Mars's 687-day orbit around the Sun will carry it to its furthest point to the Sun – its aphelion – at a distance of 1.67 AU.

Unlike most of the planets, which follow almost exactly circular orbits around the Sun which only vary in their distance from the Sun by a few percent, Mars has a significantly elliptical orbit. Its distance from the Sun varies between 1.38 AU and 1.67 AU – a variation of over 20% – meaning that it receives 31% less heat and light from the Sun at aphelion as compared to perihelion.

Finding Mars

Mars's distance from the Sun doesn't affect its appearance. From Columbus, at the moment of aphelion it will be visible in the evening sky, becoming accessible around 18:42 (EST), 23° above your eastern horizon, as dusk fades to darkness. It will then reach its highest point in the sky at 23:37, 67° above your southern horizon. It will continue to be observable until around 05:52, when it sinks below 7° above your western horizon.

A chart of the path of Mars across the sky in 2027 can be found here, and a chart of its rising and setting times here.

The position of Mars at the moment it passes aphelion will be:

The coordinates above are given in J2000.0.

The sky on 4 Mar 2027

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.

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Image credit

© NASA/Hubble Space Telescope

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