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Science Research at IPAC
Critical to the proper execution of all programs at the Greater IPAC
is a staff of active researchers who can guide the development of
those tasks and subsequently assist other astronomers in using the
final products. These pages are intended to highlight our research
activities and provide links to local and global resources, in the
hope of improving visibility and encouraging collaborations both
within IPAC and with the science community at large.
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Research in the News
New observations from NASA's Spitzer Space Telescope suggest that galaxies prefer to raise stars in cosmic suburbia
rather than in "big cities."
Like big cities on Earth, galaxy clusters are scattered throughout the universe, connected by a web of dusty "highways" called filaments.
For the first time, Spitzer's supersensitive eyes have caught an infrared glimpse of several galaxies traveling along
two filamentary roads into a galaxy cluster called Abell 1763.
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Billions of years ago, small galaxies across the universe regularly collided -- forcing the gas, dust, stars, and black
holes within them to unite. The clashing of galactic gases was so powerful it ignited star formation, while fusing central black
holes developed an insatiable appetite for gas and dust.
Astronomers have long suspected that these merging structures would eventually grow into some of the most massive galaxies in
our universe. Now, NASA's Spitzer Space Telescope has finally identified several of these transitional, or "teenage," galaxies
for further study.
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Astronomers have at last found definitive evidence that the universe's first dust -- the celestial stuff that seeded
future generations of stars and planets -- was forged in the explosions of massive stars.
The findings, made with NASA's Spitzer Space Telescope, are the most significant clue yet in the longstanding mystery of where the
dust in our very young universe came from. Scientists had suspected that exploding stars, or supernovae, were the primary source,
but nobody had been able to demonstrate that they can create copious amounts of dust -- until now. Spitzer's sensitive infrared
detectors have found 10,000 Earth masses worth of dust in the blown-out remains of the well-known supernova remnant Cassiopeia A.
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