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Baby Stars Hatching in Orion's Head

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Baby Stars Hatching in Orion's Head


Helium may act as a "throttle" for the solar wind, setting its minimum speed, according to new results with NASA's Wind spacecraft.

A new image from NASA's Spitzer Space Telescope shows infant stars "hatching" in the head of Orion, the famous hunter constellation visible from northern hemispheres during winter nights. Astronomers suspect that shockwaves from a 3-million-year-old explosion of a massive star may have initiated this newfound birth.

The region featured in the Spitzer image is called Barnard 30. It is located approximately 1,300 light-years away and sits on the right side of Orion's head, just north of the massive star Lambda Orionis.

linked-image
Image above: This image from NASA's
Spitzer Space Telescope shows infant stars
"hatching" in the head of the hunter constellation,
Orion.
Image credit: NASA/JPL-Caltech/ Laboratorio de
Astrofísica Espacial y Física Fundamental


"When we decided to study this region, it was barely known, despite the fact that its properties made it a nice target. Our aim was to carry out a comprehensive study of the region's different properties," said David Barrado y Navascués, of the Laboratorio de Astrofísica Espacial y Física Fundamental in Madrid, Spain, who led the Spitzer observations.

"We now know, thanks to Spitzer, that there is a large population of low-mass stars and brown dwarfs [or failed stars]," he added.

A visibly dark and murky cosmic cloud is bright and clear in Spitzer's infrared image. Organic molecules called polycyclic aromatic hydrocarbons can be seen as wisps of green. These molecules are formed anytime carbon-based materials are burned incompletely. On Earth, they can be found in the sooty exhaust from automobile and airplane engines. They also coat the grills where charcoal-broiled meats are cooked.

Tints of orange-red seen in the cloud are dust particles warmed by the newly forming stars. The reddish-pink dots at the top of the cloud are very young stars embedded in a cocoon of cosmic gas and dust. Blue spots throughout the image are background Milky Way stars along this line of sight.

When Barrado y Navascués first saw this image of Barnard 30, he was so impressed that he decided to use it for the cover of his upcoming astronomy textbook.

"I found the original black and white science images breathtaking, fascinating," said Barrado y Navascués.

"Once I saw the color image, it was clear it had to be the cover of the book. From the aesthetical point of view, [the image] is beautiful, it catches the eye. From the astronomical point of view, it has everything an astronomer wants – high- and low-mass stars, brown dwarfs and a dark dust cloud. It is a gift from nature."

The inspiration for Barrado y Navascués' textbook came from his one-year-old astronomical reference blog, Cuaderno de Bitacora Estelar. The blog is one of the most widely read astronomy blogs in Spanish, with a large audience in Europe, South America and United States. He decided to turn his blog into a textbook a few months ago when a Spanish editorial company asked him to.

"After hesitating and a lot of thinking about how to do it, we decided to go ahead," said Barrado y Navascués. "As far as we know, it is one of the first blogs to be converted into a book in Spanish. It is possibly the first academic blog to undergo such a conversion and, for sure, the first related to astronomy."

As for Barnard 30 and the other infant stars hatching in Orion's head, Barrado y Navascués says that this region "will no doubt become one of the cornerstones of stellar astrophysics, one of the most relevant young stellar clusters."

Media contact: Whitney Clavin 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.


Source: NASA - Spitzer - News

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Young Stars Emerge from Orion's Head

linked-image

This image from NASA's Spitzer Space Telescope shows infant stars "hatching" in the head of the hunter constellation, Orion. Astronomers suspect that shockwaves from a supernova explosion in Orion's head, nearly three million years ago, may have initiated this newfound birth

The region featured in this Spitzer image is called Barnard 30. It is located approximately 1,300 light-years away and sits on the right side of Orion's "head," just north of the massive star Lambda Orionis.

Wisps of green in the cloud are organic molecules called polycyclic aromatic hydrocarbons. These molecules are formed anytime carbon-based materials are burned incompletely. On Earth, they can be found in the sooty exhaust from automobile and airplane engines. They also coat the grills where charcoal-broiled meats are cooked.

Tints of orange-red in the cloud are dust particles warmed by the newly forming stars. The reddish-pink dots at the top of the cloud are very young stars embedded in a cocoon of cosmic gas and dust. Blue spots throughout the image are background Milky Way along this line of sight.

This composite includes data from Spitzer's infrared array camera instrument, and multiband imaging photometer instrument. Light at 4.5 microns is shown as blue, 8.0 microns is green, and 24 microns is red.

Image credit: NASA/JPL-Caltech/ Laboratorio de Astrofísica Espacial y Física Fundamental

+ High-resoluton JPEG

Source: NASA - Spitzer - Multimedia

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Young Stars Emerge from Orion's Head

linked-image

This image from NASA's Spitzer Space Telescope shows infant stars "hatching" in the head of the hunter constellation, Orion. Astronomers suspect that shockwaves from a supernova explosion in Orion's head, nearly three million years ago, may have initiated this newfound birth.

The region featured in this Spitzer image is called Barnard 30. It is located approximately 1,300 light-years away and sits on the right side of Orion's "head," just north of the massive star Lambda Orionis.

Wisps of red in the cloud are organic molecules called polycyclic aromatic hydrocarbons. These molecules are formed anytime carbon-based materials are burned incompletely. On Earth, they can be found in the sooty exhaust from automobile and airplane engines. They also coat the grills where charcoal-broiled meats are cooked.

This image shows infrared light captured by Spitzer's infrared array camera. Light with wavelengths of 8 and 5.8 microns (red and orange) comes mainly from dust that has been heated by starlight. Light of 4.5 microns (green) shows hot gas and dust; and light of 3.6 microns (blue) is from starlight.

Image credit: NASA/JPL-Caltech/ Laboratorio de Astrofísica Espacial y Física Fundamental

+ High-resoluton JPEG

Source: NASA - Spitzer - Multimedia

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