Mercury
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- Mercury is the closest planet to the sun.
- The planet Mercury has a diameter of 3100 miles.
- At a distance of 36 million miles, it takes 88 days to circle the Sun.
- One day lasts 59 days of Earth time.
Mariner 10 composite image of
Mercury, 1974. PHOTO / NASA |
Mercury is in the daytime sky every day of the year, but because of its close distance to the sun, and because
it is usually washed out in the solar glow, it is one of the most difficult planets to observe.
Mercury can never get more than 28 degrees or two hours from the sun. It is small in angular size, shows no
detail in an amateur telescope, and can be conveniently seen only within an hour after sunset or just before sunrise,
depending on its position in its orbit around the sun. The best times to view Mercury are in the evening sky around
the spring equinox, or in the morning sky, around the autumn equinox.
Mercury is brightest between greatest elongation and superior
conjunction. It should be viewed at greatest elongation
in order to obtain a high sky position. Even so, it is hard to see, since it is easily lost behind trees and rooftops
which surround the average backyard telescope.
Facts about Mercury
A. Mercury is named after the Roman messenger of the gods. Mercury is intermediate in size between the Earth
and the moon. It orbits very close to the sun and so is hard to see. In photographs, Mercury looks like the moon,
in that it is heavily cratered and has no atmosphere. Although it is closest to the sun, Mercury is not the hottest
planet. That distinction belongs to Venus. However, Mercury does have the largest temperature differences of any
planet, varying from -170 degrees C to 430 degrees C.
B. There is a large impact crater on Mercury called the Caloris Basin. On exactly the opposite side of the planet,
there is an area, where the shock waves converge known as the weird terrain.
C. Mercury is made mostly of iron. The percentage of iron in the core of the planet indicates that it may have
been hit in its early developmental stages by a very large object. This impact could have dislodged much of the
lighter materials constituting the planet, and left it as the small iron sphere it is today. The planet also has
long curved ridges called lobate scarps. These cliffs are wrinkles on the surface caused by the slow cooling of
the iron core.
D. Mercury has an odd rotation about the sun. It rotates on its axis one and a half times for each orbit around
the sun. That means there are three days in every two years on Mercury. Furthermore, the orbit of Mercury about
the sun is notable in that it is very elliptical.
It may come as a surprise, but many modern astronomers have never seen Mercury.
It is one planet which can be spotted only if you know where to look. Moving
swiftly through the sky, at maximum elongation it is never more than 28 degrees
from the Sun as seen from Earth. Named after the Roman God of commerce, it is the
closest planet to the Sun and second smallest planet in the Solar system. Its
diameter is 40% smaller than Earth and 40% larger than Moon. It's even smaller
than Jupiter's moon Ganymede and Saturn's moon Titan. Mercury is visible for
weeks in the evening sky and later in the morning sky. When observed at dawn or
dusk, Mercury is so low in the horizon that the light must pass through 10 times
the amount of Earth's atmosphere than it would if Mercury was directly overhead.
Like the moon and planet Venus, Mercury also has it phases, which can be
observed through a standard scope or binoculars. The Hindu god of business, "Booda",
is one of the nine idols of the "Nav Grah" in most Hindu temples.
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
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Mercury
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Venus
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Mars
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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
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Mean distance from sun (Au) |
1
|
0.3870987
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0.7233322
|
1.5236915
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Mean distance from sun (miles) |
9.3x10(7)
|
3.599x10(7)
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6.7239x10(7)
|
1.4136x10(8)
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Mean distance from sun (10(6) Km) |
149.6
|
57.9
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108.2
|
227.9
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Orbital period (Earth years) |
1
|
0.241
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0.615
|
1.88
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Orbital period (Earth days) |
365.24
|
87.97
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224.68
|
686.95
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Orbital velocity (Km/sec) |
29.79
|
47.89
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35.03
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24.13
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Avg. Surface Temperature (K) |
280
|
400
|
730
|
210
|
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