[net.astro] StarDate: September 14 Phobos and Mars

dipper@utastro.UUCP (Debbie Byrd) (09/21/84)

The Martian moon Phobos rises in the west -- twice a day.  We'll talk
more about this tiny moon of Mars -- after this.

September 14  Phobos and Mars

The planet Mars has two small moons -- Phobos and Deimos.  The two
Martian moons aren't round like Earth's moon -- they're so irregular
and elongated in shape that they're sometimes called the potato moons.
Phobos and Deimos look very much like small asteroids -- and may really
be asteroids that were captured by the gravity of Mars.

Like Earth's moon, the surfaces of the two Martian moons are heavily
cratered.  Also like Earth's moon, Phobos and Deimos always keep one
face turned toward the larger planet.

The two moons travel almost directly over the equator of Mars -- their
orbits are tilted less than two degrees to the Martian equator.  And
they orbit so close to the planet that an observer near one of the
Martian poles wouldn't be able to see the moons.

Phobos is the larger moon -- and orbits closer to the planet than
Deimos.  When our grandchildren visit Mars on vacations they'll see a
unique sight.  Tiny as it is, Phobos will appear about half the
diameter of our moon -- though not nearly as bright.  But an
extraordinary thing happens because Phobos moves around Mars FASTER
than the planet turns on its axis.  As a result Phobos appears to move
across the dome of the sky from WEST to EAST -- in the opposite
direction from all the other celestial objects -- even its sister
moon!  Twice each Martian day, the moon Phobos rises in the west, takes
about four and a half hours to cross the dome of the Martian sky, and
sets in the east -- the strange case of the backwards moon!

Script by Diana Hadley and Deborah Byrd.

Patrick Moore, "Astronomy Facts & Feats", p.87.  "McGraw-Hill
Encyclopedia of Astronomy," p. 179.

(c) Copyright 1983, 1984 McDonald Observatory, University of Texas at Austin