© NASA/Hubble Space Telescope

Mars at opposition

Dominic Ford, Editor
From the Outer Planets feed

Objects: Mars
Please wait
Loading 0/4
Click and drag to rotate
Mouse wheel to zoom in/out
Touch with mouse to dismiss
The sky at

Mars will reach opposition, when it lies opposite to the Sun in the sky. Lying in the constellation Cancer, it will be visible for much of the night, reaching its highest point in the sky around midnight local time.

From Ashburn, it will be visible in the morning sky, becoming accessible around 17:59, when it reaches an altitude of 7° above your north-eastern horizon. It will then reach its highest point in the sky at 00:31, 73° above your southern horizon. It will be lost to dawn twilight around 07:00, 8° above your western horizon.

Begin typing the name of a town near to you, and then select the town from the list of options which appear below.

2009–2010 apparition of Mars

20 Dec 2009 – Mars enters retrograde motion
27 Jan 2010 – Mars at perigee
29 Jan 2010 – Mars at opposition
10 Mar 2010 – Mars ends retrograde motion

A close approach to the Earth

At around the same time that Mars passes opposition, it also makes its closest approach to the Earth – termed its perigee – making it appear at its brightest and largest.

This happens because when Mars lies opposite to the Sun in the sky, the Earth passes between Mars and the Sun. The solar system is lined up with Mars and the Earth on the same side of the Sun, as shown by the configuration labelled perigee in the diagram below:


When a planet is at opposition, the solar system is aligned such that the planet lies on the same side of the Sun as the Earth. At this time, the planet makes its perigee, or closest approach to the Earth. Not drawn to scale.

The panels below show a comparison of the apparent size of Mars when seen at opposition in 2010, and when it is most distant from the Earth at solar conjunction.

Also shown is the full range of different sizes it can appear at opposition, due to the slightly oval shape of Mars' orbit. It appears largest when it reaches opposition around late August, and significantly smaller when it reaches opposition around late February.

Mars
Mars at closest opposition
Mars
Mars at 2010 opposition
Mars
Mars at furthest opposition
Mars
Mars at solar conjunction

Mars: our close neighbor

Of all the planets, Mars shows the greatest variation in its apparent size and brightness. Its angular size varies by a factor of more than seven, between 25.69" and 3.49".

This comes about because it neighbors the Earth in the solar system, orbiting the Sun at a distance of about 1.5 times the Earth's distance from the Sun. This means that its distance from the Earth varies greatly, between 0.36 AU and 2.68 AU. depending whether it lies next to, or opposite to, the Earth in its orbit.

The geometry of Mars' orbit is such that it spends much longer periods of time at large distances from the Earth than it does close to us, which provides added incentive to observe it in the weeks around opposition. Whenever it passes opposition, every two years, Mars appears large and bright for only a few weeks. The panels below show the month-by-month change in Mars' apparent size:

Mars
04 Dec 2009
Mars
01 Jan 2010
Mars
29 Jan 2010
Mars
26 Feb 2010
Mars
26 Mar 2010

The table below lists Mars' angular size at brightness at two-week intervals throughout its apparition:

Date Angular size Mag
20 Nov 20099.1”0.1
04 Dec 200910.2”-0.1
18 Dec 200911.4”-0.5
01 Jan 201012.7”-0.8
15 Jan 201013.8”-1.1
29 Jan 201014.1”-1.3
12 Feb 201013.5”-1.0
26 Feb 201012.3”-0.7
12 Mar 201010.9”-0.3
26 Mar 20109.7”0.0
09 Apr 20108.6”0.3

This data is also available in the form of a graph of the angular size of Mars here, and a graph of its brightness here.

Observing Mars

At opposition, Mars is visible for much of the night. When it lies opposite to the Sun in the sky, this means that it rises at around the time the Sun sets, and it sets at around the time the Sun rises. It reaches its highest point in the sky at around midnight local time.

But even when it is at its closest point to the Earth, it is not possible to distinguish it as more than a star-like point of light without the aid of a telescope.

A chart of the path of Mars across the sky in 2010 can be found here, and a chart of its rising and setting times here.

At the moment of opposition, Mars will lie at a distance of 0.66 AU, and its disk will measure 14.1 arcsec in diameter, shining at magnitude -1.3. Its celestial coordinates at the moment it passes opposition will be:

Object Right Ascension Declination Constellation Magnitude Angular Size
Mars 08h53m30s 22°11'N Cancer -1.3 14.1"

The coordinates above are given in J2000.0.

Over the weeks following its opposition, Mars will reach its highest point in the sky four minutes earlier each night, gradually receding from the pre-dawn morning sky while remaining visible in the evening sky for a few months.

The sky on 30 November 2021
Sunrise
07:09
Sunset
16:49
Twilight ends
18:25
Twilight begins
05:33

26-day old moon
Waning Crescent

10%

26 days old

Planets
Rise Culm. Set
Mercury 07:19 12:03 16:47
Venus 10:25 15:00 19:35
Moon 02:32 08:38 14:38
Mars 05:44 10:47 15:50
Jupiter 12:05 17:21 22:37
Saturn 11:19 16:18 21:17
All times shown in EST.

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

29 Jan 2010  –  Mars at opposition
03 Mar 2012  –  Mars at opposition
05 Mar 2012  –  Mars at perigee
08 Apr 2014  –  Mars at opposition

Image credit

© NASA/Hubble Space Telescope

Share

Follow

Ashburn

Latitude:
Longitude:
Timezone:

39.04°N
77.49°W
EST

Color scheme