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 17.3% 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 dawn sky, rising at 00:43 (PDT) and reaching an altitude of 55° above the south-eastern horizon before fading from view as dawn breaks at around 05:24.

A chart of the path of 1 Ceres across the sky in 2137 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 11h57m40s 10°43'N Leo 8.6 0.0"

The coordinates above are given in J2000.0.

The sky on 15 Jul 2026

The sky on 15 July 2026
Sunrise
05:49
Sunset
20:03
Twilight ends
21:45
Twilight begins
04:07


Waxing Crescent

4%

1 day old

Planets
Rise Culm. Set
Mercury 05:44 12:35 19:26
Venus 09:20 15:51 22:21
Moon 07:16 14:23 21:20
Mars 02:51 09:58 17:04
Jupiter 06:39 13:38 20:38
Saturn 00:03 06:14 12:26
All times shown in PDT.

Source

The circumstances of this event were computed using the DE440 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

30 Nov 2136  –  1 Ceres at opposition
25 Mar 2138  –  1 Ceres at opposition
10 Jul 2139  –  1 Ceres at opposition
05 Oct 2140  –  1 Ceres at opposition

Image credit

© NASA/Dawn 2015

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