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Mini-Me' Solar System
by NASA/JPL-Caltech/T. Pyle (SSC)
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This artist's conception shows the relative size of a
hypothetical brown dwarf-planetary system (below)
compared to our own solar system. A brown dwarf is a cool
or "failed" star, which lacks the mass to ignite and
shine like our Sun. NASA's Spitzer Space Telescope set
its infrared eyes on an extraordinarily low-mass brown
dwarf called OTS 44 and found a swirling disk of planet-
building dust. At only 15 times the mass of Jupiter, OTS
44 is the smallest known brown dwarf to host a planet-
forming, or protoplanetary, disk. Astronomers believe
that this unusual system will eventually spawn planets.
If so, they speculate that OTS 44's disk has enough mass
to make one small gas giant and a few Earth-sized rocky
planets. Examples of these possible planets are depicted
at the bottom of this picture, circling a low-mass brown
dwarf. Above, the bodies of our own solar system have
been drawn to the same scale. In each system, the
terrestrial planets have been enlarged and the distances
between the planets and their parent bodies have been
scaled down for easier viewing.
Date Published: 2009-10-06 05:39:39
Identifier: SPITZ-ssc2005-06c
Item Size: 205756
Media Type: image
# Topics
What -- Sun
What -- Spitzer Space Telescope
What -- OTS
What -- Jupiter
What -- Earth
# Collections
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spitzerspacetelescopecollection
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