من النوع ج	^{[ 110 ]}
أمفيتريت 29	102 ± 1	12.7 ± 2.0	كويكبات الحزام من النوع S	^{[ 110 ]}
إيجيريا 13	101 ± 2	9.2 ± 2.1	كويكبات الحزام من النوع G	^{[ 110 ]}
آيريس 7	100 ± 5	13.5 ± 2.3	كويكبات الحزام من النوع S	^{[ 110 ]}
أسطورة: القنطور – كويكبات تدور بين الكواكب الخارجية طروادة المشتري – كويكبات تقع في نقطتي لاغرانج L4 و _L5 _لكوكب المشتري

من 50 إلى 99 كم

تحتوي هذه القائمة على مجموعة مختارة من الأجرام التي يتراوح نصف قطرها بين 50 و99 كيلومترًا ( بمتوسط قطر يتراوح بين 100 و199 كيلومترًا). تشمل الأجرام المدرجة حاليًا معظم الأجرام في حزام الكويكبات وأقمار الكواكب العملاقة ضمن هذا النطاق الحجمي، ولكن العديد من الأجرام المكتشفة حديثًا في النظام الشمسي الخارجي غير مدرجة، مثل تلك المذكورة في المرجع التالي. ^[⁷⁶^] معظم أنواع الأطياف للكويكبات هي من نوع ثولين، ولكن قد يكون بعضها من نوع SMASS.

الجسم ^{[ ملاحظة 1 ]}	نصف القطر ^{[ ملاحظة 2 ]} ( كم )	الكتلة ( 10 ¹⁸ كجم )	يكتب	المراجع ^{[ ملاحظة 5 ]} ر · م
إلكترا 130	99.5 ± 1	6.4 ± 0.2	كويكبات حزامية من النوع G ؛ متعددة	^{[ 110 ]}
بينور 54598	99 +3 −3.5	1.119	قنطور	^{[ 155 ]}^{[ 156 ]}
شيرون 2060 أو 95P	98 ± 17		قنطور ؛ له حلقات	^{[ 157 ]}
هيبي 6	97.5 ± 1.5	12.4 ± 2.4	كويكبات الحزام من النوع S	^{[ 110 ]}
لاريسا نبتون السابع	97 ± 3	≈ 4.2	قمر نبتون	^{[ 158 ]} ·^[^م^]^[²⁷^]
أورسولا 375	96.8 ± 1.3	8.4 ± 5.3	كويكبات الحزام من النوع ج	^{[ 160 ]} ·^[¹⁵⁰^]
يوجينيا 45	94 ± 1	5.8 ± 0.1	كويكبات الحزام من النوع F ؛ ثلاثية	^{[ 110 ]}
هيرميون ١٢١	94 ± 3	5.0 ± 0.3	كويكب من النوع C في الحزام الخارجي ؛ ثنائي	^{[ 161 ]} ·^[¹⁵⁰^]
دافني 41	94 ± 7	6.1 ± 0.9	كويكب حزام من النوع C ؛ ثنائي	^{[ 110 ]}
أورورا 94	93.8 ± 3.6	6.2 ± 3.6	كويكبات الحزام من النوع ج	^{[ 162 ]} ·^[¹⁵⁰^]
بيرثا 154	93.4 ± 0.9	9.2 ± 5.2	كويكبات الحزام من النوع ج	^{[ 150 ]} ·^[¹⁵⁰^]
1995 SM ₅₅ 24835	93.4 ± 0.9		عائلة كوبيوانو ، هاوميا	^{[ 163 ]}
قمر عام 532037 تشيمينيغاوا	93 ± 13		قمر عام 532037 تشيمينيغاوا	^{[ 83 ]}
يانوس زحل العاشر	89.5 ± 1.4	1.898 ± 0.001	قمر زحل	^{[ 75 ]} ·^[⁷⁵^]
تيهارونهياواكو 88611	89 +16 −18	2.44 ± 0.03	كيوبوانو ؛ ثنائي	^{[ 81 ]} ·^[¹⁶⁴^]
إيجل 96	88.9 ± 0.8	6.4 ± 6.3	كويكبات الحزام من النوع T	^{[ 149 ]} ·^[¹⁵⁰^]
غالاتيا نبتون السادس	88 ± 4	2.12 ± 0.08	قمر نبتون	^{[ 158 ]} ·^[¹⁶⁵^]^[²⁷^]
S/2015 (136472) 1 (MK2)	87.5	4.939	قمر ماكيماكي	^{[ 166 ]}^{[ 167 ]}
فورسيس سيتو 1	87 +8 −9	≈ 1.67	ثانوي من 65489 سيتو	^{[ 151 ]} ·^[¹⁵¹^]
بالما 372	86.8 ± 1.4	5.2 ± 0.6	كويكبات الحزام من النوع ب	^{[ 168 ]} ·^[¹⁵⁰^]
ميتيس 9	86.5 ± 1	8.0 ± 1.9	كويكبات الحزام من النوع S	^{[ 149 ]} ·^[¹⁵⁰^]
ألاودا 702	86 ± 28	6.06 ± 0.36	كويكب حزام من النوع C ؛ ثنائي	^{[ 168 ]} ·^[¹⁶⁹^]
هيلدا 153	85.3 ± 1.6		كويكب الحزام الخارجي؛ هيلداس	^{[ 152 ]}
هيماليا جوبيتر السادس	85	4.2 ± 0.6	قمر المشتري	^{[ 5 ]} ·^[¹⁷⁰^]
فريا 76	84.2 ± 1.0	2.0 ± 4.2	كويكبات الحزام الخارجي من النوع P / النوع X	^{[ 160 ]} ·^[¹⁵⁰^]
أمالثيا جوبيتر الخامس	83.45 ± 2.4	2.08 ± 0.15	قمر المشتري	^{[ 171 ]} ·^[¹⁷²^]^[²⁷^]
أجاممنون 911	83.3 ± 2.0		حصان طروادة جوبيتر ( L ₄ ) من النوع D	^{[ 152 ]}
إلبس 59	82.6 ± 2.3	3 ± 0.5	كويكبات الحزام من النوع CP / النوع B	^{[ 149 ]} ·^[¹⁵⁰^]
إليونورا 354	82.5 ± 1.5	7.5 ± 2.7	كويكبات الحزام من النوع أ	^{[ 110 ]}
Weywot Quaoar I	≈ 82.5	2.4 +1.2 −1.1	قمر كواوار	^{[ 63 ]}
نيميسيس 128	81.5 ± 2.5	3.4 ± 1.7	كويكبات الحزام من النوع ج	^{[ 110 ]}
بوك أورانوس الخامس عشر	81 ± 2	1.91	قمر أورانوس	^{[ 173 ]}^{[ 174 ]}
2002 KW ₁₄ 307251	80 +18 −20	≈ 30	كيوبوانو	^{[ 81 ]}
سيكوراكس أورانوس السابع عشر	78.5 +11.5 −7.5		قمر أورانوس	^{[ 175 ]}
Io 85	77.4 ± 1.9	2.6 ± 1.5	كويكبات الحزام من النوع FC / النوع B	^{[ 152 ]} ·^[¹⁵⁰^]
مينيرفا 93	77.08 ± 0.65	3.5 ± 0.4	كويكبات الحزام من النوع ج ؛ ثلاثية	^{[ 149 ]} ·^[¹⁵⁰^]
ألكسندرا 54	77.07 ± 0.32	6.2 ± 3.5	كويكبات الحزام من النوع ج	^{[ 149 ]} ·^[¹⁵⁰^]
ليتيتيا 39	77 ± 2	4.7 ± 1.1	كويكبات الحزام من النوع S	^{[ 150 ]} ·^[¹⁵⁰^]
نيموسا 51	75 ± 1.5	3.9 ± 1.6	كويكبات الحزام من النوع G	^{[ 110 ]}
كاليوبي 22	75 ± 2.5	7.7 ± 0.4	كويكبات الحزام من النوع M ؛ ثنائي	^{[ 110 ]}
ديسبينا نبتون الخامس	75 ± 3	0.71	قمر نبتون	^{[ 27 ]}^{[ 176 ]}
ناماكا هاوميا الثاني	75 ± 25	1.18 ± 0.25	قمر هاوميا	^{[ 177 ]} ·^[⁵¹^]
مانوي 385446	≈ 75	≈ 1.41	KBO الرنان (4:7) ؛ ثنائي	^{[ 178 ]} ·^[¹⁷⁸^]
باليس 49	≈ 74.9	4.2 ± 2.2	كويكبات الحزام من النوع ج	^{[ 152 ]} ·^[¹⁵⁰^]
بارثينوب 11	74.5 ± 1	5.5 ± 0.4	كويكبات الحزام من النوع S	^{[ 110 ]}
أريثوسا 95	74.0 ± 2.4		كويكبات الحزام من النوع ج	^{[ 162 ]}
بولكوفا 762	73.7 ± 0.4	1.4 ± 0.1	كويكب حزام من النوع F ؛ ثنائي	^{[ 149 ]} ·^[¹⁷⁹^]
فلورا 8	73 ± 1	4.0 ± 1.6	كويكبات الحزام من النوع S	^{[ 110 ]}
إينو 173	72.5 ± 1.5	2.2 ± 1.3	كويكبات الحزام من النوع Xc	^{[ 110 ]}
أديونا 145	72 ± 1.5	2.4 ± 0.3	كويكبات الحزام من النوع Xc	^{[ 110 ]}
إيرين 14	72 ± 1	2.9 ± 1.9	كويكبات الحزام من النوع S	^{[ 160 ]} ·^[¹⁵⁰^]
Gīòʼé àHú GīkúnɁʼhòmdímà I	71 ± 4		الثانوية 229762 Gīkúnāʼhòmdímà	^{[ 180 ]}
أغلايا 47	71 ± 4	3.2 ± 1.7	كويكبات الحزام من النوع ج	^{[ 150 ]} ·^[¹⁵⁰^]
ميلبوميني 18	70.5 ± 1	4.5 ± 0.9	كويكبات الحزام من النوع S	^{[ 110 ]}
لامبرتا 187	70.5 ± 1	1.9 ± 0.3	نوع الكويكبات الحزامية Ch	^{[ 110 ]}
باتروكلس 617	70.2 ± 0.4	1.36 ± 0.11	_حصان طروادة جوبيتر ( L5 ) من النوع P ؛ ثنائي	^{[ 149 ]} ·^[¹⁵⁰^]
جوليا 89	70 ± 1.4	4.3 ± 3.2	كويكبات الحزام من النوع S	^{[ 110 ]}
تايفون 42355	69 ± 4.5	0.87 ± 0.03	مرصد ديناميكا الشمس الرنيني (7:10)؛ ثنائي	^{[ 155 ]} ·^[¹⁸¹^]
ǂKá̦gára 469705	69 ± 12	1.29 ± 0.07	بارد كلاسيكي KBO ؛ ثنائي	^{[ 182 ]}
ماساليا 20	67.8 ± 1.8	5 ± 1.04	كويكبات الحزام من النوع S	^{[ 168 ]} ·^[¹⁵⁰^]
بورتيا أورانوس الثاني عشر	67.6 ± 4		قمر أورانوس	^{[ 5 ]}
إيما 283	66.2 ± 0.1	1.38 ± 0.03	كويكبات الحزام من النوع X ؛ ثنائي	^{[ 149 ]} ·^[¹⁵⁰^]
باها ليمبو 1	66 ± 4	0.746 ± 0.001	قمر ليمبو 47171	^{[ 140 ]} ·^[¹⁸³^]
لوسينا 146	65.9 ±؟		كويكبات الحزام من النوع ج	^{[ 184 ]}
ساويسكيرا تيهارونهياواكو 1	66 +12 −13		الثانوية 88611 تيهارونهيواكو	^{[ 81 ]}
أخيل 588	65.0 ± 0.3		حصان طروادة للمشتري ( L ₄ ) من النوع DU	^{[ 149 ]}
بانوبايا 70	64.0 ± 0.4	4.33 ± 1.09	كويكبات الحزام من النوع ج	^{[ 149 ]} ·^[¹⁵⁰^]
ثول 279	63.3 ± 1.8		كويكب من النوع د في الحزام الخارجي	^{[ 152 ]}
بوراسي 66652	63 +12 −26	3.433 ± 0.027	كيوبوانو ؛ ثنائي	^{[ 81 ]} ·^[¹⁸⁵^]
ألبيون 15760	≈ 62.5 ^{[ i ]}		TNO، أول جسم كوري تم اكتشافه
هيستيا 46	62.1 ± 1.7	3.5	كويكبات الحزام من النوع P / النوع Xc	^{[ 152 ]} ·^[¹⁸⁶^]
ليتو 68	61.3 ± 1.6	3.28 ± 1.9	كويكبات الحزام من النوع S	^{[ 149 ]} ·^[¹⁵⁰^]
ǃHãunu ǂKá̦gára I	61 ± 9	0.89 ± 0.05	ثانوي من 469705 ǂKá̦gára	^{[ 187 ]}
أوندينا 92	60.46 ± 0.85	4.43 ± 0.25	كويكبات الحزام من النوع X	^{[ 160 ]} ·^[¹⁵⁰^]
بيلونا 28	60.45 ± 1.90	2.62 ± 0.15	كويكبات الحزام من النوع S	^{[ 188 ]} ·^[¹⁵⁰^]
ديانا 78	60.30 ± 1.35	1.27 ± 0.13	كويكبات الحزام من النوع ج	^{[ 189 ]} ·^[¹⁵⁰^]
أنشيسيس 1173	60.2 ± 1.5		حصان طروادة المشتري ( L ₅ ) من النوع P	^{[ 160 ]}
برناردينيلي-بيرنشتاين C/2014 الأمم المتحدة ₂₇₁	60 ± 7		مذنب	^{[ 190 ]}
غالاتيا 74	59.4 ± 1.4	6.13 ± 5.36	كويكبات الحزام من النوع ج	^{[ 191 ]} ·^[¹⁵⁰^]
ديفوبوس 1867	59.1 ± 0.8		حصان طروادة جوبيتر ( L ₅ ) من النوع D	^{[ 192 ]}
أنياس 1172	59.01 ± 0.40		حصان طروادة جوبيتر ( L ₅ ) من النوع D	^{[ 193 ]}
كليوباترا 216	59 ± 1	3.0 ± 0.3	كويكبات الحزام من النوع M ؛ ثلاثية	^{[ 110 ]}
أثامانتيس 230	59 ± 1	2.3 ± 1.1	كويكبات الحزام من النوع S	^{[ 110 ]}
ديوميدس 1437	58.89 ± 0.59		حصان طروادة جوبيتر ( L ₄ ) من النوع D	^{[ 194 ]}
تيربسيكوري 81	58.9 ± 0.4	6.19 ± 5.31	كويكبات الحزام من النوع ج	^{[ 195 ]} ·^[¹⁵⁰^]
إبيميثيوس زحل الحادي عشر	58.1 ± 1.8	0.5266 ± 0.0006	قمر زحل	^{[ 75 ]} ·^[⁷⁵^]
فيكتوريا ١٢	58 ± 1	2.7 ± 1.3	كويكبات الحزام من النوع S	^{[ 110 ]}
سيرسي 34	57.7 ± 1.0	≈ 3.66 ± 0.03	كويكبات الحزام من النوع ج	^{[ 149 ]} ·^[¹⁵⁰^]
ليدا 38	57.7 ± 0.7	5.71 ± 5.47	كويكبات الحزام من النوع ج	^{[ 150 ]} ·^[¹⁵⁰^]
أوديسيوس 1143	57.3 ± 0.3		حصان طروادة جوبيتر ( L ₄ ) من النوع D	^{[ 196 ]}
ألكاثوس 2241	56.8 ± 0.9		حصان طروادة جوبيتر ( L ₅ ) من النوع D	^{[ 197 ]}
ميليت 56	56.62 ± 0.85	4.61	كويكبات الحزام من النوع P	^{[ 152 ]} ·^[¹⁵⁰^]
منيموسين 57	56.3 ± 1.4	≈ 12.6 ± 2.4	كويكبات الحزام من النوع S	^{[ 198 ]} ·^[¹⁵⁰^]
نيستور 659	56.2 ± 0.9		حصان طروادة المشتري ( L ₄ ) من النوع XC	^{[ 199 ]}
هارمونيا 40	55.6 ± 0.2		كويكبات الحزام من النوع S	^{[ 200 ]}
هيسبيريا 69	55 ± 8	5.86 ± 1.18	كويكبات الحزام من النوع M	^{[ 152 ]} ·^[¹⁵⁰^]^[²⁰¹^]
يوتربي 27	54.9 ± 0.8	1.67 ± 1.01	كويكبات الحزام من النوع S	^{[ 160 ]} ·^[¹⁵⁰^]
أنتيلوخوس 1583	54.4 ± 0.3		حصان طروادة جوبيتر ( L ₄ ) من النوع D	^{[ 149 ]}
ثوروندور مانوي الأول	54	0.5	رقم ثانوي لـ 385446 مانوي	^{[ 178 ]} ·^[¹⁷⁸^]
ثاليا 23	53.8 ± 1.1	1.96 ± 0.09	كويكبات الحزام من النوع S	^{[ 202 ]} ·^[¹⁵⁰^]
إراتو 62	53.5 ± 0.3		كويكبات الحزام من النوع BU / النوع Ch	^{[ 203 ]}
أستريا 5	53.3 ± 1.6	2.9	كويكبات الحزام من النوع S	^{[ 204 ]} ·^[¹⁸⁶^]
بابو بوراسي الأول	52 +10 −21		ثانوي من 66652 بوراسيسي	^{[ 81 ]}
إيوس 221	51.76 ± 2.8	≈ 5.87 ± 0.34	كويكبات الحزام من النوع S / النوع K	^{[ 150 ]} ·^[¹⁵⁰^]
إيجينا 91	51.7 ± 0.2		كويكبات الحزام من النوع ج	^{[ 205 ]}
ليوكوثيا 35	51.5 ± 0.6		كويكبات الحزام من النوع ج	^{[ 206 ]}
مينويتيوس باتروكلس الأول	51.4 ± 0.25		ثانوي من 617 باتروكلس	^{[ 207 ]}
إيزيس 42	51.4 ± 1.4	1.58 ± 0.52	كويكبات الحزام من النوع S	^{[ 150 ]} ·^[¹⁵⁰^]
كلوثو 97	50.4 ± 0.3	1.33 ± 0.13	كويكبات الحزام من النوع M	^{[ 149 ]} ·^[¹⁵⁰^]
ترويلوس 1208	50.3 ± 0.5		حصان طروادة جوبيتر ( L ₅ ) من نوع FCU	^{[ 208 ]}

من 20 إلى 49 كم

تتضمن هذه القائمة أمثلة قليلة، إذ يوجد حوالي 589 كويكبًا في حزام الكويكبات بنصف قطر يتراوح بين 20 و49 كيلومترًا. ^{[ 209 ]} ولا يزال هناك آلاف الأجسام بهذا الحجم في المنطقة ما وراء نبتون بانتظار الاكتشاف. عدد الأرقام لا يدل على دقة الأرقام المعنوية . ينتقل الجدول من × 10¹⁸ كجم إلى × 10¹⁵ كجم ( Eg ). تم افتراض معظم قيم كتلة الكويكبات.^{[ 150 ]}^{[ 210 ]}

الجسم ^{[ ملاحظة 1 ]}	نصف القطر ^{[ ملاحظة 2 ]} ( كم )	الكتلة ( 10-15 كجم )	النوع - ملاحظات	المراجع ^{[ ملاحظة 5 ]} ر · م
أستيروب 233	49.8 ± 0.6		كويكبات الحزام من النوع T / النوع K	^{[ 211 ]}
فولوس 5145	49.5 +7.5 −7		قنطور	^{[ 155 ]}
ثيبي جوبيتر الرابع عشر	49 ± 2		قمر المشتري	^{[ 171 ]}
لوتيتيا 21	49 ± 1	1700 ± 20	كويكبات الحزام من النوع M	^{[ 110 ]}
كاليپسو 53	49 ± 13	≈ 5630 ± 5000	كويكبات الحزام من النوع XC	^{[ 212 ]} ·^[¹⁵⁰^]
نوتبورغا 626	48.4 ± 2.3		كويكبات الحزام من النوع XC	^{[ 150 ]}
بروسربينا 26	47.4 ± 0.8	748 ± 895	كويكبات الحزام من النوع S	^{[ 213 ]} ·^[¹⁵⁰^]
جولييت أورانوس الحادي عشر	46.8 ± 4		قمر أورانوس	^{[ 5 ]}
يورانيا 30	44 ± 1	1300 ± 900	كويكبات الحزام من النوع S	^{[ 110 ]}
أوسونيا 63	46.5 ± 1.5	1200 ± 200	كويكبات الحزام من النوع S	^{[ 110 ]}
بياتريكس 83	44.8 ± 1.3		كويكبات الحزام من النوع X	^{[ 149 ]}
كونكورديا 58	44.81 ± 0.42		كويكبات الحزام من النوع ج	^{[ 149 ]}
إيكيدنا تايفون الأول	44.5 ± 3		قمر تيفون 42355	^{[ 181 ]}
أوتوميدون 2920	44.29 ± 0.90		حصان طروادة جوبيتر ( L ₄ ) من النوع D	^{[ 214 ]}
أنتيوب 90	43.9 ± 0.5	828 ± 22	كويكب حزام من النوع C ؛ ثنائي	^{[ 215 ]} ·^[²¹⁵^]
بروميثيوس زحل السادس عشر	43.1 ± 2.7	159.5 ± 1.5	قمر زحل	^{[ 75 ]} ·^[⁷⁵^]
داناي 61	43.0 ± 1.1	2890 ± 2780	كويكبات الحزام من النوع S	^{[ 216 ]} ·^[¹⁵⁰^]
ثيتيس 17	42.4 ± 1.0	1200	كويكبات الحزام من النوع S	^{[ 217 ]} ·^[²¹⁰^]
باندورا 55	42.4 ± 1.3		كويكبات الحزام من النوع M	^{[ 218 ]}
هوينا 379	42.39 ± 0.78	383 ± 19	كويكبات الحزام من النوع B / النوع C ؛ ثنائي	^{[ 219 ]} ·^[²²⁰^]
فرجينيا 50	42.04 ± 0.12	2310 ± 700	كويكبات الحزام من النوع X / النوع Ch	^{[ 221 ]} ·^[¹⁵⁰^]
فيرونيا 72	42.0 ± 2.0	≈ 3320 ± 8490	كويكبات الحزام من نوع TDG	^{[ 150 ]} ·^[¹⁵⁰^]
S/2000 (90) 1 أنتيوب 1	41.9 ± 0.5		ثانوي من 90 أنتيوب	^{[ 215 ]}
بوليداماس 4348	41.07 ± 0.31		حصان طروادة جوبيتر ( L ₅ ) من النوع C	^{[ 222 ]}
الشعارات 58534	41 ± 9	458 ± 6.9	كيوبوانو ؛ ثنائي	^{[ 223 ]} ·^[²²³^]
باندورا زحل السابع عشر	40.7 ± 1.5	137.1 ± 1.9	قمر زحل	^{[ 75 ]} ·^[⁷⁵^]
ثالاسا نبتون 4	40.7 ± 2.8		قمر نبتون	^{[ 158 ]}
نيوبي 71	40.4 ± 0.4		كويكبات الحزام من النوع S	^{[ 160 ]}
بومونا 32	40.4 ± 0.8		كويكبات الحزام من النوع S	^{[ 224 ]}
بليندا أورانوس الرابع عشر	40.3 ± 8		قمر أورانوس	^{[ 5 ]}
إيلارا جوبيتر السابع	40.0 ± 1.7		قمر المشتري	^{[ 225 ]}
كريسيدا أورانوس التاسع	39.8 ± 2		قمر أورانوس	^{[ 5 ]}
أميكوس 55576	38.2 ± 6.2		قنطور	^{[ 119 ]}
هايلونوم 10370	37 ± 8		قنطور	^{[ 226 ]}
سوكوس 3708	37.83 ± 0.40		حصان طروادة جوبيتر ( L ₅ ) من النوع C	^{[ 149 ]}
نايسا 44	37.83 ± 0.37		كويكبات الحزام من النوع E	^{[ 160 ]}
روزاليند أورانوس الثالث عشر	36 ± 6		قمر أورانوس	^{[ 5 ]}
مايو 66	35.90 ± 0.46		كويكبات الحزام من النوع ج	^{[ 160 ]}
أريادني 43	35.67 ± 0.63	≈ 1210 ± 220	كويكبات الحزام من النوع S	^{[ 227 ]} ·^[¹⁵⁰^]
إيفيجينيا 112	35.54 ± 0.26	≈ 1970 ± 6780	كويكبات الحزام من النوع ج	^{[ 150 ]} ·^[¹⁵⁰^]
شيانغليو جونجونج آي	≈ 35 ± 15		قمر عام 225088 غونغ غونغ
السد 99	33.68 ± 0.21		كويكبات الحزام من النوع ج	^{[ 228 ]}
إيكلس 60558 أو 174P	32.3 ± 0.8		قنطور	^{[ 155 ]}
ديسديمونا أورانوس العاشر	32 ± 4		قمر أورانوس	^{[ 5 ]}
يوريباتس 3548	31.94 ± 0.15		حصان طروادة جوبيتر ( L ₄ ) من النوع CP	^{[ 149 ]}
يورينوم 79	31.74 ± 0.48		كويكبات الحزام من النوع S	^{[ 229 ]}
يوريديك 75	31.19 ± 0.80		كويكبات الحزام من النوع M	^{[ 230 ]}
فوكايا 25	30.53 ± 1.23	599 ± 60	كويكبات الحزام من النوع S	^{[ 149 ]} ·^[¹⁵⁰^]
نايد نبتون الثالث	30.2 ± 3.2		قمر نبتون	^{[ 158 ]}
شواسمان - واخمان 1 29P	30.2 ± 3.7		مذنب	^{[ 231 ]}
أنجلينا 64	29.15 ± 0.54		كويكبات الحزام من النوع E	^{[ 232 ]}
باسيفاي جوبيتر الثامن	28.9 ± 0.4		قمر المشتري	^{[ 225 ]}
ألكمني 82	28.81 ± 0.36		كويكبات الحزام من النوع S	^{[ 233 ]}
نيسوس 7066	28.5 ± 8.5		قنطور	^{[ 155 ]}
بولانا 142	27.41 ± 0.14		كويكبات الحزام من النوع F	^{[ 234 ]}
بيانكا أورانوس الثامن	27 ± 2		قمر أورانوس	^{[ 5 ]}
ماتيلد 253	26.4	103.3 ± 4.4	كويكبات الحزام من النوع ج	^{[ 235 ]} ·^[²³⁶^]
هيدالغو 944	26.2 ± 1.8		قنطور	^{[ 160 ]}
أوروس 21900	25.40 ± 0.40		حصان طروادة جوبيتر ( L ₄ ) من النوع C / النوع D	^{[ 149 ]}
أمالثيا 113	25.07 ± 0.63		كويكب حزام من النوع S ؛ ثنائي	^{[ 149 ]}
بروسبيرو أورانوس الثامن عشر	≈ 25		قمر أورانوس	^{[ 5 ]}
سيتيبوس أورانوس التاسع عشر	≈ 24		قمر أورانوس	^{[ 5 ]}
كارمي جوبيتر الحادي عشر	23.35 ± 0.45		قمر المشتري	^{[ 225 ]}
كليتيا 73	22.30 ± 0.47		كويكبات الحزام من النوع S	^{[ 237 ]}
إيكو 60	21.61 ± 0.29	315 ± 32	كويكبات الحزام من النوع S	^{[ 238 ]} ·^[¹⁵⁰^]
ميتيس جوبيتر السادس عشر	21.5 ± 2	≈ 119.893	قمر المشتري	^{[ 171 ]} ·^[²³⁹^]
أوفيليا أورانوس السابع	21.4 ± 4		قمر أورانوس	^{[ 5 ]}
ليسيثيا جوبيتر العاشر	21.1 ± 0.35		قمر المشتري	^{[ 225 ]}
كاليبان أورانوس السادس عشر	21 +10 −6		قمر أورانوس	^{[ 175 ]}
كورديليا أورانوس السادس	20.1 ± 3		قمر أورانوس	^{[ 5 ]}

من 1 إلى 19 كم

تحتوي هذه القائمة على بعض الأمثلة لأجرام النظام الشمسي التي يتراوح نصف قطرها بين 1 و19 كيلومترًا. وهذا حجم شائع للكويكبات والمذنبات والأقمار غير المنتظمة.

الجسم ^{[ ملاحظة 1 ]}	نصف القطر ^{[ ملاحظة 2 ]} ( كم )	الكتلة ( 10-15 كجم )	النوع - ملاحظات	المراجع ^{[ ملاحظة 5 ]} ر · م
أوردا 167	19.968 ± 0.132		كويكبات الحزام من النوع S	^{[ 240 ]}
هيدرا بلوتو 3	19.65	48 ± 42	قمر بلوتو	^{[ 241 ]} ·^[²⁴²^]
سيارناق زحل التاسع والعشرون	19.65 ± 2.95		قمر زحل	^{[ 225 ]}
كورونيس 158	19.513 ± 0.231		كويكبات الحزام من النوع S	^{[ 243 ]}
نيكس بلوتو 2	19.017	45 ± 40	قمر بلوتو	^{[ 241 ]} ·^[²⁴²^]
غانيميد 1036	18.84 ± 0.20	≈ 167 ± 318	كويكب أمور من النوع S	^{[ 149 ]} ·^[¹⁵⁰^]
أوكيرهوي 52872	18 ± 0.6		قنطور	^[244]
HeleneSaturn XII	17.6±0.4		moon of Saturn; Dione trojan (L₄)	^[75]
SinopeJupiter IX	17.5±0.3		moon of Jupiter	^[225]
HippocampNeptune XIV	17.4±1	≈ 50	moon of Neptune	^[158] ·^[158]
Leucus11351	17.08±0.32		Jupiter trojan (L₄) type D	^[149]
StephanoUranus XX	≈ 16		moon of Uranus	^[5]
Arrokoth486958	15.85±0.25		cubewano; contact binary	^[245]
Ida243	15.7	42±6	belt asteroid type S; binary	^[246] ·^[247]
AtlasSaturn XV	15.1±0.9	6.6	moon of Saturn	^[75] ·^[75]
Great cometC/1811 F1	15 - 20		comet	^[248]
AnankeJupiter XII	14.55±0.3		moon of Jupiter	^[225]
AlbiorixSaturn XXVI	14.3±2.7		moon of Saturn	^[225]
LinusKalliope I	14±1	≈ 60	asteroid moon of 22 Kalliope	^[249] ·^[250]
Dioretsa20461	14±3		centaur; damocloid	^[251]
PanSaturn XVIII	13.7±0.3	4.30±0.22	moon of Saturn	^[252] ·^[252]
PerditaUranus XXV	13±1		moon of Uranus	^[5]
TelestoSaturn XIII	12.4±0.4		moon of Saturn; Tethys trojan (L₄)	^[75]
MabUranus XXVI	12±1		moon of Uranus	^[5]
PhobosMars I	11.1±0.15	10.659	moon of Mars	^[253] ·^[254]
PaaliaqSaturn XX	≈ 11		moon of Saturn	^[5]
FranciscoUranus XXII	≈ 11		moon of Uranus	^[5]
ليدا جوبيتر الثالث عشر	10.75 ± 0.85		قمر المشتري	^{[ 225 ]}
كاليبسو زحل الرابع عشر	10.7 ± 0.7		أقمار زحل؛ طروادة تيثيس ( L ₅ )	^{[ 75 ]}
بوليميل 15094	10.548 ± 0.068		حصان طروادة المشتري ( L ₄ ) من النوع P	^{[ 152 ]}
كيوبيد أورانوس السابع والعشرون	9 ± 1		قمر أورانوس	^{[ 5 ]}
يمير زحل التاسع عشر	≈ 9		قمر زحل	^{[ 5 ]}
ترينكولو أورانوس الحادي والعشرون	≈ 9		قمر أورانوس	^{[ 5 ]}
إيروس 433	8.42 ± 0.02	6.687 ± 0.003	كويكب أمور من النوع S	^{[ 255 ]} ·^[²⁵⁵^]
أدراستيا جوبيتر الخامس عشر	8.2 ± 2		قمر المشتري	^{[ 5 ]}
كيفيوك زحل الرابع والعشرون	≈ 8		قمر زحل	^{[ 5 ]}
تارفوس زحل الحادي والعشرون	≈ 7.5		قمر زحل	^{[ 5 ]}
كيربيروس بلوتو 4	≈ 6.333	16 ± 9	قمر بلوتو	^{[ 256 ]} ·^[²⁵⁷^]
جاسبرا 951	6.266	20-30	كويكبات الحزام من النوع S	^{[ 258 ]} ·^[²⁵⁹^]
ديموس مارس 2	6.27 ± 0.07	1.51	قمر المريخ	^{[ 260 ]} ·^[²⁶⁰^]
سكاماندريوس هيكتور الأول	6 ± 1.5		قمر كويكب تابع لـ 624 هيكتور	^{[ 143 ]}
إيجراق زحل الثاني والعشرون	≈ 6		قمر زحل	^{[ 5 ]}
تسوتشينشان–أطلس C/2023 A3	<5.9 ± 0.2		مذنب	^{[ 261 ]}
مذنب هالي 1P	5.75	0.22	مذنب	^{[ 262 ]} ·^[²⁶³^]
ستيكس بلوتو الخامس	≈ 5.5	≈ 7.65	قمر بلوتو	^{[ 256 ]} ·^[²⁵⁷^]
رومولوس سيلفيا الأول	5.4 ± 2.8		قمر الكويكب 87 سيلفيا	^{[ 264 ]}
ماسورسكي 2685	5.372 ± 0.085		كويكبات الحزام من النوع S	^{[ 265 ]}
إريابوس زحل الثامن والعشرون	≈ 5		قمر زحل	^{[ 5 ]}
كاليرهوي جوبيتر السابع عشر	4.8 ± 0.65		قمر المشتري	^{[ 225 ]}
أليكسيليوس كليوباترا الأولى	4.45 ± 0.8		قمر كويكب 216 كليوباترا	^{[ 266 ]}
Esclangona1509	4.085±0.3		inner belt asteroid type S; binary	^[267]
ThemistoJupiter XVIII	≈ 4		moon of Jupiter	^[5]
DaphnisSaturn XXXV	3.8±0.8	0.077±0.015	moon of Saturn	^[75] ·^[75]
Petit-PrinceEugenia I	3.5±1		asteroid moon of 45 Eugenia	^[268]
PraxidikeJupiter XXVII	3.5±0.35		moon of Jupiter	^[225]
BestlaSaturn XXXIX	≈ 3.5		moon of Saturn	^[5]
RemusSylvia II	≈ 3.5		asteroid moon of 87 Sylvia	^[264]
KalykeJupiter XXIII	3.45±0.65		moon of Jupiter	^[225]
CleoseleneKleopatra II	3.45±0.8		asteroid moon of 216 Kleopatra	^[266]
Moon of 31 Euphrosyne	3.35±1.2		asteroid moon of 31 Euphrosyne	^[269]
Tempel 19P	3±0.1		Jupiter-family comet; Deep Impact flyby and impacted	^[270]
Ireland5029	3		belt asteroid	^[271]
Phaethon3200	2.9		Apollo asteroid type F	^[272]
1999 JM₈53319	2.7±0.6		Apollo asteroid type X	^[273]
Borrelly19P	2.66		Jupiter-family comet	^[274]
Šteins2867	2.58±0.084		belt asteroid type E	^[149]
Atira163693	2.4±0.25		Atira asteroid type S; binary	^[275]
Annefrank5535	2.4		belt asteroid type S	^[276]
Balam3749	2.33±0.11	0.51±0.02	belt asteroid type S; trinary	^[277] ·^[278]
PalleneSaturn XXXIII	2.22±0.07		moon of Saturn	^[279]
Florence3122	2.201±0.015	0.079±0.002	Amor asteroid type S; trinary	^[162] ·^[280]
Wild 281P	2.133		Jupiter family comet	^[281]
Litva2577	2.115		Mars-crosser type EU; trinary	^[282]
Churyumov–Gerasimenko67P	2	0.00998	Jupiter-family comet	^[283] ·^[284]
Donaldjohanson52246	1.948±0.007		belt asteroid type C	^[285]
Camelot9500	1.9		belt asteroid	^[286]
Cuno4183	1.826±0.051		Apollo asteroid type S/type Q	^[287]
1986 DA6178	1.575		Amor asteroid type M	^[288]
Pichi üñëmAlauda I	1.55±0.45		asteroid moon of 702 Alauda	^[289]
Toutatis4179	1.516	0.0505	Apollo asteroid type S	^[290] ·^[290]
Kaʻepaokaʻāwela514017	1.5		Jupiter trojan	^[291]
MethoneSaturn XXXII	1.45±0.03		moon of Saturn	^[279]
CarpoJupiter XLVI	1.44		Moon of Jupiter
Gault6478	1.4+0.2−0.1		Phocaea asteroid type S	^[292]
1998 QE₂285263	1.375		Amor asteroid type S; binary	^[293]
PolydeucesSaturn XXXIV	1.3±0.4		moon of Saturn; Dione trojan (L₅)	^[75]
2001 SN₂₆₃153591	1.315±0.2	0.00951±0.00013	Amor asteroid type C; trinary	^[294] ·^[295]
S/2003 (1509) 1Moon of 1509 Esclangona	1.285		asteroid moon of 1509 Esclangona	^[296]
APL132524	≈ 1.25		belt asteroid type S	^[297]
Camillo3752	1.153±0.044		Apollo asteroid type S	^[162]
Cruithne3753	1.036±0.053		Aten asteroid type Q; quasi-satellite of Earth	^[298]
1996 HW18567	1.01		Amor asteroid	^[299]

Below 1 km

This list contains examples of objects below 1 km in radius. That means that irregular bodies can have a longer chord in some directions, hence the mean radius averages out. In the asteroid belt alone there are estimated to be between 1.1 and 1.9 million objects with a radius above 0.5 km,^[300] many of which are in the range 0.5–1.0 km. Countless more have a radius below 0.5 km. Very few objects in this size range have been explored or even imaged. The exceptions are objects that have been visited by a probe, or have passed close enough to Earth to be imaged. Radius is by mean geometric radius. Number of digits not an endorsement of significant figures. Mass scale shifts from × 10¹⁵ to 10⁹ kg, which is equivalent to one billion kg or 10¹² grams (Teragram – Tg). Currently most of the objects of mass between 10⁹kg to 10¹²kg (less than 1000 teragrams (Tg)) listed here are near-Earth asteroids (NEAs). The Aten asteroid1994 WR₁₂ has less mass than the Great Pyramid of Giza, 5.9 × 10⁹ kg. For more about very small objects in the Solar System, see meteoroid, micrometeoroid, cosmic dust, and interplanetary dust cloud. (See also Visited/imaged bodies.)

Object	Radius^{[note 2]}(m)	Mass(10⁹ kg)	Type – notes	Refs^{[note 5]}r ·M
Ra-Shalom2100	990±25		Aten asteroid type C	^[160]
Geographos1620	980±30		Apollo asteroid type S	^[149]
Midas1981	975±35		Apollo asteroid type S	^[160]
Mithra4486	924.5±11		Apollo asteroid type S	^[162]
2006 VW₁₃₉300163	900±0.1		Active asteroid	^[301]
1998 OH12538	831.5±164.5		Apollo asteroid type S	^[162]
Tantalus2102	824.5±22.5		Apollo asteroid type Q	^[302]
Braille9969	820		Mars-crosser type Q	^[303]
2005 GO₂₁308242	780		Aten asteroid type S	^[304]
Apollo1862	≈ 750		Apollo asteroid type Q	^[305]
1999 JD₆85989	731±10.5		Aten asteroid type K; contact binary	^[306]
Icarus1566	730		Apollo asteroid type S	^[307]
DactylIda I	700		asteroid moon of 243 Ida	^[308]
Castalia4769	700		Apollo asteroid type S; contact binary	^[309]
2007 PA₈214869	675±70		Apollo asteroid type Q	^[310]
Moshup66391	658.5±20	2490±54	Aten asteroid type S; binary	^[311] ·^[312]
1950 DA29075	653	≈ 2000	Apollo asteroid type S	^[313] ·^[314]
2006 HY₅₁394130	609±114		Apollo asteroid	^[315]
Hartley 2103P	570±80	≈ 300	Jupiter-family comet	^[316] ·^[316]
2003 SD₂₂₀163899	515		Aten asteroid type S	^[317]
Nyx3908	500±75		Amor asteroid type V	^[318]
Wikipedia274301	475		Vestian asteroid	^[319] ·^[320]
Astronautica100000	470		Hungaria asteroid type E	^[319] ·^[320]
2001 WN₅153814	466±5.5		Apollo asteroid	^[321]
2017 YE5	450±25		Apollo asteroid type S; binary	^[322]
Ryugu162173	432.5±7.5	≈ 450	Apollo asteroid type Cg	^[323] ·^[324]
1997 AE₁₂162058	423.5±6.5		Amor asteroid type S	^[325]
2014 JO₂₅671294	409		Apollo asteroid type S; contact binary	^[326]
Hermes69230	400±50		Apollo asteroid type Sq	^[327]
Didymos65803	390±4	527	Apollo asteroid type Xk; binary	^[328] ·^[329]
Dinkinesh152830	369		belt asteroid type Sq	^[330]
Aten2062	365±15		Aten asteroid type S	^[149]
AegaeonSaturn LIII	330±60		moon of Saturn	^[279]
2015 TB145	325±15		Apollo asteroid type S	^[331]
2001 WR₁172034	315.5±9		Amor asteroid type S	^[332]
1994 CC136617	310±30	266±32.9	Apollo asteroid type Sq; trinary	^[333] ·^[334]
LINEAR252P	300±30		Jupiter-family comet	^[335]
Golevka6489	265±15		Apollo asteroid type Q	^[336]
ATLAS3I	260 - 374		Interstellar comet	^[337]
2000 WO₁₀₇153201	255±41.5		Aten asteroid type X	^[338]
Bennu101955	245.03±0.08	78±9	Apollo asteroid type B	^[339] ·^[340]
Torifune98943	232.5±7.5		Apollo asteroid	^[341]
2002 CU₁₁163132	230±8.5		Apollo asteroid	^[342]
SquannitMoshup I	225.5±13.5		asteroid moon of 66391 Moshup	^[312]
2014 HQ124	204.5±84		Aten asteroid type S	^[149]
2013 YP139	201±13		Apollo asteroid	^[343]
2008 EV₅341843	200±7		Aten asteroid type X/type C	^[162]
2006 DP₁₄388188	≈ 200		Apollo asteroid type S; contact binary	^[344]
1988 EG6037	199.5±1.35		Apollo asteroid type S	^[345]
2010 TK₇706765	189.5±61.5		Aten asteroid; Earth trojan (L₄)	^[346]
2006 SU₄₉292220	≈ 188.5	≈ 73	Apollo asteroid	^[347] ·^[347]
2005 YU₅₅308635	180±20		Apollo asteroid type C	^[348]
2010 SO₁₆419624	178.5±63		Apollo asteroid; co-orbital with Earth	^[343]
Itokawa25143	173	35.1±1.05	Apollo asteroid type S	^[349] ·^[349]
Nereus4660	165		Apollo asteroid	^[350]
Apophis99942	162.5±7.5	≈ 61	Aten asteroid type Sq	^[351] ·^[352]
S/2009 S 1	≈ 150		moon of Saturn	^[353]
2005 WK₄277475	142		Apollo asteroid type S	^[354]
2004 BL₈₆357439	131.5±13		Apollo asteroid type V; binary	^[355]
2007 TU24	125		Apollo asteroid type S	^[356]
Zoozve524522	≈ 118		Aten asteroid type X; co-orbital with Venus	^[357]
2011 UW₁₅₈436724	110±20		Apollo asteroid type S	^[358]
Hathor2340	105±0.015		Aten asteroid type S	^[359]
DimorphosDidymos I	85±15		asteroid moon of 65803 Didymos	^[329]
Cardea164207	81.5		Apollo asteroid; quasi-satellite of Earth	^[360]
2017 BQ6	78		Apollo asteroid type S	^[361]
1994 WR12	65		Aten asteroid	^[362]
YORP54509	61.8		Apollo asteroid type S	^[363]
2019 OK	28.5 – 165		Apollo asteroid	^[364]
Duende367943	23.75		Aten asteroid type L	^[365]
Kamoʻoalewa469219	20.5		Apollo asteroid type S; quasi-satellite of Earth	^[366]
2012 TC4	11.5		Apollo asteroid type E/type Xe	^[367]
2014 RC	≈ 11		Apollo asteroid type Sq	^[368]
1998 KY26	5.5±1		Apollo asteroid type E	^[369]
2010 RF12	≈ 3.5	≈ 0.0005	Apollo asteroid	^[370]
2011 MD	3+2−1		Apollo asteroid/Amor asteroid type S	^[371]
2020 VT4	2.5 - 5.5		Aten asteroid	^[364]
2012 KT42	2.1 - 4.7		Apollo asteroid	^[364]
2008 TC3	2.05	0.00008	Apollo asteroid type F/type M	^[372]
2023 BU	1.5		Apollo asteroid	^[373]
2015 TC25	1		Apollo asteroid type E	^[374]
2018 LA	0.8 - 2.6		Apollo asteroid	^[319] ·^[375]
2025 TF	0.6 - 1.35		Apollo asteroid	^[364]
2011 CQ1	0.5 - 1.15		Aten asteroid	^[364]
2020 CD3	0.45±0.05		Apollo asteroid	^[376]
2020 CW	0.41 - 0.9		Apollo asteroid	^[364]
2008 TS26	0.305 - 0.68		Apollo asteroid	^[377]
2015 FF415	0.25		Apollo asteroid	^[319] ·^[378]
2024 BX1	0.22		Apollo asteroid	^[379]
2025 UC11	0.205 - 0.465		Aten asteroid	^[364]
2022 WJ1	0.2 - 0.3		Apollo asteroid	^[380]
EN131090	0.1425 - 0.15	0.000000044	Apollo asteroid	^[381]

Gallery

Notes

1 2 3 4 5Radius estimated using equatorial radius and assuming body is spherical
1 2Radius has been determined by various methods, such as optical (Hubble), thermal (Spitzer), or direct imaging via spacecraft
↑The mass of Eris by itself is the difference between the mass of the system ((1.6466±0.0085)×10²² kg)^[44] and the mass of Dysnomia by itself ((8.2±5.7)×10¹⁹ kg).^[45]
1 2Radius estimated by using three radii and assuming body is spheroid
↑Calculated in Wolfram Alpha using semi axes of 1050 × 840 × 537^[50](Ellipsoid volume: 1.98395×10^9 km³)
↑Best fit physical model assuming hydrostatic equilibrium for Haumea.^[50]
1 2 3 4This value refers to the system mass
↑Mass calculated by Muñoz-Gutiérrez et al. (2019 & 2021) using Achlys's area-equivalent diameter of 772 km and predicted density of 0.87 g/cm³.^[78]^:2^[79]^:2 Muñoz-Gutiérrez et al. give the mass in terms of Earth masses (M_🜨), which can be converted into kilograms by multiplying by 5.9722×10²⁴ kg/M_🜨. This calculation does not treat Achlys as an ellipsoid (which would have a volume of $V={\frac {4}{3}}\pi abc\approx 1.85\times 10^{17}{\text{ m}}^{3}$ ), though the mass calculated from Achlys's ellipsoid volume and density ( $M=\rho V\approx 1.61\times 10^{20}{\text{ kg}}$ ) is equivalent to Muñoz-Gutiérrez et al.'s mass calculation when rounded to a single digit.
1 2 3 4 5 6 7 8 9 10 11Radius estimated from an assumed albedo
↑Using Grundy et al.'s working diameters of 361 km and 163 km, and assuming the densities of the two bodies are equal, Varda would contribute 91.6% of the system mass of (2.664±0.064)×10²⁰ kg, meaning Varda's mass is about (2.44±0.06)×10²⁰ kg.^[84]
↑very approximate figure, assuming equivalent spherical diameter of ≈600 km and density ≈2.64 g/cm³
↑A density of 0.4–0.8 g/cm³ was calculated when assuming the volume as a sphere with a radius of 210±7 km.^[124] The mass was calculated with the provided density and the assumed volume.
↑The mass estimate is based on the assumed density of 1.2 g/cm³, and a volume of 3.5 ×10⁶ km³ obtained from a detailed shape model in Stooke (1994).^[159]

1 2 3 4 5 6Name of body, including alternative names using Roman numerals to designate moons (such as "Saturn I" for Mimas), and numbers to designate minor planets
1 2 3 4 5 6 7Volumetric radius including uncertainties
↑Given as surface gravity (1 bar for gaseous planets)
↑Figures from default source Johnston's Archive—List of Known Trans-Neptunian Objects,^[76] if otherwise not mentioned in the References column
1 2 3 4 5 6Reference column specifically for radius (r) and mass (M) citations

References

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↑José María Gómez-Limón Gallardo et al. (2024) New evidence that (19521) Chaos might be a large compact binary
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↑Chen, Ying-Tung; Lykawka, Patryk Sofia; Huang, Yukun; Kavelaars, J. J.; Fraser, Wesley C.; Bannister, Michele T.; Wang, Shiang-Yu; Chang, Chan-Kao; Lehner, Matthew J. (2025-08-04), "Discovery and dynamics of a Sedna-like object with a perihelion of 66 au", Nature Astronomy, 9 (9): 1309–1316, arXiv:2508.02162, Bibcode:2025NatAs...9.1309C, doi:10.1038/s41550-025-02595-7
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1 2Johnston, Wm. Robert (20 September 2014). "(79360) Sila-Nunam". Johnston's Archive. Retrieved 28 April 2019.
↑Based on a spherical diameter of 250 km and a density of 0.73 g/cm3
↑Mass calculated using diameter and density
↑Based on a spherical diameter of 235 km and a density of 0.73 g/cm3
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System. 247: EAR–A–COMPIL–5–NEOWISEDIAM–V1.0. Bibcode:2016PDSS..247.....M. Retrieved 31 October 2018.
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1 2 3 4 5 6 7 8 9 10Tedesco; et al. (2004). "Supplemental IRAS Minor Planet Survey (SIMPS)". IRAS-A-FPA-3-RDR-IMPS-V6.0. Planetary Data System. Archived from the original on 17 August 2009. Retrieved 29 December 2008.
↑Mass calculated using diameter and primary’s density
↑Buie, Marc W.; Leiva, Rodrigo; Keller, John M.; Desmars, Josselin; Sicardy, Bruno; Kavelaars, J. J.; et al. (April 2020). "A Single-chord Stellar Occultation by the Extreme Trans-Neptunian Object (541132) Leleākūhonua". The Astronomical Journal. 159 (5): 230. arXiv:2011.03889. Bibcode:2020AJ....159..230B. doi:10.3847/1538-3881/ab8630. S2CID 219039999. 230.
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↑Mass calculated using dimensions of 254, 110, and 90 km and a density of 0.85
↑Sickafoose, Amanda A.; Levine, Stephen E.; Bosh, Amanda S.; Person, Michael J.; Zuluaga, Carlos A.; Knieling, Bastian; Lewis, Mark C.; Schindler, Karsten (1 November 2023). "Material around the Centaur (2060) Chiron from the 2018 November 28 UT Stellar Occultation". The Planetary Science Journal. 4 (11): 221. arXiv:2310.16205. Bibcode:2023PSJ.....4..221S. doi:10.3847/PSJ/ad0632.
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↑Mass calculated using a diameter of 175 km and a density of 1.76
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↑Karkoschka, Erich (2001). "Voyager's Eleventh Discovery of a Satellite of Uranus and Photometry and the First Size Measurements of Nine Satellites". Icarus. 151 (1): 69–77. Bibcode:2001Icar..151...69K. doi:10.1006/icar.2001.6597.
↑French, Richard G.; Hedman, Matthew M.; Nicholson, Philip D.; Longaretti, Pierre-Yves; McGhee-French, Colleen A. (March 2024). "The Uranus system from occultation observations (1977–2006): Rings, pole direction, gravity field, and masses of Cressida, Cordelia, and Ophelia". Icarus. 411 115957. arXiv:2401.04634. Bibcode:2024Icar..41115957F. doi:10.1016/j.icarus.2024.115957. ISSN 0019-1035.
1 2Farkas-Takács, A.; Kiss, Cs.; Pál, A.; Molnár, L.; Szabó, Gy. M.; Hanyecz, O.; et al. (September 2017). "Properties of the Irregular Satellite System around Uranus Inferred from K2, Herschel, and Spitzer Observations". The Astronomical Journal. 154 (3): 13. arXiv:1706.06837. Bibcode:2017AJ....154..119F. doi:10.3847/1538-3881/aa8365. S2CID 118869078. 119.
↑mass calculated using dimensions and density
↑Müller, T.; Kiss, Cs.; Alí-Lagoa, V.; Ortiz, J. L.; Lellouch, E.; Santos-Sanz, P.; et al. (December 2019). "Haumea's thermal emission revisited in the light of the occultation results". Icarus. 334: 39–51. arXiv:1811.09476. Bibcode:2019Icar..334...39M. doi:10.1016/j.icarus.2018.11.011. S2CID 118999774. 39–51.
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↑Johnston, Wm. Robert (21 September 2014). "(762) Pulcova". Johnston's Archive. Retrieved 10 June 2019.
↑Johnston, Wm. Robert (9 October 2021). "(229762) Gǃkúnǁʼhòmdímà and GǃòʼéǃHú". Johnston's Archive. Retrieved 2025-09-07.
1 2Johnston, Wm. Robert (31 January 2015). "(42355) Typhon and Echidna". Johnston's Archive. Retrieved 14 June 2019.
↑Johnston, Wm. Robert (9 October 2021). "(469705) |Kagara [sic]and !Haunu". Johnston's Archive. Retrieved 2025-09-07.
↑Benecchi, S.D; Noll, K. S.; Grundy, W. M.; Levison, H. F. (2010). "(47171) 1999 TC36, A Transneptunian Triple". Icarus. 207 (2): 978–991. arXiv:0912.2074. Bibcode:2010Icar..207..978B. doi:10.1016/j.icarus.2009.12.017. S2CID 118430134.
↑Pravec, P.; Harris, A. W.; Kusnirak, P.; Galad, A.; Hornoch, K. (2012). "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations". Icarus. 221 (1): 365–387. Bibcode:2012LPICo1667.6089P. doi:10.1016/j.icarus.2012.07.026.
↑Grundy, W. M.; Noll, K. S.; Nimmo, F.; Roe, H. G.; Buie, M. W.; Porter, S. B.; Benecchi, S. D.; Stephens, D. C.; Levison, H. F.; Stansberry, J. A. (2011). "Five new and three improved mutual orbits of transneptunian binaries"(PDF). Icarus. 213 (2): 678. arXiv:1103.2751. Bibcode:2011Icar..213..678G. doi:10.1016/j.icarus.2011.03.012. S2CID 9571163.
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↑"JPL Small-Body Database Browser: 28 Bellona" (2018-10-18 last obs). Retrieved 30 April 2019.
↑"JPL Small-Body Database Browser: 78 Diana" (2018-10-22 last obs). Retrieved 2 May 2019.
↑Hui, Man-To; Jewitt, David; Yu, Liang-Liang; Mutchler, Max J. (12 Apr 2022). "Hubble Space Telescope Detection of the Nucleus of Comet C/2014 UN₂₇₁ (Bernardinelli–Bernstein)". The Astrophysical Journal Letters. 929 (L12): L12. arXiv:2202.13168. Bibcode:2022ApJ...929L..12H. doi:10.3847/2041-8213/ac626a. S2CID 247158849.
↑"JPL Small-Body Database Browser: 74 Galatea" (2018-05-22 last obs). Retrieved 2 May 2019.
↑"JPL Small-Body Database Browser: 1867 Deiphobus (1971 EA)" (2018-06-21 last obs). Retrieved 2 May 2019.
↑"JPL Small-Body Database Browser: 1172 Aneas (1930 UA)" (2018-07-03 last obs). Retrieved 1 May 2019.
↑"JPL Small-Body Database Browser: 1437 Diomedes (1937 PB)" (2018-10-22 last obs). Retrieved 30 April 2019.
↑"JPL Small-Body Database Browser: 81 Terpsichore" (2018-10-22 last obs). Retrieved 2 May 2019.
↑"JPL Small-Body Database Browser: 1143 Odysseus (1930 BH)" (2018-10-22 last obs). Retrieved 2 May 2019.
↑"JPL Small-Body Database Browser: 2241 Alcathous (1979 WM)" (2018-06-17 last obs). Retrieved 2 May 2019.
↑"JPL Small-Body Database Browser: 57 Mnemosyne" (2018-06-25 last obs). Retrieved 30 April 2019.
↑"JPL Small-Body Database Browser: 659 Nestor (A908 FE)" (2018-10-22 last obs). Retrieved 2 May 2019.
↑"JPL Small-Body Database Browser: 40 Harmonia" (2018-09-15 last obs). Retrieved 3 May 2019.
↑Shepard, Michael K.; Harris, Alan W.; Taylor, Patrick A.; Clark, Beth Ellen; Ockert-Bell, Maureen; Nolan, Michael C.; et al. (2011). "Radar observations of Asteroids 64 Angelina and 69 Hesperia"(PDF). Icarus. 215 (2): 547–551. arXiv:1104.4114. Bibcode:2011Icar..215..547S. doi:10.1016/j.icarus.2011.07.027.
↑"JPL Small-Body Database Browser: 23 Thalia" (2018-10-21 last obs). Retrieved 2 May 2019.
↑"JPL Small-Body Database Browser: 62 Erato" (2018-05-24 last obs). Retrieved 3 May 2019.
↑"JPL Small-Body Database Browser: 5 Astraea" (2018-09-16 last obs). Retrieved 30 April 2019.
↑"JPL Small-Body Database Browser: 91 Aegina" (2018-07-31 last obs). Retrieved 3 May 2019.
↑"JPL Small-Body Database Browser: 35 Leukothea" (2018-10-22 last obs). Retrieved 3 May 2019.
↑"LCDB Data for (617)". Asteroid Lightcurve Database (LCDB). Archived from the original on 19 October 2020. Retrieved 1 May 2019.
↑"JPL Small-Body Database Browser: 1208 Troilus (1931 YA)" (2018-07-22 last obs). Retrieved 2 May 2019.
↑Chamberlin, Alan. "JPL Small-Body Database Search Engine".
1 2Baer, James; Steven R. Chesley (2008). "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris". Celestial Mechanics and Dynamical Astronomy. 100 (2008): 27–42. Bibcode:2008CeMDA.100...27B. doi:10.1007/s10569-007-9103-8.
↑"JPL Small-Body Database Browser: 233 Asterope" (2018-10-24 last obs). Retrieved 3 May 2019.
↑"JPL Small-Body Database Browser: 53 Kalypso" (2018-10-18 last obs). Retrieved 30 April 2019.
↑"JPL Small-Body Database Browser: 26 Prosperina" (2018-10-22 last obs). Retrieved 3 May 2019.
↑"JPL Small-Body Database Browser: 2920 Automedon (1981 JR)" (2018-10-15 last obs). Retrieved 2 May 2019.
1 2 3Johnston, Wm. Robert (21 September 2014). "(90) Antiope and S/2000 (90) 1". Johnston's Archive. Retrieved 14 June 2019.
↑"JPL Small-Body Database Browser: 61 Danae" (2018-07-13 last obs). Retrieved 4 May 2019.
↑"JPL Small-Body Database Browser: 17 Thetis" (2018-05-13 last obs). Retrieved 3 May 2019.
↑"JPL Small-Body Database Browser: 55 Pandora" (2018-10-22 last obs). Retrieved 4 May 2019.
↑"JPL Small-Body Database Browser: 379 Huenna (A894 AA)" (2018-08-30 last obs). Retrieved 3 May 2019.
↑Marchis, Franck; P. Descamps; J. Berthier; D. hestroffer; F. vachier; M. Baek; et al. (2008). "Main Belt Binary Asteroidal Systems With Eccentric Mutual Orbits". Icarus. 195 (1): 295–316. arXiv:0804.1385. Bibcode:2008Icar..195..295M. doi:10.1016/j.icarus.2007.12.010. S2CID 119244052.
↑"JPL Small-Body Database Browser: 50 Virginia" (2018-10-19 last obs). Retrieved 3 May 2019.
↑"JPL Small-Body Database Browser: 4348 Poulydamas (1988 RU)" (2018-07-13 last obs). Retrieved 4 May 2019.
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للمزيد من القراءة

نظام بيانات الكواكب التابع لناسا (PDS)
الكويكبات ذات الأقمار الصناعية
ظروف اكتشاف الكواكب الصغيرة
المسح التكميلي للكواكب الصغيرة IRAS (SIMPS) والمسح التكميلي للكواكب الصغيرة IRAS (IMPS)
- SIMPS & IMPS ( الإصدار 6 ، إضافي ، من هنا )
- أرشيف بيانات الكويكبات ^{[ تمت إزالة الرابط ]} أرشيف معهد علوم الكواكب

روابط خارجية

[equatorial-31] 1 2 3 4 5Radius estimated using equatorial radius and assuming body is spherical

[various-47] 1 2Radius has been determined by various methods, such as optical (Hubble), thermal (Spitzer), or direct imaging via spacecraft

[51] The mass of Eris by itself is the difference between the mass of the system ((1.6466±0.0085)×10²² kg)^[44] and the mass of Dysnomia by itself ((8.2±5.7)×10¹⁹ kg).^[45]

[three_radii-53] 1 2Radius estimated by using three radii and assuming body is spheroid

[WolframVolume-58] Calculated in Wolfram Alpha using semi axes of 1050 × 840 × 537^[50](Ellipsoid volume: 1.98395×10^9 km³)

[HE-60] Best fit physical model assuming hydrostatic equilibrium for Haumea.^[50]

[system_mass-67] 1 2 3 4This value refers to the system mass

[mc-92] Mass calculated by Muñoz-Gutiérrez et al. (2019 & 2021) using Achlys's area-equivalent diameter of 772 km and predicted density of 0.87 g/cm³.^[78]^:2^[79]^:2 Muñoz-Gutiérrez et al. give the mass in terms of Earth masses (M_🜨), which can be converted into kilograms by multiplying by 5.9722×10²⁴ kg/M_🜨. This calculation does not treat Achlys as an ellipsoid (which would have a volume of $V={\frac {4}{3}}\pi abc\approx 1.85\times 10^{17}{\text{ m}}^{3}$ ), though the mass calculated from Achlys's ellipsoid volume and density ( $M=\rho V\approx 1.61\times 10^{20}{\text{ kg}}$ ) is equivalent to Muñoz-Gutiérrez et al.'s mass calculation when rounded to a single digit.

[assumedalbedo-95] 1 2 3 4 5 6 7 8 9 10 11Radius estimated from an assumed albedo

[wd-99] Using Grundy et al.'s working diameters of 361 km and 163 km, and assuming the densities of the two bodies are equal, Varda would contribute 91.6% of the system mass of (2.664±0.064)×10²⁰ kg, meaning Varda's mass is about (2.44±0.06)×10²⁰ kg.^[84]

[110] very approximate figure, assuming equivalent spherical diameter of ≈600 km and density ≈2.64 g/cm³

[141] A density of 0.4–0.8 g/cm³ was calculated when assuming the volume as a sphere with a radius of 210±7 km.^[124] The mass was calculated with the provided density and the assumed volume.

[mass_estimate-177] The mass estimate is based on the assumed density of 1.2 g/cm³, and a volume of 3.5 ×10⁶ km³ obtained from a detailed shape model in Stooke (1994).^[159]

[A-13] 1 2 3 4 5 6Name of body, including alternative names using Roman numerals to designate moons (such as "Saturn I" for Mimas), and numbers to designate minor planets

[B-14] 1 2 3 4 5 6 7Volumetric radius including uncertainties

[Gravity-15] Given as surface gravity (1 bar for gaseous planets)

[default-87] Figures from default source Johnston's Archive—List of Known Trans-Neptunian Objects,^[76] if otherwise not mentioned in the References column

[Refs-88] 1 2 3 4 5 6Reference column specifically for radius (r) and mass (M) citations

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[Rizos2025-149] Rizos, J. L.; Ortiz, J. L.; Rommel, F. L.; Sicardy, B.; Morales, N.; Santos-Sanz, P.; et al. (May 2025). "The Trans-Neptunian Object (119951) 2002 KX14 as revealed by multiple stellar occultations". Astronomy & Astrophysics. 697. arXiv:2503.19179. Bibcode:2025A&A...697A..62R. doi:10.1051/0004-6361/202554154. S2CID 277313950. A62.

[Fernandez-Valenzuela2025-review-150] 1 2Fernández-Valenzuela, Estela; et al. (December 2025). "Accurate geometric albedo, shape, and size of Hi'iaka from a stellar occultation – Peer Review File"(PDF). Nature Portfolio. 16 (1): 10926. doi:10.1038/s41467-025-65749-1. PMC 12686452. PMID 41326341. Retrieved 2025-12-20.

[Fernandez-Valenzuela-2021-151] Fernández-Valenzuela, E.; Pinilla-Alonso, N.; Stansberry, J.; Emery, J. P.; Perkins, W.; Van Laerhoven, C.; et al. (February 2021). "Compositional Study of Trans-Neptunian Objects at λ > 2.2 μm". The Planetary Science Journal. 2 (1): 10. arXiv:2011.07121. Bibcode:2021PSJ.....2...10F. doi:10.3847/PSJ/abc34e. ISSN 2632-3338. S2CID 234003733.

[Interamnia-152] Hanuš, J.; Vernazza, P.; Viikinkoski, M.; Ferrais, M.; Rambaux, N.; Podlewska-Gaca, E.; et al. (2020). "(704) Interamnia: A transitional object between a dwarf planet and a typical irregular-shaped minor body". Astronomy & Astrophysics. 633: A65. arXiv:1911.13049. Bibcode:2020A&A...633A..65H. doi:10.1051/0004-6361/201936639. S2CID 208512707.

[TNOsCool14-153] 1 2Vilenius, E.; Stansberry, D.; Müller, T., T.; Mueller, M.; Kiss, C.; Santos-Sanz, P.; et al. (October 2018). ""TNOs are Cool": A survey of the trans-Neptunian region. XIV. Size/albedo characterization of the Haumea family observed with Herschel and Spitzer". Astronomy & Astrophysics. 618: A136. arXiv:1904.06333. Bibcode:2018A&A...618A.136V. doi:10.1051/0004-6361/201732564. A136.

[Gómez-Limón2025-154] Gómez-Limón, J. M.; Leiva, R.; Ortiz, J. L.; Morales, N.; Kretlow, M.; Vara-Lubiano, M.; et al. (May 2025). "Size and shape of the trans-Neptunian object (470316) 2007 OC10: Comparison with thermal data"(PDF). Astronomy & Astrophysics. 697: A157. arXiv:2504.02457. Bibcode:2025A&A...697A.157G. doi:10.1051/0004-6361/202453540.

[155] Chen, Ying-Tung; Lykawka, Patryk Sofia; Huang, Yukun; Kavelaars, J. J.; Fraser, Wesley C.; Bannister, Michele T.; Wang, Shiang-Yu; Chang, Chan-Kao; Lehner, Matthew J. (2025-08-04), "Discovery and dynamics of a Sedna-like object with a perihelion of 66 au", Nature Astronomy, 9 (9): 1309–1316, arXiv:2508.02162, Bibcode:2025NatAs...9.1309C, doi:10.1038/s41550-025-02595-7

[Elliot2010-156] 1 2Elliot, J. L.; Person, M. J.; Zuluaga, C. A.; Bosh, A. S.; Adams, E. R.; Brothers, T. C.; et al. (2010). "Size and albedo of Kuiper belt object 55636 from a stellar occultation"(PDF). Nature. 465 (7300): 897–900. Bibcode:2010Natur.465..897E. doi:10.1038/nature09109. PMID 20559381. S2CID 4431420. Archived from the original(PDF) on February 22, 2014.

[johnston-47171-157] 1 2 3Johnston, Wm. Robert (8 October 2017). "(47171) Lempo, Paha, and Hiisi". Johnston's Archive. Retrieved 10 June 2019.

[johnston-26308-158] 1 2Johnston, Wm. Robert (21 September 2014). "(26308) 1998 SM165 and S/2001 (26308) 1". Johnston's Archive. Retrieved 28 April 2019.

[Marsset2022-159] Marsset et al. (2022) The equilibrium shape of (65) Cybele: primordial or relic of a large impact?

[Marchis-2014-160] 1 2 3Marchis, F.; Durech, J.; Castillo-Rogez, J.; Vachier, F.; Cuk, M.; Berthier, J.; et al. (March 2014). "The Puzzling Mutual Orbit of the Binary Trojan Asteroid (624) Hektor". The Astrophysical Journal Letters. 783 (2): 6. arXiv:1402.7336. Bibcode:2014ApJ...783L..37M. doi:10.1088/2041-8205/783/2/L37. S2CID 19868908.

[Morgado2021-161] Morgado, B. E.; Sicardy, B.; Braga-Ribas, F.; Desmars, J.; Gomes-Júnior, A. R.; Bérard, D.; et al. (January 2020). "Refined physical parameters for Chariklo's body and rings from stellar occultations observed between 2013 and 2020". Astronomy & Astrophysics. 652: A141. arXiv:2107.07904. Bibcode:2021A&A...652A.141M. doi:10.1051/0004-6361/202141543. S2CID 236034389. A141.

[johnston-79360-162] 1 2Johnston, Wm. Robert (20 September 2014). "(79360) Sila-Nunam". Johnston's Archive. Retrieved 28 April 2019.

[163] Based on a spherical diameter of 250 km and a density of 0.73 g/cm3

[164] Mass calculated using diameter and density

[165] Based on a spherical diameter of 235 km and a density of 0.73 g/cm3

[Mainzer-2016-166] 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System. 247: EAR–A–COMPIL–5–NEOWISEDIAM–V1.0. Bibcode:2016PDSS..247.....M. Retrieved 31 October 2018.

[Carry2012-167] 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58Carry, B. (December 2012). "Density of asteroids". Planetary and Space Science. 73 (1): 98–118. arXiv:1203.4336. Bibcode:2012P&SS...73...98C. doi:10.1016/j.pss.2012.03.009. S2CID 119226456.

[Grundy2007-168] 1 2 3Grundy, W.M.; Stansberry, J.A.; Noll K.S.; Stephens, D.C.; et al. (2007). "The orbit, mass, size, albedo, and density of (65489) Ceto/Phorcys: A tidally-evolved binary Centaur". Icarus. 191 (1): 286–297. arXiv:0704.1523. Bibcode:2007Icar..191..286G. doi:10.1016/j.icarus.2007.04.004. S2CID 1532765.

[SIMPS-169] 1 2 3 4 5 6 7 8 9 10Tedesco; et al. (2004). "Supplemental IRAS Minor Planet Survey (SIMPS)". IRAS-A-FPA-3-RDR-IMPS-V6.0. Planetary Data System. Archived from the original on 17 August 2009. Retrieved 29 December 2008.

[170] Mass calculated using diameter and primary’s density

[171] Buie, Marc W.; Leiva, Rodrigo; Keller, John M.; Desmars, Josselin; Sicardy, Bruno; Kavelaars, J. J.; et al. (April 2020). "A Single-chord Stellar Occultation by the Extreme Trans-Neptunian Object (541132) Leleākūhonua". The Astronomical Journal. 159 (5): 230. arXiv:2011.03889. Bibcode:2020AJ....159..230B. doi:10.3847/1538-3881/ab8630. S2CID 219039999. 230.

[TNOsCool11-172] 1 2 3 4 5Duffard, R.; Pinilla-Alonso, N.; Santos-Sanz, P.; Vilenius, E.; Ortiz, J. L.; Mueller, T.; et al. (April 2014). ""TNOs are Cool": A survey of the trans-Neptunian region. XI. A Herschel-PACS view of 16 Centaurs". Astronomy and Astrophysics. 564: 17. arXiv:1309.0946. Bibcode:2014A&A...564A..92D. doi:10.1051/0004-6361/201322377. S2CID 119177446.

[173] Mass calculated using dimensions of 254, 110, and 90 km and a density of 0.85

[Sickafoose2023-174] Sickafoose, Amanda A.; Levine, Stephen E.; Bosh, Amanda S.; Person, Michael J.; Zuluaga, Carlos A.; Knieling, Bastian; Lewis, Mark C.; Schindler, Karsten (1 November 2023). "Material around the Centaur (2060) Chiron from the 2018 November 28 UT Stellar Occultation". The Planetary Science Journal. 4 (11): 221. arXiv:2310.16205. Bibcode:2023PSJ.....4..221S. doi:10.3847/PSJ/ad0632.

[Showalter2019-175] 1 2 3 4 5 6Showalter, M. R.; de Pater, I.; Lissauer, J. J.; French, R. S. (2019). "The seventh inner moon of Neptune"(PDF). Nature. 566 (7744): 350–353. Bibcode:2019Natur.566..350S. doi:10.1038/s41586-019-0909-9. PMC 6424524. PMID 30787452.

[Stooke1994-176] Stooke, Philip J. (1994). "The surfaces of Larissa and Proteus". Earth, Moon, and Planets. 65 (1): 31–54. Bibcode:1994EM&P...65...31S. doi:10.1007/BF00572198. S2CID 121825800.

[AKARI-178] 1 2 3 4 5 6 7 8 9 10 11 12Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117.

[johnston-121-179] Johnston, Wm. Robert (21 September 2014). "(121) Hermione and S/2002 (121) 1 ("LaFayette")". Johnston's Archive. Retrieved 5 June 2019.

[WISE-180] 1 2 3 4 5 6 7Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID 118700974.

[Ortiz2025-181] Ortiz, Jose L.; Morales, N.; Sicardy, B.; Fernandez-Valenzuela, E.; Braga-Ribas, F.; Kilic, Y.; et al. (18 Sep 2025). "A high geometric albedo and small size for the Haumea cluster member (24835) 1995 SM ₅₅ determined from a stellar occultation and photometric observations". Astronomy & Astrophysics. 703: A147. arXiv:2509.15384. Bibcode:2025A&A...703A.147O. doi:10.1051/0004-6361/202556498.

[johnston-88611-182] Johnston, Wm. Robert (20 September 2014). "(88611) Teharonhiawako and Sawiskera". Johnston's Archive. Retrieved 13 June 2019.

[Porco1991-183] Porco, C.C. (1991). "An Explanation for Neptune's Ring Arcs". Science. 253 (5023): 995–1001. Bibcode:1991Sci...253..995P. doi:10.1126/science.253.5023.995. PMID 17775342. S2CID 742763.

[184] "In Depth | Makemake - NASA Solar System Exploration". 14 November 2017.

[185] Mass calculated using a diameter of 175 km and a density of 1.76

[Masiero-2012-186] 1 2 3Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; Cabrera, M. S. (10 October 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): L8. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. S2CID 46350317.

[Rojo-2011-187] Rojo, P.; Margot, J. L. (February 2011). "Mass and Density of the B-type Asteroid (702) Alauda". The Astrophysical Journal. 727 (2): 5. arXiv:1011.6577. Bibcode:2011ApJ...727...69R. doi:10.1088/0004-637X/727/2/69. S2CID 59449907.

[Emelyanov2005-188] Emelyanov, N.V.; Archinal, B. A.; A'hearn, M. F.; et al. (2005). "The mass of Himalia from the perturbations on other satellites"(PDF). Astronomy and Astrophysics. 438 (3): L33–L36. Bibcode:2005A&A...438L..33E. doi:10.1051/0004-6361:200500143.

[ThomasBurns1998-189] 1 2 3Thomas, P. C.; Burns, J. A.; Rossier, L.; Simonelli, D.; Veverka, J.; Chapman, C. R.; Klaasen, K.; Johnson, T. V.; Belton, M. J. S.; Galileo Solid State Imaging Team (September 1998). "The Small Inner Satellites of Jupiter". Icarus. 135 (1): 360–371. Bibcode:1998Icar..135..360T. doi:10.1006/icar.1998.5976.

[AndersonJohnson2005-190] Anderson, J. D.; Johnson, T. V.; Schubert, G.; Asmar, S.; Jacobson, R. A.; Johnston, D.; Lau, E. L.; Lewis, G.; Moore, W. B.; Taylor, A.; Thomas, P. C.; Weinwurm, G. (27 May 2005). "Amalthea's Density is Less Than That of Water". Science. 308 (5726): 1291–1293. Bibcode:2005Sci...308.1291A. doi:10.1126/science.1110422. PMID 15919987. S2CID 924257.

[UranusVoyager-191] Karkoschka, Erich (2001). "Voyager's Eleventh Discovery of a Satellite of Uranus and Photometry and the First Size Measurements of Nine Satellites". Icarus. 151 (1): 69–77. Bibcode:2001Icar..151...69K. doi:10.1006/icar.2001.6597.

[192] French, Richard G.; Hedman, Matthew M.; Nicholson, Philip D.; Longaretti, Pierre-Yves; McGhee-French, Colleen A. (March 2024). "The Uranus system from occultation observations (1977–2006): Rings, pole direction, gravity field, and masses of Cressida, Cordelia, and Ophelia". Icarus. 411 115957. arXiv:2401.04634. Bibcode:2024Icar..41115957F. doi:10.1016/j.icarus.2024.115957. ISSN 0019-1035.

[FarkasTakacs2017-193] 1 2Farkas-Takács, A.; Kiss, Cs.; Pál, A.; Molnár, L.; Szabó, Gy. M.; Hanyecz, O.; et al. (September 2017). "Properties of the Irregular Satellite System around Uranus Inferred from K2, Herschel, and Spitzer Observations". The Astronomical Journal. 154 (3): 13. arXiv:1706.06837. Bibcode:2017AJ....154..119F. doi:10.3847/1538-3881/aa8365. S2CID 118869078. 119.

[194] ss calculated using dimensions and density

[Muller2019-195] Müller, T.; Kiss, Cs.; Alí-Lagoa, V.; Ortiz, J. L.; Lellouch, E.; Santos-Sanz, P.; et al. (December 2019). "Haumea's thermal emission revisited in the light of the occultation results". Icarus. 334: 39–51. arXiv:1811.09476. Bibcode:2019Icar..334...39M. doi:10.1016/j.icarus.2018.11.011. S2CID 118999774. 39–51.

[Rabinowitz2019-196] 1 2 3 4Rabinowitz, David L.; Benecchi, Susan D.; Grundy, William M.; Verbiscer, Anne J.; Thirouin, Audrey (November 2019). "The Complex Rotational Light Curve of (385446) Manwë-Thorondor, a Multi-Component Eclipsing System in the Kuiper Belt". arXiv:1911.08546 [astro-ph.EP].

[johnston-762-197] Johnston, Wm. Robert (21 September 2014). "(762) Pulcova". Johnston's Archive. Retrieved 10 June 2019.

[johnston-229762-198] Johnston, Wm. Robert (9 October 2021). "(229762) Gǃkúnǁʼhòmdímà and GǃòʼéǃHú". Johnston's Archive. Retrieved 2025-09-07.

[johnston-42355-199] 1 2Johnston, Wm. Robert (31 January 2015). "(42355) Typhon and Echidna". Johnston's Archive. Retrieved 14 June 2019.

[johnston-469705-200] Johnston, Wm. Robert (9 October 2021). "(469705) |Kagara [sic]and !Haunu". Johnston's Archive. Retrieved 2025-09-07.

[Lempo-201] Benecchi, S.D; Noll, K. S.; Grundy, W. M.; Levison, H. F. (2010). "(47171) 1999 TC36, A Transneptunian Triple". Icarus. 207 (2): 978–991. arXiv:0912.2074. Bibcode:2010Icar..207..978B. doi:10.1016/j.icarus.2009.12.017. S2CID 118430134.

[Pravec2012-202] Pravec, P.; Harris, A. W.; Kusnirak, P.; Galad, A.; Hornoch, K. (2012). "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations". Icarus. 221 (1): 365–387. Bibcode:2012LPICo1667.6089P. doi:10.1016/j.icarus.2012.07.026.

[Grundy2011-203] Grundy, W. M.; Noll, K. S.; Nimmo, F.; Roe, H. G.; Buie, M. W.; Porter, S. B.; Benecchi, S. D.; Stephens, D. C.; Levison, H. F.; Stansberry, J. A. (2011). "Five new and three improved mutual orbits of transneptunian binaries"(PDF). Icarus. 213 (2): 678. arXiv:1103.2751. Bibcode:2011Icar..213..678G. doi:10.1016/j.icarus.2011.03.012. S2CID 9571163.

[Michalak2001-204] 1 2Michalak, G. (2001). "Determination of asteroid masses". Astronomy & Astrophysics. 374 (2): 703–711. Bibcode:2001A&A...374..703M. doi:10.1051/0004-6361:20010731.

[205] Johnston, Wm. Robert (9 October 2021). "(469705) |Kagara and !Haunu". Johnston's Archive. Retrieved 2025-09-07.

[jplssd-28-206] "JPL Small-Body Database Browser: 28 Bellona" (2018-10-18 last obs). Retrieved 30 April 2019.

[jplssd-78-207] "JPL Small-Body Database Browser: 78 Diana" (2018-10-22 last obs). Retrieved 2 May 2019.

[208] Hui, Man-To; Jewitt, David; Yu, Liang-Liang; Mutchler, Max J. (12 Apr 2022). "Hubble Space Telescope Detection of the Nucleus of Comet C/2014 UN₂₇₁ (Bernardinelli–Bernstein)". The Astrophysical Journal Letters. 929 (L12): L12. arXiv:2202.13168. Bibcode:2022ApJ...929L..12H. doi:10.3847/2041-8213/ac626a. S2CID 247158849.

[jplssd-74-209] "JPL Small-Body Database Browser: 74 Galatea" (2018-05-22 last obs). Retrieved 2 May 2019.

[jplssd-1867-210] "JPL Small-Body Database Browser: 1867 Deiphobus (1971 EA)" (2018-06-21 last obs). Retrieved 2 May 2019.

[jplssd-1172-211] "JPL Small-Body Database Browser: 1172 Aneas (1930 UA)" (2018-07-03 last obs). Retrieved 1 May 2019.

[jplssd-1437-212] "JPL Small-Body Database Browser: 1437 Diomedes (1937 PB)" (2018-10-22 last obs). Retrieved 30 April 2019.

[jplssd-81-213] "JPL Small-Body Database Browser: 81 Terpsichore" (2018-10-22 last obs). Retrieved 2 May 2019.

[jplssd-1143-214] "JPL Small-Body Database Browser: 1143 Odysseus (1930 BH)" (2018-10-22 last obs). Retrieved 2 May 2019.

[jplssd-2241-215] "JPL Small-Body Database Browser: 2241 Alcathous (1979 WM)" (2018-06-17 last obs). Retrieved 2 May 2019.

[jplssd-57-216] "JPL Small-Body Database Browser: 57 Mnemosyne" (2018-06-25 last obs). Retrieved 30 April 2019.

[jplssd-659-217] "JPL Small-Body Database Browser: 659 Nestor (A908 FE)" (2018-10-22 last obs). Retrieved 2 May 2019.

[jplssd-40-218] "JPL Small-Body Database Browser: 40 Harmonia" (2018-09-15 last obs). Retrieved 3 May 2019.

[219] Shepard, Michael K.; Harris, Alan W.; Taylor, Patrick A.; Clark, Beth Ellen; Ockert-Bell, Maureen; Nolan, Michael C.; et al. (2011). "Radar observations of Asteroids 64 Angelina and 69 Hesperia"(PDF). Icarus. 215 (2): 547–551. arXiv:1104.4114. Bibcode:2011Icar..215..547S. doi:10.1016/j.icarus.2011.07.027.

[jplssd-23-220] "JPL Small-Body Database Browser: 23 Thalia" (2018-10-21 last obs). Retrieved 2 May 2019.

[jplssd-62-221] "JPL Small-Body Database Browser: 62 Erato" (2018-05-24 last obs). Retrieved 3 May 2019.

[jplssd-5-222] "JPL Small-Body Database Browser: 5 Astraea" (2018-09-16 last obs). Retrieved 30 April 2019.

[jplssd-91-223] "JPL Small-Body Database Browser: 91 Aegina" (2018-07-31 last obs). Retrieved 3 May 2019.

[jplssd-35-224] "JPL Small-Body Database Browser: 35 Leukothea" (2018-10-22 last obs). Retrieved 3 May 2019.

[lcdb-617-225] "LCDB Data for (617)". Asteroid Lightcurve Database (LCDB). Archived from the original on 19 October 2020. Retrieved 1 May 2019.

[jplssd-1208-226] "JPL Small-Body Database Browser: 1208 Troilus (1931 YA)" (2018-07-22 last obs). Retrieved 2 May 2019.

[diameter40-100-227] Chamberlin, Alan. "JPL Small-Body Database Search Engine".

[Baer2007-228] 1 2Baer, James; Steven R. Chesley (2008). "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris". Celestial Mechanics and Dynamical Astronomy. 100 (2008): 27–42. Bibcode:2008CeMDA.100...27B. doi:10.1007/s10569-007-9103-8.

[jplssd-233-229] "JPL Small-Body Database Browser: 233 Asterope" (2018-10-24 last obs). Retrieved 3 May 2019.

[jplssd-53-230] "JPL Small-Body Database Browser: 53 Kalypso" (2018-10-18 last obs). Retrieved 30 April 2019.

[jplssd-26-231] "JPL Small-Body Database Browser: 26 Prosperina" (2018-10-22 last obs). Retrieved 3 May 2019.

[jplssd-2920-232] "JPL Small-Body Database Browser: 2920 Automedon (1981 JR)" (2018-10-15 last obs). Retrieved 2 May 2019.

[johnston-90-233] 1 2 3Johnston, Wm. Robert (21 September 2014). "(90) Antiope and S/2000 (90) 1". Johnston's Archive. Retrieved 14 June 2019.

[jplssd-61-234] "JPL Small-Body Database Browser: 61 Danae" (2018-07-13 last obs). Retrieved 4 May 2019.

[jplssd-17-235] "JPL Small-Body Database Browser: 17 Thetis" (2018-05-13 last obs). Retrieved 3 May 2019.

[jplssd-55-236] "JPL Small-Body Database Browser: 55 Pandora" (2018-10-22 last obs). Retrieved 4 May 2019.

[jplssd-379-237] "JPL Small-Body Database Browser: 379 Huenna (A894 AA)" (2018-08-30 last obs). Retrieved 3 May 2019.

[Marchis2008-238] Marchis, Franck; P. Descamps; J. Berthier; D. hestroffer; F. vachier; M. Baek; et al. (2008). "Main Belt Binary Asteroidal Systems With Eccentric Mutual Orbits". Icarus. 195 (1): 295–316. arXiv:0804.1385. Bibcode:2008Icar..195..295M. doi:10.1016/j.icarus.2007.12.010. S2CID 119244052.

[jplssd-50-239] "JPL Small-Body Database Browser: 50 Virginia" (2018-10-19 last obs). Retrieved 3 May 2019.

[jplssd-4348-240] "JPL Small-Body Database Browser: 4348 Poulydamas (1988 RU)" (2018-07-13 last obs). Retrieved 4 May 2019.

[johnston-58534-241] 1 2Johnston, Wm. Robert (20 September 2014). "(58534) Logos and Zoe". Johnston's Archive. Retrieved 4 May 2019.

[jplssd-32-242] "JPL Small-Body Database Browser: 32 Pomona" (2018-06-12 last obs). Retrieved 4 May 2019.

[Grav2015-243] 1 2 3 4 5 6 7 8 9 10 11 12Grav, T.; Bauer, J. M.; Mainzer, A. K.; Masiero, J. R.; Nugent, C. R.; Cutri, R. M.; et al. (August 2015). "NEOWISE: Observations of the Irregular Satellites of Jupiter and Saturn". The Astrophysical Journal. 809 (1): 9. arXiv:1505.07820. Bibcode:2015ApJ...809....3G. doi:10.1088/0004-637X/809/1/3. S2CID 5834661. 3.

[lcdb-10370-244] "LCDB Data for (10370)". Asteroid Lightcurve Database (LCDB). Archived from the original on 10 July 2021. Retrieved 4 May 2019.

[jplssd-43-245] "JPL Small-Body Database Browser: 43 Ariadne" (2018-10-20 last obs). Retrieved 4 May 2019.

[jplssd-99-246] "JPL Small-Body Database Browser: 99 Dike" (2018-10-24 last obs). Retrieved 4 May 2019.

[jplssd-79-247] "JPL Small-Body Database Browser: 79 Eurynome" (2018-08-18 last obs). Retrieved 4 May 2019.

[jplssd-75-248] "JPL Small-Body Database Browser: 75 Eurydike" (2019-05-08 last obs). Retrieved 3 June 2019.

[jplssd-29P-249] "JPL Small-Body Database Browser: 29P/Schwassmann-Wachmann 1" (2018-10-16 last obs). Retrieved 4 May 2019.

[jplssd-64-250] "JPL Small-Body Database Browser: 64 Angelina" (2019-05-09 last obs). Retrieved 3 June 2019.

[jplssd-82-251] "JPL Small-Body Database Browser: 82 Alkmene" (2019-05-09 last obs). Retrieved 3 June 2019.

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