1 Ceres will reach opposition – the optimal time to observe it, when it will be visible for much of the night in the constellation Coma Berenices. At this time, it also appears brightest in the sky and at its largest when viewed through a telescope.
From South El Monte, it will be visible in the morning sky, becoming accessible around 19:35, when it reaches an altitude of 21° above your eastern horizon. It will then reach its highest point in the sky at 00:27, 70° above your southern horizon. It will be lost to dawn twilight around 04:53, 27° above your western horizon.
A close approach to the Earth
When a planet is at opposition, the solar system is aligned with that planet on the same side of the Sun as the Earth.
The term opposition refers to the moment when a planet passes opposite to the Sun in the sky. For those planets which orbit the Sun at a greater distance than the Earth – like 1 Ceres – this geometry occurs as the two planets pass each other in their orbits and they make closest approach – termed its perigee.
At opposition / perigee, planets are visible for much of the night, reaching their highest point in the sky around midnight local time, just as the Sun, 180° away, dips to its lowest point below the horizon.
Because it passes closest to the Earth at this time, the planet also appears at its brightest around opposition.
In practice, the variation for 1 Ceres is quite modest since it orbits much further out in the solar system than the Earth – at an average distance from the Sun of 2.77 times that of the Earth. Consequently, its distance and brightness does not vary much as it cycles between opposition and solar conjunction. The variation is much greater for Mars, since it lies much closer to the Earth.
Observing 1 Ceres
At opposition, 1 Ceres is visible for much of the night. Even when it is at its closest point to the Earth, however, 1 Ceres is so distant from the Earth that it is not possible to distinguish it as more than a star-like point of light, even through a telescope.
A chart of the path of 1 Ceres across the sky in 1977 can be found here, and a chart of its rising and setting times here.
At the moment of opposition, 1 Ceres will lie at a distance of 1.60 AU, and reach a peak brightness of magnitude 6.9. At opposition, its celestial coordinates will be:
| Object | Right Ascension | Declination | Constellation | Magnitude | Angular Size |
| 1 Ceres | 12h34m20s | 14°37'N | Coma Berenices | 6.9 | 0.0" |
The coordinates above are given in J2000.0.
Over the weeks following its opposition, 1 Ceres will reach its highest point in the sky around four minutes earlier each night, gradually receding from the pre-dawn morning sky while remaining visible in the evening sky for a few months.
The sky on 16 Dec 2025
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8% 26 days old |
All times shown in PST.
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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
| 22 Mar 1977 | – 1 Ceres at opposition |
| 07 Jul 1978 | – 1 Ceres at opposition |
| 03 Oct 1979 | – 1 Ceres at opposition |
| 08 Jan 1981 | – 1 Ceres at opposition |
Image credit
© NASA/Dawn 2015