The largest asteroids

TOP 50

The largest asteroid in this catalogue is 1 Ceres, with a radius of 469.7 km. Next are 20000 Varuna and 4 Vesta.

The four largest bodies in the asteroid belt hold roughly half its total mass, and all of it together would not make a Moon. Sizes come from the Small-Body Database and are best estimates, not measured diameters, for most of the list.

NAME
CLASS
MASS
DISTANCE
MAG
CONSTELLATION
1 Ceres
Main-belt asteroid
1.57×10⁻⁴ M⊕
2.76555 AU · Sun
3.34 H
20000 Varuna
Trans-Neptunian object
43.2 AU · Sun
3.79 H
4 Vesta
Main-belt asteroid
2.59×10²⁰ kg
2.36137 AU · Sun
3.25 H
2 Pallas
Main-belt asteroid
2.04×10²⁰ kg
2.76956 AU · Sun
4.12 H
10 Hygiea
Main-belt asteroid
1.05×10²⁰ kg
3.15097 AU · Sun
5.65 H
15789
Trans-Neptunian object
39.6833 AU · Sun
7.09 H
704 Interamnia
Main-belt asteroid
7.49×10¹⁹ kg
3.05681 AU · Sun
6.34 H
52 Europa
Main-belt asteroid
3.09414 AU · Sun
6.65 H
10199 Chariklo
Centaur
15.7344 AU · Sun
6.55 H
511 Davida
Main-belt asteroid
3.16179 AU · Sun
6.42 H
31 Euphrosyne
Main-belt asteroid
3.1619 AU · Sun
6.83 H
451 Patientia
Main-belt asteroid
3.06455 AU · Sun
6.78 H
87 Sylvia
Outer main-belt asteroid
3.49093 AU · Sun
6.93 H
3 Juno
Main-belt asteroid
2.67099 AU · Sun
5.19 H
65 Cybele
Outer main-belt asteroid
3.40715 AU · Sun
6.83 H
88 Thisbe
Main-belt asteroid
2.76622 AU · Sun
7.24 H
15 Eunomia
Main-belt asteroid
2.64196 AU · Sun
5.42 H
95626
Centaur
22.9871 AU · Sun
7.19 H
624 Hektor
Jupiter trojan
5.27699 AU · Sun
7.32 H
16 Psyche
Main-belt asteroid
2.4×10¹⁹ kg
2.92572 AU · Sun
6.20 H
324 Bamberga
Main-belt asteroid
2.68256 AU · Sun
7.19 H
48 Doris
Main-belt asteroid
3.11356 AU · Sun
7.10 H
375 Ursula
Main-belt asteroid
3.12675 AU · Sun
7.48 H
107 Camilla
Outer main-belt asteroid
1.12×10¹⁹ kg
3.49673 AU · Sun
7.09 H
121 Hermione
Outer main-belt asteroid
3.45777 AU · Sun
7.39 H
117 Lomia
Main-belt asteroid
2.99179 AU · Sun
8.15 H
106 Dione
Main-belt asteroid
3.18209 AU · Sun
7.76 H
41 Daphne
Main-belt asteroid
2.76723 AU · Sun
7.58 H
94 Aurora
Main-belt asteroid
3.15906 AU · Sun
7.70 H
13 Egeria
Main-belt asteroid
2.57636 AU · Sun
6.92 H
45 Eugenia
Main-belt asteroid
2.72328 AU · Sun
7.74 H
19 Fortuna
Main-belt asteroid
2.44151 AU · Sun
7.49 H
7 Iris
Main-belt asteroid
2.38575 AU · Sun
5.70 H
334 Chicago
Outer main-belt asteroid
3.94015 AU · Sun
7.63 H
24 Themis
Main-belt asteroid
3.144 AU · Sun
7.21 H
154 Bertha
Main-belt asteroid
3.1937 AU · Sun
7.65 H
42355 Typhon
Trans-Neptunian object
37.7797 AU · Sun
7.63 H
702 Alauda
Main-belt asteroid
3.19226 AU · Sun
7.47 H
5145 Pholus
Centaur
20.2897 AU · Sun
7.07 H
9 Metis
Main-belt asteroid
2.38657 AU · Sun
6.18 H
29 Amphitrite
Main-belt asteroid
2.55457 AU · Sun
5.97 H
54598 Bienor
Centaur
16.6028 AU · Sun
7.49 H
6 Hebe
Main-belt asteroid
2.42566 AU · Sun
5.62 H
130 Elektra
Main-belt asteroid
3.1253 AU · Sun
7.46 H
165 Loreley
Main-belt asteroid
3.12637 AU · Sun
7.81 H
39 Laetitia
Main-belt asteroid
2.76926 AU · Sun
5.97 H
209 Dido
Main-belt asteroid
3.15368 AU · Sun
8.30 H
96 Aegle
Main-belt asteroid
3.04816 AU · Sun
7.66 H
423 Diotima
Main-belt asteroid
3.06833 AU · Sun
7.39 H
259 Aletheia
Main-belt asteroid
3.13336 AU · Sun
7.80 H
[

COMMON QUESTIONS

] 8 ANSWERED
How large is the largest?
Ceres, at about 940 km across, holds roughly a third of the mass of the entire asteroid belt and is round enough to be classed as a dwarf planet. Below the first few, sizes fall away very quickly.
Why are most of them not round?
Because they are too small for their own gravity to overcome the strength of rock. Below a few hundred kilometres a body keeps whatever shape collisions left it, which is why most asteroids are lumps rather than spheres.
What does the size column actually measure?
Not always the same thing, and the site says which. A round body has a mean radius; an oblate planet may have an equatorial one; an irregular asteroid has an effective radius, meaning the radius of a sphere that would show the same disc. Each object's page names the kind it holds.
How firm is the order?
Firm at the top and soft further down. The largest bodies have been resolved or visited and their sizes are known to a per cent or two; the smaller ones are often sized from brightness plus an assumed reflectivity, which can be wrong by a factor of two in either direction.
Why are some asteroids missing?
Because no size is recorded for them here. Measuring one needs a resolved image, an occultation, a transit or a radar echo, and most catalogued bodies have had none of those.
How is an asteroid's size measured?
The best figures come from spacecraft, radar, or watching one pass in front of a star. Otherwise size is inferred from brightness plus an assumed reflectivity — and since a dark asteroid and a small bright one look identical, that estimate can be wrong by a factor of two.
Do the big ones ever come near the Earth?
No. The largest asteroids are all in the main belt between Mars and Jupiter and stay there. Near-Earth objects are a separate and much smaller population, tracked precisely because their orbits cross ours.
Could the belt have been a planet?
There was never enough material. Everything in the belt together comes to about 3 per cent of the mass of the Moon, and Jupiter's gravity stirs the region hard enough that collisions there break bodies up rather than build them.