On Monday I asked you to identify this “evening star”. This
is a term that is generally associated with the planet Venus, and has been
since Roman times. However this particular object isn’t Venus, although it
looks very similar to it when seen in this way. I also mentioned that there was
another, smaller, body in this image. This other solar system object is just
below the main planet, although it is hard to see without enhancing the image. These
two objects appear close together in the sky, which doesn’t necessarily mean
that they are close together in space. However in this case they actually are.
This is Earth and its Moon as seen from Mars. The picture was taken by NASA’s
Curiosity Rover. The annotated image below was released by the Curiosity Rover
team, and shows the positions of Earth and the Moon.
It is no surprise that Earth appears as a bright planet in
the martian sky. It is the largest of the terrestrial planets, and at closest
approach Earth and Mars are only 54.6 million kilometres apart. None of the
planets emit their own light, so how easy they are to see when we look up at
the night sky is entirely down to how much sunlight they reflect. This is
controlled by a number of factors. First it is fairly intuitive that larger
planets will reflect more light, and that the closer you are to the sun the
more light there will be to reflect. If Jupiter and Saturn were the size of
Earth they would be much harder to see, but as they are vastly larger they more
than make up for the reduced sunlight in their distant part of the solar
system. Venus is very bright because it is relatively large, close to the sun
and close to the Earth. However Mercury, which is closer to the Sun, is much
darker. This tells us that there is another factor in play, and that it must be
to do with how reflective Mercury and Venus are.
If we look at images of these two planets we can see that
they are very different. Venus is covered with bright clouds, while the surface
of mercury is much darker, covered with solidified lava and potted by meteorites.
The reflectivity of the surface is called its “albedo” and there is a sharp
contrast between that of Mercury and Venus. Every type of surface has an
Albedo, so a planet’s overall reflectivity is the average of the different terrain
types that cover its surface. The clouds of Venus reflect most of the sunlight
which hits them, 75 percent in total. Mercury on the other hand reflects only 6
percent of incident light.
The albedos of Earth and Mars are actually very similar,
although for different reasons. Mars has a lot of bare, redish rock, but also
the bright polar caps, and wisps of cloud in its thin atmosphere. Earth has
much more cloud and ice, but is also covered with a large ocean. The seas are
dark, and so reduce the overall albedo of our planet. Even so Earth comes out
slightly brighter, with an albedo of around 30 percent, compared to 29 percent
for Mars.
From this information we can infer that Earth will look
somewhat brighter in the martian sky than Mars does to us. Their albedos are
similar, and they are obviously the same distance apart. However the earth is
closer to the sun, and substantially larger.
Image Credit:
Earth from Mars: NASA/JPL-Caltech/MSSS/TAMU
https://photojournal.jpl.nasa.gov/catalog/PIA17936
Mercury: https://upload.wikimedia.org/wikipedia/commons/d/d9/Mercury_in_color_-_Prockter07-edit1.jpg
Venus: https://upload.wikimedia.org/wikipedia/commons/e/e5/Venus-real_color.jpg
Further reading:
More about this image here: https://www.space.com/24593-mars-rover-curiosity-sees-earth-photos.html
Brightness of the planets: http://magicvalley.com/lifestyles/recreation/column-a-planet-s-brightness-depends-on-several-factors/article_4bce554f-c310-5071-88d0-e39e68a54da4.html
Albedo of solar system bodies: http://sciencing.com/albedo-planets-5203.html
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