|
June
2, 2000 -- There will be two good times to see the elusive
planet Mercury this year, and next week is one of them.
Mercury is the solar system's innermost planet, so it never strays
very far in the sky from the blinding glare of the Sun. Its angular
separation from the Sun (or elongation) is always less
than 28 degrees. Mercury approaches its maximum eastern elongation
on June 9, 2000. It will be 24 degrees from the Sun, appearing
as a bright zero-magnitude object above the western horizon after
sunset.
Above: Artist Duane Hilton's rendition of the close
encounter between the Moon and Mercury after sunset on Saturday,
June 3, 2000. The setting is Yosemite National Park in north-central
California. The Moon and Mercury will appear close together in
the sky, but they are really very far apart. On June 3, Mercury
will be 139 million km from Earth while the Moon is only 359
thousand km away.
Although Mercury will be a little farther from the Sun
on June 9, the best time to look will be six days earlier on
Saturday evening, June 3. That's when the slender crescent Moon
will pass less than 3 degrees from the planet. All you need to
see the show is a clear view of the western horizon. Go outside
just after sunset and look west-northwest. Mercury will appear
to the upper right of the Moon's waxing crescent for observers
at mid-latitudes in both hemispheres.
While you're enjoying the rare appearance of Mercury in plain
view, don't miss another notable sight: cradled in the arms of
the slim crescent Moon will appear the ghostly outline of the
full Moon, a dim glow that astronomers call "Earthshine."
Like all the planets we see in the night sky, including
Mercury, the Moon does not shine by its own light. It reflects
sunlight. The side of the Moon facing the Sun shines brightly;
the side facing away is nearly dark. The only significant illumination
on the "dark side of the Moon" is due to Earthshine
-- sunlight that bounces off the Earth and falls on the lunar
surface. A slender crescent Moon with Earthshine is widely regarded
as one of the most delicate and beautiful sights in the night
sky.
"The
phase of the Earth as seen from the Moon is nearly full when
the Moon is crescent," says Dr. George Lebo, a Marshall
Space Flight Center 2000 Summer Faculty Fellow. "Because
the Earth is four times bigger than the Moon and is a ten times
better reflector, the 'Full Earth' is 160 times brighter than
the 'Full Moon.' That's why earthshine is so noticeable."
Left: The western sky on June 9, 2000, just after sunset
at mid-Northern latitudes. Mercury appears in the constellation
Gemini about 14 degrees above the WNW horizon to mid-latitude
observers in both hemispheres.
Now that you've spotted Mercury using the Moon as a finder on
June 3, you can watch Mercury's progress in the sky throughout
the month. In early June, Mercury will remain at about the same
height above the horizon each night if you look at the same time.
After the 10th, the planet will head back toward the Sun. By
the third week of June, Mercury will be almost impossible to
find as it becomes lost in the Sun's glare.
After June, the best time this year to spot Mercury from northern
latitudes will be in mid-November when the planet is 14 degrees
over the horizon before sunrise.
THE UPS AND DOWNS OF MERCURY
Mercury approaches maximum elongation six times in the year 2000,
but each time is not an equally good opportunity to see the planet.
If the ecliptic plane (the path in the sky followed by the Sun
and planets) is nearly parallel to the horizon when the Sun sets
or rises, Mercury can be at a low altitude even when its elongation
is large. That's what happens on October 6, 2000, when Mercury
is 25 degrees from the Sun, but only about 4 degrees above the
horizon at sunset for observers at mid-Northern latitudes. Dates
marked in red denote the best times to spot Mercury during the
remainder of 2000.
|
dates of maximum elongation for Mercury |
elongation |
morning or evening star |
altitude at sunrise/sunset
(as seen from mid-Northern latitudes) |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
Mysterious Mercury
If it's any consolation to the often-frustrated Earthbound
observers of Mercury, NASA spacecraft have a hard time, too.
For instance, ground controllers can't point the Hubble Space
Telescope toward Mercury because small pointing errors might
allow intense sunlight to damage sensitive cameras. The only
spacecraft to explore Mercury close-up was Mariner 10, which
executed 3 flybys of Mercury in 1974 and 1975, surveying just
45 percent of its surface.
Last
week, astronomers from Boston University announced that they
had captured unprecedented ground-based pictures of Mercury covering
parts of the planet's surface that Mariner 10 missed. The images,
taken at the Mt. Wilson Observatory in California, revealed surface
markings similar to the bright craters and dark maria ("seas")
found on the Moon. [Boston
University Press Release]
Right: This image of a portion of Mercury's surface
not photographed by Mariner 10 in 1974-75 was obtained by Boston
University astronomers using observations made at the Mt. Wilson
Observatory in August 1998. Hundreds of thousands of pictures
taken with short time exposures (1/60th) were examined to find
the 30 images with the clearest surface markings, taken during
instances of "perfect seeing" through the Earth's atmosphere.
The Boston team plans to make more observations this fall. They
might even succeed in detecting sodium in Mercury's wispy atmosphere,
which consists of atoms blasted off its surface by the solar
wind. Because the planet is so hot, these atoms quickly escape
into space. In contrast to the stable atmospheres of Earth and
Venus, Mercury's atmosphere is constantly being replenished.
Mercury's dynamic atmosphere is just one of the planet's many
exotic aspects. Mercury's density is the higher than any planet
except the Earth -- its iron core is probably bigger than Earth's
entire Moon! It is the only terrestrial planet besides Earth
to possess a global magnetic field. Temperatures on the surface
of Mercury vary from nearly the highest in the solar system at
the equator to among the coldest in permanently shadowed areas
at the poles. Radar data suggest that fiery Mercury, like the
Moon, actually harbors polar deposits of ice.
In 2004, scientists hope to launch a satellite called MESSENGER
(MErcury: Surface, Space ENvironment, GEochemistry and Ranging)
to study Mercury in greater detail. The spacecraft is slated
to enter orbit around Mercury in 2009 carrying instruments to
answer the following questions:
- What is the origin of Mercury's high density?
- What are the composition and structure of its crust?
- What is Mercury's tectonic history, and is its surface shaped
by volcanism?
- What is the nature and origin of Mercury's magnetic field?
- What are the characteristics of the thin atmosphere and miniature
magnetosphere?
- What is the nature of the mysterious polar caps?
If all goes as planned, MESSENGER will get the closest, clearest
view ever of the solar system's innermost planet.
Above: This mosaic of Mariner 10 images shows that Mercury's
surface looks similar to our Moon's. Each is heavily cratered
and made of rock. Mercury's diameter is about 4800 km, while
the Moon's is slightly less at about 3500 km (compared with about
12,700 km for the Earth). Mercury is the closest planet to the
Sun, orbiting at about 1/3 the radius of the Earth's orbit. As
Mercury slowly rotates, its surface temperature varies from an
unbearably cold -180 degrees Celsius to an unbearably hot 400
degrees Celsius. [more
information]
The MESSENGER mission is managed for NASA by the Johns
Hopkins University Applied Physics Laboratory in Laurel, MD.
The Principal Investigator is Dr. Sean C. Solomon of the Carnegie
Institution of Washington. For more complete information on the
mission, including animations of the trajectory to Mercury with
flybys of Earth, Venus, and Mercury, visit the MESSENGER
home page.
Editor's note: the opening line of this story was inspired by
a recent episode of Jack Horkheimer's PBS program "Stargazer." |