Mars at opposition

Dominic Ford, Editor
From the Outer Planets feed


Objects: Mars

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

From Fairfield, it will be visible between 21:18 and 04:27. It will become accessible at around 21:18, when it rises to an altitude of 7° above your south-eastern horizon. It will reach its highest point in the sky at 00:53, 24° above your southern horizon. It will become inaccessible at around 04:27 when it sinks below 7° above your south-western horizon.

1969 apparition of Mars

27 Apr 1969 – Mars enters retrograde motion
31 May 1969 – Mars at opposition
09 Jun 1969 – Mars at perigee
08 Jul 1969 – 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 1969, 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 at closest opposition
Mars at 1969 opposition
Mars at furthest opposition
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:

05 Apr 1969
03 May 1969
31 May 1969
28 Jun 1969
26 Jul 1969

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

Date Angular size Mag
22 Mar 196910.2”-0.1
05 Apr 196911.8”-0.5
19 Apr 196913.7”-0.9
03 May 196915.9”-1.4
17 May 196917.9”-1.8
31 May 196919.3”-2.2
14 Jun 196919.4”-2.1
28 Jun 196918.4”-1.8
12 Jul 196916.8”-1.5
26 Jul 196915.2”-1.2
09 Aug 196913.6”-0.9

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 1969 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 0.49 AU, and its disk will measure 19.3 arcsec in diameter, shining at magnitude -2.2. Its celestial coordinates at the moment it passes opposition will be:

Object Right Ascension Declination Constellation Magnitude Angular Size
Mars 16h34m00s 24°00'S Ophiuchus -2.2 19.3"

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 22 Nov 2024

The sky on 22 November 2024
Sunrise
06:47
Sunset
16:28
Twilight ends
18:05
Twilight begins
05:10


Waning Crescent

44%

21 days old

Planets
Rise Culm. Set
Mercury 08:40 13:06 17:32
Venus 10:13 14:39 19:06
Moon 22:16 05:32 12:36
Mars 20:52 04:15 11:38
Jupiter 17:26 00:53 08:20
Saturn 13:09 18:41 00:13
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

31 May 1969  –  Mars at opposition
09 Jun 1969  –  Mars at perigee
08 Jul 1969  –  Mars ends retrograde motion
11 Jul 1971  –  Mars enters retrograde motion

Image credit

© NASA/Hubble Space Telescope

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