| 
  Astronomy Picture of the Day   | 
APOD: 2006 May 15 - Volcanic Bumpy Boulder on Mars 
 Explanation: 
What created this unusually textured rock on Mars?  
 
Most probably: a volcano.  
 
Dubbed Bumpy Boulder, the strange stone measuring just under a 
half-metre high was found by the 
robotic Spirit rover 
currently rolling across Mars.  
 
Pits on the 
ragged rock are likely 
vesicles and arise from hot gas bubbling out of 
hot rock ejected by an active Martian volcano.  
 
Several similar rocks are visible near Bumpy Boulder that 
likely have a similar past. 
 
The above true-colour image was taken about one month ago.  
 
The Spirit rover, now in its third year of operation on Mars, 
is weathering the low sunlight winter of Mar's northern hemisphere on a 
hillside slope in order to maximize the amount of absorbable 
battery-refreshing sunlight.
APOD: 1999 July 5 - Four Faces of Mars 
 Explanation: 
As Mars rotates, most of its surface becomes visible.  During 
Earth's recent pass between Mars and the 
Sun, the 
Hubble Space Telescope was able to 
capture the most detailed time-lapse pictures ever from the 
Earth.  
Dark and light 
sand and gravel create an unusual 
blotted appearance for the 
red planet.  
Winds cause sand-tinted 
features on the 
Martian surface 
to shift over time.  
Visible in the 
above pictures are the north polar cap, made of
water ice and  
dry ice, 
clouds including an 
unusual cyclone, and 
huge volcanoes 
leftover from ancient times.  
The 
Mars Global Surveyor satellite orbiting Mars continues to scan the surface 
for good places to land future robot explorers.
APOD: 2001 July 18 - Mars from Earth  
 Explanation: 
Last month, Mars and Earth were right next 
to each other in their orbits.  
Formally called 
opposition, the event was highlighted by a 
very bright Mars for skywatchers 
and a good photo opportunity for the 
Hubble Space Telescope.  
Above, Hubble snapped the 
highest resolution picture of Mars ever obtained from the 
Earth.  
Visible on 
Mars are 
ice caps over the poles in white, 
regions covered with sand and gravel 
in dark brown and orange, and 
large dust storms in light orange. 
A particularly 
large dust storm 
can be seen on the lower right pouring out of 
Hellas Basin.  
This storm has since 
erupted into a huge planet wide storm 
that continues even today.
Pictures like these allow 
planetary astronomers to continue to 
compare the 
weather patterns of 
Mars and Earth.  
When Mars next 
reaches opposition in 2003, its elliptical orbit will cause it to be even 20 percent closer.
 Authors & editors: 
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
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 NASA Official:  Jay Norris.
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EUD at
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GSFC
& Michigan Tech. U.