1 Ceres will pass close to the Sun in the sky as its orbit carries it around the far side of the solar system from the Earth.
At closest approach, 1 Ceres will appear at a separation of only 4°26' from the Sun, making it totally unobservable for several weeks while it is lost in the Sun's glare.
At around the same time, 1 Ceres will also be at its most distant from the Earth – receding to a distance of 3.92 AU – since the two planets will lie on opposite sides of the solar system.
Over following weeks and months, 1 Ceres will re-emerge to the west of the Sun, gradually becoming visible for ever-longer periods in the pre-dawn sky. After around six months, it will reach opposition, when it will be visible for virtually the whole night. A chart of the path of 1 Ceres across the sky in 1997 can be found here, and a chart of its rising and setting times here.
The position of 1 Ceres at the moment it passes solar conjunction will be:
| Object | Right Ascension | Declination | Constellation | Angular Size |
| 1 Ceres | 19h47m10s | 25°39'S | Sagittarius | 0.0" |
| Sun | 19h43m | 21°17'S | Sagittarius | 32'31" |
The coordinates above are given in J2000.0.
The sky on 9 May 2024
| The sky on 9 May 2024 | ||||||||||||||||||||||||||||||||||
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6% 1 day old |
All times shown in EDT.
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Warning
Never attempt to point a pair of binoculars or a telescope at an object close to the Sun. Doing so may result in immediate and permanent blindness.
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
| 29 May 1996 | – 1 Ceres at opposition |
| 29 Aug 1997 | – 1 Ceres at opposition |
| 28 Nov 1998 | – 1 Ceres at opposition |
| 21 Mar 2000 | – 1 Ceres at opposition |
Image credit
© NASA/Dawn 2015