Wednesday, October 5, 2016

SOFIA Detects Collapsing Clouds Becoming Young Suns

An infrared image of the W43 star-forming region located 20,000 light years away in the direction of the constellation Aquila, one of the places where Wyrowski et al. detected cloud clumps collapsing to become massive stars. Credits: NASA/JPL-Caltech/2MASS

Researchers on board NASA’s Stratospheric Observatory for Infrared Astronomy, SOFIA, observed the collapse of portions of six interstellar clouds on their way to becoming new stars that will be much larger than our sun. When a gas cloud collapses on itself, the cloud’s own gravity causes it to contract and the contraction produces heat friction. Heat from the contraction eventually causes the core to ignite hydrogen fusion reactions creating a star.

Astronomers are excited about this SOFIA research because there have been very few previous direct observations of collapse motion. These SOFIA observations have enabled scientists to confirm theoretical models about how interstellar clouds collapse to become stars and the pace at which they collapse. Actually observing this collapse, called “infall,” is extremely challenging because it happens relatively quickly in astronomical terms.

“Detecting infall in protostars is very difficult to observe, but is critical to confirm our overall understanding of star formation,” said Universities Space Research Association’s Erick Young, SOFIA Science Mission Operations director.

Using the observatory’s GREAT instrument, the German Receiver for Astronomy at Terahertz Frequencies, scientists searched for this developmental stage in nine embryonic stars, called protostars, by measuring the motions of the material within them. They found that six of the nine protostars were actively collapsing, adding substantially to the previous list of less than a dozen protostars directly determined to be in this infall stage.

For several weeks each year, the SOFIA team operates from Christchurch, New Zealand, to study objects best observed from southern latitudes, including the complete center of the Milky Way where many star-forming regions are located. Heading south during the Southern Hemisphere’s winter months, when the nights are long and infrared-blocking water vapor is especially low, also creates prime observing conditions.

“With the Southern Hemisphere deployments of SOFIA, the full inner Milky Way comes into reach for star formation studies. This is crucial for observations of the earliest phases of high-mass star formation, since this is a relatively rapid and rare event,” said Friedrich Wyrowski, astronomer at the Max-Planck Institute for Radio Astronomy in Bonn, Germany.

The results were from observations made in the Southern Hemisphere in 2015, and were published in Astronomy and Astrophysics earlier this year. SOFIA spent seven weeks during 2016 observing from Christchurch. The scientific teams involved in the Southern Hemisphere observations are analyzing the acquired data now.

SOFIA is a Boeing 747SP jetliner modified to carry a 100-inch diameter telescope. It is a joint project of NASA and the German Aerospace Center, DLR. NASA’s Ames Research Center in California’s Silicon Valley manages the SOFIA program, science and mission operations in cooperation with the Universities Space Research Association headquartered in Columbia, Maryland, and the German SOFIA Institute (DSI) at the University of Stuttgart. The aircraft is based at NASA’s Armstrong Flight Research Center's Hangar 703, in Palmdale, California.

Credit: NASA

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