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Ceres

File:Ceres_-_RC3_-_Haulani_Crater_(22381131691)_(cropped).jpg · Wikimedia Commons · See Wikimedia Commons

EntityQ596· pop 143· linked from 874 articles

Also known as (1) Ceres, 1 Ceres, Ceres (dwarf planet)

Güneş'e en yakın aynı zamanda en küçük cüce gezegen

AI overview

Ceres is the largest asteroid in the asteroid belt between Mars and Jupiter, and it's officially classified as a dwarf planet. Scientists study it because understanding its composition and structure helps reveal how the early Solar System formed.

AI-generated from the Wikipedia summary — may contain errors.

In the Vinony graph

Within Vinony's link graph, Ceres is referenced by 874 other articles, and connects out to infrared radiation, apsis and cryovolcano.

It is catalogued under topics including Active asteroids, Astronomical objects discovered in 1801 and Background asteroids.

Its subject is documented across 139 Wikipedia language editions.

Wikidata facts

Diameter
939.4
Mass
939300000000000000000
Orbital period
1679.910572771899
Image
Ceres - RC3 - Haulani Crater (22381131691) (cropped).jpg
Show 22 more facts
IPA transcription
ˈt͡seːʁɛs
Commons category
Ceres (dwarf planet)
Unicode character
time of discovery or invention
1801-01-01
Commons gallery
(1) Ceres
provisional designation
A801 AA
apparent magnitude
6.79
albedo
0.090
density
2.162
rotation period
9.07417
absolute magnitude
3.34
volume as quantity
434000000
angular diameter
0.854
orbital eccentricity
0.07957631994408416
semi-major axis of an orbit
2.765615651508659
periapsis
2.545538135581839
apoapsis
2.985693167435478
orbital inclination
10.58788658206854
longitude of ascending node
80.24963090816965
argument of periapsis
73.29975464616518
mean anomaly
231.5397330043706
time of periapsis
2461599.9493352976
Sources (8)

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Gallery (12)

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