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Hubble Takes A Close-Up View Of A Reflection Nebula In Orion

Date:
March 6, 2000
Source:
Space Telescope Science Institute
Summary:
Just weeks after NASA astronauts repaired the Hubble Space Telescope in December 1999, the Hubble Heritage Project snapped a picture of NGC 1999, a nebula in the constellation Orion. The Heritage astronomers, in collaboration with scientists in Texas and Ireland, used Hubble's Wide Field Planetary Camera 2 (WFPC2) to obtain the color image.

Just weeks after NASA astronauts repaired the Hubble Space Telescope in December 1999, the Hubble Heritage Project snapped this picture of NGC 1999, a nebula in the constellation Orion. The Heritage astronomers, in collaboration with scientists in Texas and Ireland, used Hubble's Wide Field Planetary Camera 2 (WFPC2) to obtain the color image.

NGC 1999 is an example of a reflection nebula. Like fog around a street lamp, a reflection nebula shines only because the light from an embedded source illuminates its dust; the nebula does not emit any visible light of its own. NGC 1999 lies close to the famous Orion Nebula, about 1,500 light-years from Earth, in a region of our Milky Way galaxy where new stars are being formed actively. The nebula is famous in astronomical history because the first Herbig-Haro object was discovered immediately adjacent to it (it lies just outside the new Hubble image). Herbig-Haro objects are now known to be jets of gas ejected from very young stars.

The NGC 1999 nebula is illuminated by a bright, recently formed star, visible in the Hubble photo just to the left of center. This star is cataloged as V380 Orionis, and its white color is due to its high surface temperature of about 10,000 degrees Celsius (nearly twice that of our own Sun). Its mass is estimated to be 3.5 times that of the Sun. The star is so young that it is still surrounded by a cloud of material left over from its formation, here seen as the NGC 1999 reflection nebula.

The WFPC2 image of NGC 1999 shows a remarkable jet-black cloud near its center, resembling a letter T tilted on its side, located just to the right and lower right of the bright star. This dark cloud is an example of a "Bok globule," named after the late University of Arizona astronomer Bart Bok. The globule is a cold cloud of gas, molecules, and cosmic dust, which is so dense it blocks all of the light behind it. In the Hubble image, the globule is seen silhouetted against the reflection nebula illuminated by V380 Orionis. Astronomers believe that new stars may be forming inside Bok globules, through the contraction of the dust and molecular gas under their own gravity.

NGC 1999 was discovered some two centuries ago by Sir William Herschel and his sister Caroline, and was cataloged later in the 19th century as object 1999 in the New General Catalogue.

These data were collected in January 2000 by the Hubble Heritage Team with the collaboration of star-formation experts C. Robert O'Dell (Rice University), Thomas P. Ray (Dublin Institute for Advanced Study), and David Corcoran (University of Limerick).

Image Credit: NASA and the Hubble Heritage Team (STScI)

NOTE TO EDITORS -- For additional information, please contact: Professor C. R. O'Dell, Rice University, MS 108, PO Box 1892, Houston, Texas 77251-1892, (phone) 713-348-3633, (fax) 713-348-5143, (e-mail) cro@rice.edu or

Professor T.P. Ray, School Of Cosmic Physics, Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland, (phone) +353 1 6621333, (fax) +353 1 6621477, (e-mail) tr@cp.dias.ie or

Keith Noll, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Md. 21218, (e-mail) noll@stsci.edu.

Image files are available on the Internet at:http://heritage.stsci.eduhttp://oposite.stsci.edu/pubinfo/pr/2000/10 or via links inhttp://oposite.stsci.edu/pubinfo/latest.html andhttp://oposite.stsci.edu/pubinfo/pictures.html

Higher resolution digital versions (300 dpi JPEG and TIFF) are available at:http://oposite.stsci.edu/pubinfo/pr/2000/10/pr-photos.html

STScI press releases and other information are available automatically by sending an Internet electronic mail message to public-request@stsci.edu. Leave the subject line blank. In the body of the message (not the subject line) users should type the word "subscribe" (don't use quotes). The system will respond with a confirmation of the subscription, and users will receive new press releases as they are issued. Please subscribe using the email account with which you would like to receive list messages. To unsubscribe, send mail to public-request@stsci.edu. Leave the subject line blank. Type "unsubscribe" (don't use quotes) in the body of the message. Please unsubscribe using the email account that you used to subscribe to the list.


Story Source:

The above story is based on materials provided by Space Telescope Science Institute. Note: Materials may be edited for content and length.


Cite This Page:

Space Telescope Science Institute. "Hubble Takes A Close-Up View Of A Reflection Nebula In Orion." ScienceDaily. ScienceDaily, 6 March 2000. <www.sciencedaily.com/releases/2000/03/000306082320.htm>.
Space Telescope Science Institute. (2000, March 6). Hubble Takes A Close-Up View Of A Reflection Nebula In Orion. ScienceDaily. Retrieved September 20, 2014 from www.sciencedaily.com/releases/2000/03/000306082320.htm
Space Telescope Science Institute. "Hubble Takes A Close-Up View Of A Reflection Nebula In Orion." ScienceDaily. www.sciencedaily.com/releases/2000/03/000306082320.htm (accessed September 20, 2014).

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