Mars
- Mars is the 4th planet from the Sun.
- The planet Mars has a diameter of 4200 miles.
- At a distance of 141 million miles, it takes 687 days to circle the Sun.
- One day lasts 24 hours, 24 minutes of Earth time.
Good views of Mars occur every other
year. Best views occur when most favorable opposition takes place, every 15 or 17 years. This happens when Mars
is in opposition during the months of August or September. Mars' period of revolution around the Sun is about two
years.
This NASA photo of Mars is a composite created with images snapped by the Mars Global Surveyor. The picture is a made up of color strips taken on nine successive orbits from pole-to-pole over the planet in March 1999. The color in this picture is computer-enhanced and is not as it would appear to the human eye.
Learn about the Mars Hoax and how you
can help
Mars at Opposition
Mars Opposition - 2018
Mars will come into Opposition on July 28, 2018, in
the constellation Capricornus, when it will shine at an apparent
visual brightness of -2.78 mag. Four days later, on July 31, 2018,
it will have its closest approach to Earth during this apparition,
with a distance of only 35.994 million miles (57.59 million km,
0.38496 AU), and an apparent diameter of 24.31". This will be the
closest approach since the record
opposition of 2003, and become comparatively close only in
2031. Mars will not be this close again until the opposition of
2287.
Learn more at
SEDS
Mars Opposition - 2005
During October and November 2005, Mars will be just as
bright as it was during the opposition of 2003, but, this year, the
time frame is shifted to autumn.
Mars will be rising in the east around midnight during July and
August. By October, it will be rising at sunset. Once above the
horizon, it will be the brightest object in the sky, a bright
red-orange "star". It will be brighter in a pair of binoculars, but
you will need a telescope to see any detail.
Mars Opposition will be in early November, which means it will be
directly overhead at midnight, local time, on November 7.
As your read about the 2003 Opposition of Mars, keep in mind that
most of this information, except for the dates, also applies to the
Opposition of 2005.
Mars Opposition -
2003
During August 2003, Mars, the Red Planet, will be closer to
Earth than it has ever been before in recorded history. On the date of
closest approach, August 28, 2003, Mars will be only 55.8 million
kilometers from Earth, little more than 1/3 of an Astronomical Unit
(AU). An astronomical unit is the average distance from the Earth to the
Sun, about 165 million kilometers. This will be the closest together
Mars and Earth have been in the last 50,000 years!
Oppositions of Mars 1988-2003
This chart by C.F. Chapin shows the
relative positions of Mars and Earth for the years 1988 to 2003. The
last great opposition of Mars was 1988. On August 28, 2003, Mars
will be at its closest approach to Earth in recorded history, at a
distance of only 34,646,418 miles. Click on
image for enlarged view 2003 - A Great Year
to Observe Mars
While the orbit of Earth around the Sun is very nearly circular, the
orbit of Mars is not. During opposition, when the Earth and Mars lie in
line with the Sun, the distance between the two planets varies
considerably from year to year depending on Mars’ position in its orbit.
If Mars comes to opposition when it is farthest from the Sun (at
aphelion), it will lie 61 million miles from Earth. But if Mars reaches
opposition when it is closest to the Sun (at perihelion), it will lie
only 34.6 million miles from Earth. Perihelic oppositions occur every
fifteen to seventeen years. In August and September 2003, Mars will
reach perihelic opposition again. Because of the way Mars’ orbit is
located in space, the very closest oppositions occur when we see
Mars against the stars of Sagittarius and Scorpius, the southernmost
constellations on the ecliptic. Thus, the best oppositions occur
when Mars is too far south for good viewing in the Northern
Hemisphere. This is what happened in 1988: the opposition was very
close, but Mars was low in the sky in the northern hemisphere. But
in 2003, Mars will be higher up, the light from Mars will reach us
via a shorter path through Earth’s atmosphere, and we will have a
better, sharper view of the planet during the current opposition.
Planning for the Public
In planning any special Mars observing activities for the general
public or the media during the 2003 opposition, keep in mind that in
late August when Mars is closest (diameter about 25 arc sec), it
will only rise about 30 degrees above the horizon at midnight ... so
not good for "early evening" observing. However, this situation
improves through September: at end of September, Mars will still be
over 20 arc sec. in diameter, but will cross the meridian (a bit
more than 30 degrees high) earlier ... about 9:30PM. This placement
is somewhat better for public programs.
As always, there is the danger of planet-wide dust storms at this
perihelion. Storm activity on Mars will easily wipe out any surface
features otherwise visible.
The Planetary Society has proclaimed August 27, 2003, the date of
opposition, as "Mars Day". The Planetary Society has a goal of "half
of the world's population looking at, or thinking about, Mars" on
Mars day. So please circle this day on your calendar. Now is the
time to start planning Mars Parties in your local area.
During the June 21, 2001 opposition, Earth and Mars
came within about 42 million miles (67.3 million kilometers) of each
other, the closest they had been since 1988 when they came within 37
million miles (59 million kilometers) of each other. Throughout the
summer that year, and until October when it finally set, Mars was
prominent in the southern sky, visible in the constellation of
Scorpius, and just to
the left of Antares. As the space between Earth and Mars narrowed,
even observers using small, 4 to 6 inch telescopes were able to make
out some of the Martian features, including clouds, surface markings
and polar caps. Unfortunately, this opposition waw marred by
extensive dust storms on the surface of the planet, obscuring
sufrace details from view for most of the opposition.
The Mars viewing gets even better in coming years. On August 27, 2003, Earth will swing to within 34.6 million miles (55.7 million kilometers) of Mars. On that date, the Earth-Mars distance will be the smallest it has been in at least 50,000 years. During
the 2003 opposition, Mars will be located in the constellation
Aquarius.
During the Spring of 1999, Mars could be found in the constellation
Virgo, very bright and up most of the night.
It was in opposition to Earth and at closest approach on May 1, 1999.
During the month of June, 2000, Mars was in conjunction with Saturn behind the Sun, and
was not
visibile from Earth.
Facts about Mars
A . Mars is named after the Roman god of war. It is about half the size of Earth, with about one-tenth the mass.
In some ways, Mars is much like the Earth. It has a similar rotational period and its yearly orbit is only twice
that of Earth’s. However, Mars is much colder than Earth, and its small size has affected its ability to retain
an atmosphere.
B. Mars' atmosphere is very similar in composition to that of Venus, but much thinner. It is thinner because
Mars has a very small gravitational field, and hence cannot hold onto light gasses. The thin CO2 atmosphere therefore
does not contribute greatly to any greenhouse effect. Mars does have polar ice caps which are composed of a combination
of water ice and carbon dioxide ice (dry ice).
C. The dried-out river channels on Mars give evidence that Mars did in fact once have water on its surface.
When Mars was cooling after its initial formation, water vapor was probably outgassed. The water then condensed
into clouds and rained down to the surface to form rivers and lakes. In addition, large quantities of water could
have been released in the form of mud slides and the like. The lack of an ozone layer, however, means that the
water molecules could be easily broken up into their constitutive elements, and these gasses could escape Mars'
small gravitational field. Therefore, Mars now has no water existing in the liquid state. However frozen water
exists in the polar ice caps and as permafrost beneath the surface.
D. Mars has a very thick outer crust. This determines many of its geological features. The largest volcano in
the solar system is on Mars, the Olympus Mons. Its base is approximately the size of the state of Missouri, and
it is more than twice as tall as the largest volcano on Earth. The largest valley in the solar system is also on
Mars. In a region called Tharsis, a massive bulge about 10 Km above the surface has formed. Near this bulge is
the Valles Marineris (named after the Mariner Space Probe which discovered it). The Valles Marineris is long enough
to reach from New York to Los Angeles, and is at some spots, over 4 miles deep. The Tharsis bulge and the Valles
Marineris are thought to be causally related to one another.
E. Mars is red because it has a great deal of oxidized iron on the surface; i.e. because it is rusty.
F. Mars has two small moons, Phobos (fear) and Deimos (panic). Deimos is the smallest cataloged satellite in
the solar system.
Oxidized crystalline rocks on the surface of Mars give it it's tinged blood-red
color. It was natural that the ancient observers linked it with combat and war.
The Babylonians called Mars as Nergal, their God of War. Ares was the brave,
quarrelsome but arrogant Greek God of War. His two sons Phobos and Deimos (Fear
& Panic) accompanied Ares. Appropriately, both the moons of Mars are named after
them. The only other red object in the night sky is a red star in the Scorpio
constellation that was named Antares (Anti-Ares). However, the Roman god Mars enjoyed
the portfolio of both War and Agriculture. So important was Mar to the Romans
that the first month of the Roman year was named March after Mars. Its no
wonder that, even for ancient Indians, Mangal (Mars) represents anger, aggression,
ambition, courage, lust for power, roguery etc. Hindu marriage is not complete
without the Mangal sutra; a necklace made from blood red corrals.
Mars is the only planet in the Solar System besides the Earth that has polar
ice caps. Made of water ice and carbon dioxide, these ice caps expand and recede
seasonally like those on Earth. In the middle of the 19th Century astronomers
described Mars as a hospitable place for life forms.
Manoj Pai, Ahmedabad, Gujurat, India
Earn The Astronomical League's Award for Observing the Solar System
Planetary
Club Rules and Regulations
Comparative Data on the Terrestrial Planets
Quantity |
Earth
|
Mercury
|
Venus
|
Mars
|
Equatorial diameter (Km) |
12756
|
4878
|
12104
|
6794
|
Density (kg/m') |
5517
|
5500
|
5250
|
3933
|
Mass (Earth-1) |
1
|
0.055
|
0.815
|
0.107
|
Surface gravity (Earth=1) |
1
|
0.38
|
0.903
|
0.38
|
Escape velocity (km/s) |
11.2
|
4.3
|
10.36
|
5.03
|
Mean distance from sun (Au) |
1
|
0.3870987
|
0.7233322
|
1.5236915
|
Mean distance from sun (miles) |
9.3x10(7)
|
3.599x10(7)
|
6.7239x10(7)
|
1.4136x10(8)
|
Mean distance from sun (10(6) Km) |
149.6
|
57.9
|
108.2
|
227.9
|
Orbital period (Earth years) |
1
|
0.241
|
0.615
|
1.88
|
Orbital period (Earth days) |
365.24
|
87.97
|
224.68
|
686.95
|
Orbital velocity (Km/sec) |
29.79
|
47.89
|
35.03
|
24.13
|
Avg. Surface Temperature (K) |
280
|
400
|
730
|
210
|
|