The largest comets
TOP 25The largest comet in this catalogue is C/2014 UN271 (Bernardinelli-Bernstein), with a radius of 68.5 km. Next are 167P/CINEOS and 29P/Schwassmann-Wachmann 1.
Radius here means the solid nucleus: the few kilometres of ice and dust that stay behind once the tail has boiled away. That tail can be longer than the distance from the Earth to the Sun and is gone within months, while the nucleus is the comet itself — so it is the nucleus that is ranked.
NAME
CLASS
MASS
DISTANCE
MAG
CONSTELLATION
C/2014 UN271 (Bernardinelli-Bernstein)★
Comet
—
14 766.6 AU · Sun
—
—
167P/CINEOS
Chiron-type comet
—
16.1418 AU · Sun
—
—
29P/Schwassmann-Wachmann 1
Jupiter-family comet
—
6.04598 AU · Sun
—
—
C/1995 O1 (Hale-Bopp)★
Comet
—
177.433 AU · Sun
—
—
C/2011 KP36 (Spacewatch)
Jupiter-family comet
—
38.4114 AU · Sun
—
—
109P/Swift-Tuttle
Halley-type comet
—
26.0921 AU · Sun
—
—
28P/Neujmin 1
Jupiter-family comet
—
6.96547 AU · Sun
—
—
C/2001 OG108 (LONEOS)
Halley-type comet
—
13.3001 AU · Sun
—
—
C/1991 L3 (Levy)
Halley-type comet
—
13.8131 AU · Sun
—
—
1P/Halley★
Halley-type comet
—
17.9286 AU · Sun
—
—
65P/Gunn
Jupiter-family comet
—
3.88449 AU · Sun
—
—
10P/Tempel 2
Jupiter-family comet
—
3.06325 AU · Sun
—
—
99P/Kowal 1
Jupiter-family comet
—
6.13451 AU · Sun
—
—
C/1983 H1 (IRAS-Araki-Alcock)
Comet
—
98.0344 AU · Sun
—
—
117P/Helin-Roman-Alu 1
Jupiter-family comet
—
4.09608 AU · Sun
—
—
49P/Arend-Rigaux
Jupiter-family comet
—
3.56684 AU · Sun
—
—
151P/Helin
Jupiter-family comet
—
5.80725 AU · Sun
—
—
32P/Comas Sola
Jupiter-family comet
—
4.49888 AU · Sun
—
—
77P/Longmore
Jupiter-family comet
—
3.61287 AU · Sun
—
—
30P/Reinmuth 1
Jupiter-family comet
—
3.77087 AU · Sun
—
—
90P/Gehrels 1
Jupiter-family comet
—
6.06865 AU · Sun
—
—
53P/Van Biesbroeck
Jupiter-family comet
—
5.40467 AU · Sun
—
—
96P/Machholz 1
Jupiter-family comet
—
3.03507 AU · Sun
—
—
184P/Lovas 2
Jupiter-family comet
—
3.52249 AU · Sun
—
—
31P/Schwassmann-Wachmann 2
Jupiter-family comet
—
4.24342 AU · Sun
—
—
[
COMMON QUESTIONS
] 8 ANSWERED- What is being measured — the comet or the tail?
- The nucleus: the solid body of ice and dust, typically a few kilometres across. The coma and tail can be larger than the Sun and longer than the distance from here to it, but they are thinner than a laboratory vacuum and last only while the comet is near the Sun.
- Why are so few sizes known?
- Because a nucleus is small, dark and normally buried inside its own coma. The reliable figures come from spacecraft that have visited one, or from observations made far from the Sun where the comet is inactive and the bare nucleus is what is being seen.
- 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 comets 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 big can a comet nucleus be?
- Most are a few kilometres. The largest known, Bernardinelli-Bernstein, is around 120 km across — big enough that it was first mistaken for a dwarf planet, and it will not come closer to the Sun than the orbit of Saturn.
- Does size decide how bright a comet becomes?
- Only partly, and less than people expect. Brightness depends on how much volatile ice is left near the surface and how close the comet passes to the Sun, so a small fresh comet can outshine a large exhausted one.
- Do comets shrink?
- Yes. Every pass boils off part of the surface, and a short-period comet loses metres of material each orbit. Eventually it either breaks apart or seals over with dust and becomes indistinguishable from a dark asteroid.
SEE ALSOALL COMETS