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 2.54 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 Fairfield, at the moment of perihelion it will be visible in the dawn sky, rising at 00:02 (EDT) and reaching an altitude of 57° above the south-eastern horizon before fading from view as dawn breaks at around 05:50.

A chart of the path of 1 Ceres across the sky in 2045 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 12h02m00s 10°59'N Virgo 8.4 0.0"

The coordinates above are given in J2000.0.

The sky on 27 Sep 2024

The sky on 27 September 2024
Sunrise
06:43
Sunset
18:40
Twilight ends
20:13
Twilight begins
05:11


Waning Crescent

21%

24 days old

Planets
Rise Culm. Set
Mercury 06:30 12:35 18:40
Venus 09:21 14:36 19:51
Moon 01:20 09:08 16:44
Mars 23:49 07:21 14:53
Jupiter 22:18 05:46 13:14
Saturn 17:54 23:28 05:02
All times shown in EDT.

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

25 Nov 2044  –  1 Ceres at opposition
20 Mar 2046  –  1 Ceres at opposition
06 Jul 2047  –  1 Ceres at opposition
01 Oct 2048  –  1 Ceres at opposition

Image credit

© NASA/Dawn 2015

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