1 Ceres at perihelion

Dominic Ford, Editor
From the Dwarf Planets feed


Objects: 1 Ceres

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 17.2% 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 dawn sky, rising at 00:05 (PDT) and reaching an altitude of 63° above the south-eastern horizon before fading from view as dawn breaks at around 05:37.

A chart of the path of 1 Ceres across the sky in 2068 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 12h02m30s 10°59'N Virgo 8.4 0.0"

The coordinates above are given in J2000.0.

The sky on 15 Jul 2025

The sky on 15 July 2025
Sunrise
05:49
Sunset
20:03
Twilight ends
21:44
Twilight begins
04:07


Waning Gibbous

72%

20 days old

Planets
Rise Culm. Set
Mercury 07:41 14:22 21:04
Venus 03:00 10:00 17:00
Moon 22:49 04:40 10:41
Mars 10:06 16:26 22:45
Jupiter 04:40 11:50 19:00
Saturn 23:28 05:27 11:25
All times shown in PDT.

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

26 Nov 2067  –  1 Ceres at opposition
19 Mar 2069  –  1 Ceres at opposition
05 Jul 2070  –  1 Ceres at opposition
02 Oct 2071  –  1 Ceres at opposition

Image credit

© NASA/Dawn 2015

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