The largest asteroids
TOP 50The 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.
SEE ALSOALL ASTEROIDS