Asteroid Vesta Full Frame
Explanation:
Why is the northern half of asteroid Vesta more heavily cratered than the south?
No one is yet sure.
This unexpected mystery has come to light only in the past few weeks since the robotic
Dawn mission became the first
spacecraft to orbit
the second largest object in the
asteroid belt
between Mars and Jupiter.
The northern half of
Vesta, seen on the upper left of the
above image, appears to show some of the densest cratering in the Solar System,
while the southern half is unexpectedly smooth.
Also unknown is the origin of grooves that circle the asteroid nears its equator,
particularly visible on
this Vesta rotation movie,
and the nature of
dark streaks that delineate some of Vesta's craters,
for example the crater just above the
the image center.
As
Dawn spirals in toward
Vesta over the coming months,
some answers may emerge, as well as higher resolution and color images.
Studying 500-km diameter
Vesta is yielding clues
about its history and the early years of our Solar System.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
