Rho Ophiuchi monograph - scitechlab.files.wordpress.comRho Ophiuchi Cloud SciTechLab.com Monograph...
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Rho Ophiuchi Cloud SciTechLab.com Monograph ASM-0001 (2/23/08) Edited by Robert Reuss This free monograph and a poster for purchase are available from: http://www.SciTechLab.com/ Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope. Called "Rho Oph" by astronomers, it's one of the closest star-forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a region made up of a large main cloud of molecular hydrogen, a key molecule allowing new stars to form from cold cosmic gas, with two long streamers trailing off in different directions. Recent studies using the latest X-ray and infrared observations reveal more than 300 young stellar objects within the large central cloud. Their median age is only 300,000 years, very young compared to some of the universe's oldest stars, which are more than 12 billion years old. "Rho Oph is a favorite region for astronomers studying star formation. Because the stars are so young, we can observe them at a very early evolutionary stage, and because the Ophiuchus molecular cloud is relatively close, we can resolve more detail than in more distant clusters, like Orion," said Lori Allen, lead investigator of the new observations, from the Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass. This false-color image of Rho Oph's main cloud, Lynds 1688, was created with data from Spitzer's infrared array camera, which has the highest spatial resolution of Spitzer's three imaging instruments, and its multiband imaging photometer, best for detecting cooler materials. Blue represents 3.6-micron light; green shows light of 8 microns; and red is 24-micron light. The multiple wavelengths reveal different aspects of the dust surrounding and between the embedded stars, yielding information about the stars and their birthplace. The colors in this image reflect the relative temperatures and evolutionary states of the various stars. The youngest stars are surrounded by dusty disks of gas from which they, and their potential planetary systems, are forming. These young disk systems show up as red in this image. Some of these young stellar objects are surrounded by their own
Transcript of Rho Ophiuchi monograph - scitechlab.files.wordpress.comRho Ophiuchi Cloud SciTechLab.com Monograph...
Rho Ophiuchi Cloud
SciTechLab.com Monograph ASM-0001 (2/23/08)Edited by Robert Reuss
This free monograph and a poster for purchase are available from: http://www.SciTechLab.com/
Newborn stars peek out from beneath their natal blanket of dust in this dynamic imageof the Rho Ophiuchi dark cloud from NASA's Spitzer Space Telescope.
Called "Rho Oph" by astronomers, it's one of the closest star-forming regions to ourown solar system. Located near the constellations Scorpius and Ophiuchus, the nebula isabout 407 light years away from Earth.
Rho Oph is a region made up of a large main cloud of molecular hydrogen, a keymolecule allowing new stars to form from cold cosmic gas, with two long streamerstrailing off in different directions. Recent studies using the latest X-ray and infraredobservations reveal more than 300 young stellar objects within the large central cloud.Their median age is only 300,000 years, very young compared to some of the universe'soldest stars, which are more than 12 billion years old.
"Rho Oph is a favorite region for astronomers studying star formation. Because thestars are so young, we can observe them at a very early evolutionary stage, and becausethe Ophiuchus molecular cloud is relatively close, we can resolve more detail than inmore distant clusters, like Orion," said Lori Allen, lead investigator of the newobservations, from the Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.
This false-color image of Rho Oph's main cloud, Lynds 1688, was created with data fromSpitzer's infrared array camera, which has the highest spatial resolution of Spitzer's threeimaging instruments, and its multiband imaging photometer, best for detecting coolermaterials.
Blue represents 3.6-micron light; green shows light of 8 microns; and red is 24-micronlight. The multiple wavelengths reveal different aspects of the dust surrounding andbetween the embedded stars, yielding information about the stars and their birthplace.
The colors in this image reflect the relative temperatures and evolutionary states of thevarious stars. The youngest stars are surrounded by dusty disks of gas from which they,and their potential planetary systems, are forming. These young disk systems show up asred in this image. Some of these young stellar objects are surrounded by their own
Rho Ophiuchi Cloud
SciTechLab.com Monograph ASM-0001 (2/23/08)Edited by Robert Reuss
This free monograph and a poster for purchase are available from: http://www.SciTechLab.com/
compact nebulae. More evolved stars, which have shed their natal material, are blue.
The extended white nebula in the center right of the image is a region of the cloudglowing in infrared light due to the heating of dust by bright young stars near the cloud'sright edge. Fainter multi-hued diffuse emission fills the image. The color of thenebulosity depends on the temperature, composition and size of the dust grains. Most ofthe stars forming now are concentrated in a filament of cold, dense gas that shows up asa dark cloud in the lower center and left side of the image against the bright backgroundof the warm dust. Although infrared radiation at 24 microns pierces through dust easily,this dark filament is incredibly opaque, appearing dark even at the longest wavelengths inthe image.
NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Spitzer SpaceTelescope mission for NASA's Science Mission Directorate, Washington. Scienceoperations are conducted at the Spitzer Science Center at the California Institute ofTechnology, also in Pasadena. Caltech manages JPL for NASA.
Spitzer's infrared array camera was built by NASA's Goddard Space Flight Center,Greenbelt, Md. The instrument's principal investigator is Giovanni Fazio of the Harvard-Smithsonian Center for Astrophysics. The multiband imaging photometer for Spitzerwas built by Ball Aerospace Corporation, Boulder, Colo.; the University of Arizona; andBoeing North American, Canoga Park, Calif. Its principal investigator is George Rieke ofthe University of Arizona, Tucson.
About the Object Object Name: Rho OphObject Type: Star Forming RegionPosition (J2000): RA: 16h27m12.5s Dec:: -24d19m30sDistance: 125 pc, 407 light-yearsConstellation: Ophiuchus / Scorpius
About the Data Text Credit: NASA/JPL/Rosemary SullivantImage Credit: NASA/JPL-Caltech/L. Allen (Harvard-Smithsonian Center for Astrophysics)Instrument: IRAC and MIPSExposure Date: March 7, 18, 19, 2004Exposure Time: IRAC - 48 seconds per position; MIPS - 30 seconds per positionRelease Date: February 11, 2007Page URL: http://www.spitzer.caltech.edu/Media/releases/ssc2008-03/index.shtml
Observers G.G. Fazio (Harvard-Smithsonian Center for Astrophysics)P.C. Myers (Harvard-Smithsonian Center for Astrophysics)L. Allen (Harvard-Smithsonian Center for Astrophysics)S.T. Megeath (University of Toledo)E.T. Young (University of Arizona)J. Muzerolle (University of Arizona)N.J. Evans II (University of Texas)G.A. Blake (Caltech)P.M. Harvey (University of Colorado)D.W. Koerner (Northern Arizona University)L.G. Mundy (University of Maryland)D.L. Padgett (Spitzer Science Center)A.I. Sargent (Caltech)K.R. Stapelfeldt (JPL)E.F. van Dishoeck (Leiden University)
