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New MESSENGER Mercury Images



 
 
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Old October 1st 09, 09:07 PM posted to sci.space.news
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Default New MESSENGER Mercury Images

http://messenger.jhuapl.edu

MESSENGER Mission News
October 1, 2009

NEW MESSENGER MERCURY IMAGES

A Bright Spot in the Latest Imaging

Humans have now had three views of the bright area shown near the top
center of this
image
http://messenger.jhuapl.edu/gallery/...tos/image.php?
gallery_id=2&image_id=336.
The first view was as a mere tiny bright spot seen in telescopic
images
of Mercury obtained from Earth by astronomer Ronald Dantowitz. The
second view
http://messenger.jhuapl.edu/gallery/...tos/image.php?
page=3&gallery_id=2&image_id=236
was obtained by the MESSENGER Narrow Angle Camera during the
spacecraft's
second Mercury flyby on October 6, 2008. At that time, the bright
feature
was just on the planet's limb (edge) as seen from MESSENGER. Now
MESSENGER
has provided a new, even better view. The geometry of MESSENGER's
third
Mercury flyby allows us to see the feature and its surroundings in
greater
detail, including the smooth plains in the foreground and the rim of
a
newly discovered impact basin
http://messenger.jhuapl.edu/gallery/...tos/image.php?
gallery_id=2&image_id=332
at lower left. Surprisingly, at the center of the bright halo is an
irregular
depression, which may have formed through volcanic processes. Color
images
from MESSENGER's Wide Angle Camera reveal that the irregular
depression
and bright halo have distinctive color. This area will be of
particular
interest for further observation during MESSENGER's orbital
operations
starting in 2011.

Evening Shadows

These images
http://messenger.jhuapl.edu/gallery/...tos/image.php?
gallery_id=2&image_id=337
were taken on approach to Mercury during the spacecraft's second
(left)
and third (right) flybys. The image from the second flyby was
featured
in an earlier release
http://messenger.jhuapl.edu/gallery/...tos/image.php?
page=1&gallery_id=2&image_id=287.
The image on the right was taken about 75 minutes before MESSENGER's
closest
approach. The two images cover very nearly the same terrain, but for
the
right image the Suns illumination is more nearly grazing (local time
is almost sunset) and the viewing perspective of the spacecraft is
more
nearly vertical. The large impact crater bisected with a prominent
scarp
or cliff is the same feature in both images. Because of Mercurys
rotation
between the two encounters, the position of the crater in the right
image
is nearly at the terminator (the division between the dayside and
night
side of the planet), and thus the shadows are longer. The near-
grazing
illumination emphasizes the topography of the crater floor, including
the relief of the wrinkle ridges on either side of the large scarp.
To
the west of the crater, the shadows and viewing angle show that the
terrain
is far more rugged than it appeared from the second flyby.

Seeing Double?

This image
http://messenger.jhuapl.edu/gallery/...tos/image.php?
gallery_id=2&image_id=338
shows a double-ring impact basin, with another large impact crater on
its south-southwestern side. Smaller, more recent impacts formed
comparatively
fresh craters across the entire surface visible in this image. The
floor
within the inner or peak ring appears to be smoother than the floor
between
the peak ring and the outer rim, possibly the result of lava flows
that
partially flooded the basin some time after impact. Double-ring
basins
are formed when a large meteoroid strikes the surface of a rocky
planet.

Crater Ejecta and Chains of Secondary Impacts

This newly observed flat-floored crater
http://messenger.jhuapl.edu/gallery/...tos/image.php?
gallery_id=2&image_id=339
was viewed at an oblique angle as MESSENGER approached Mercury for
its
third flyby, about two hours from closest approach. This crater is
younger
than nearby craters of similar size, indicated by the distinctive
halo
of small secondary craters that radiate outward from the central
structure.
Many of these secondaries are aligned in chain-like formations and
some
show characteristic herringbone features pointing back to the crater
of origin. Crater chains are just one of many ejecta types observed
on
Mercury. Other ejecta features include distinct continuous ejecta
http://messenger.jhuapl.edu/gallery/...tos/image.php?
image_id=311
and crater rays
http://messenger.jhuapl.edu/gallery/...tos/image.php?
image_id=280,
which are composed of both ejecta and secondaries. Another ejecta
feature
of note in this mosaic of two images is a zone of lighter terrain
extending
a bit west of north from the crater itself, possibly providing
information
about the direction of impact. This unnamed crater is partially
superposed
on an older and smaller crater to the south.

Additional information and features from this encounter will be
available
online at http://messenger.jhuapl.edu/mer_flyby3.html.
Be sure to check back frequently to see the latest released images
and
science results!

________________________________

Highlights from Three Mercury Flybys

Tonight, three MESSENGER team members - Principal Investigator
Sean Solomon, of the Carnegie Institution of Washington, Project
Manager
Peter Bedini, of APL, and Co-Investigator Louise Prockter, of APL -
will
talk about what we've learned about Mercury from MESSENGER's
encounters
with the planet, and release new pictures from the spacecraft's third
flyby of Mercury. The event, to be held at the Kossiakoff Center on
the
campus of the Johns Hopkins University Applied Physics Laboratory in
Laurel,
Md., will begin at 5 p.m.
________________________________

MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and
Ranging)
is a NASA-sponsored scientific investigation of the planet Mercury
and
the first space mission designed to orbit the planet closest to the
Sun.
The MESSENGER spacecraft launched on August 3, 2004, and after flybys
of
Earth, Venus, and Mercury will start a yearlong study of its target
planet in March 2011. Dr. Sean C. Solomon, of the Carnegie
Institution
of Washington, leads the mission as Principal Investigator. The Johns
Hopkins University Applied Physics Laboratory built and operates the
MESSENGER spacecraft and manages this Discovery-class mission for
NASA.

________________________________



 




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