1 Ceres's 4.6-year orbit around the Sun will carry it to its closest point to the Sun – its perihelion – at a distance of 2.55 AU.
In practice, however, 1 Ceres's orbit is very close to circular; its distance from the Sun only varies by about 17.3% between perihelion and aphelion. This means that the difference in the amount of heat and light it receives from the Sun between aphelion and perihelion is extremely small.
Finding 1 Ceres
1 Ceres's distance from the Sun doesn't affect its appearance. From South El Monte, at the moment of perihelion it will be visible in the morning sky, becoming accessible around 20:00, when it reaches an altitude of 21° above your eastern horizon. It will then reach its highest point in the sky at 01:14, 79° above your southern horizon. It will be lost to dawn twilight around 05:33, 33° above your western horizon.
A chart of the path of 1 Ceres across the sky in 2055 can be found here, and a chart of its rising and setting times here.
The position of 1 Ceres at the moment it passes perihelion will be:
| Object | Right Ascension | Declination | Constellation | Magnitude | Angular Size |
| 1 Ceres | 11h03m50s | 23°42'N | Leo | 6.9 | 0.0" |
The coordinates above are given in J2000.0.
The sky on 26 Mar 2026
| The sky on 26 March 2026 | ||||||||||||||||||||||||||||||||||
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63% 7 days old |
All times shown in PDT.
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Source
The circumstances of this event were computed using the DE430 planetary ephemeris published by the Jet Propulsion Laboratory (JPL).
This event was automatically generated by searching the ephemeris for planetary alignments which are of interest to amateur astronomers, and the text above was generated based on an estimate of your location.
Related news
| 08 Nov 2053 | – 1 Ceres at opposition |
| 24 Feb 2055 | – 1 Ceres at opposition |
| 17 Jun 2056 | – 1 Ceres at opposition |
| 15 Sep 2057 | – 1 Ceres at opposition |
Image credit
© NASA/Dawn 2015