Mars will reach the end of its retrograde motion, ending its westward movement through the constellations and returning to more usual eastward motion instead. This reversal of direction is a phenomenon that all the solar system's outer planets periodically undergo, a few months after they pass opposition.
The retrograde motion is caused by the Earth's own motion around the Sun. As the Earth circles the Sun, our perspective changes, and this causes the apparent positions of objects to move from side-to-side in the sky with a one-year period. This nodding motion is super-imposed on the planet's long-term eastward motion through the constellations.
The diagram below illustrates this. The grey dashed arrow shows the Earth's sight-line to the planet, and the diagram on the right shows the planet's apparently movement across the sky as seen from the Earth:
2027 apparition of Mars
|10 Jan 2027||–||Mars enters retrograde motion|
|19 Feb 2027||–||Mars at opposition|
|19 Feb 2027||–||Mars at perigee|
|01 Apr 2027||–||Mars ends retrograde motion|
Mars leaves retrograde motion as its 2027 apparition comes to an end, although it will remain visible for some weeks in the dusk sky.
Its celestial coordinates as it leaves retrograde motion will be:
|Object||Right Ascension||Declination||Constellation||Magnitude||Angular Size|
The coordinates above are given in J2000.0.
From Fairfield , it will be visible in the evening sky, becoming accessible around 19:41 (EDT), 53° above your south-eastern horizon, as dusk fades to darkness. It will then reach its highest point in the sky at 21:50, 66° above your southern horizon. It will continue to be observable until around 04:02, when it sinks below 8° above your western horizon.
Over the following weeks, Mars will reach its highest point in the sky four minutes earlier each night, gradually disappearing into evening twilight.
The panels below show the month-by-month change in Mars' apparent size in coming weeks, as it recedes from the Earth:
The table below lists Mars' angular size at brightness at two-week intervals throughout its apparition:
|21 Jan 2027||12.2”||-0.6|
|04 Feb 2027||13.3”||-1.0|
|18 Feb 2027||13.8”||-1.2|
|04 Mar 2027||13.5”||-1.0|
|18 Mar 2027||12.4”||-0.7|
|01 Apr 2027||11.2”||-0.4|
|15 Apr 2027||9.9”||-0.0|
|29 Apr 2027||8.8”||0.3|
|13 May 2027||8.0”||0.5|
|27 May 2027||7.2”||0.7|
|10 Jun 2027||6.6”||0.9|
|The sky on 01 April 2027|
24 days old
All times shown in EDT.
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.
|19 Feb 2027||– Mars at perigee|
|25 Mar 2029||– Mars at opposition|
|29 Mar 2029||– Mars at perigee|
|04 May 2031||– Mars at opposition|
© NASA/Hubble Space Telescope