Topic: Protostars

NASA’s SOFIA telescope discovers how Swan Nebula was born

January 11, 2020 |

Washington, D.C. – NASA says one of the brightest and most massive star-forming regions in our galaxy, the Omega or Swan Nebula, came to resemble the shape resembling a swan’s neck we see today only relatively recently.

New observations reveal that its regions formed separately over multiple eras of star birth. The new image from the Stratospheric Observatory for Infrared Astronomy, or SOFIA, is helping scientists chronicle the history and evolution of this well-studied nebula.

“The present-day nebula holds the secrets that reveal its past; we just need to be able to uncover them,” said Wanggi Lim, a Universities Space Research Association scientist at the SOFIA Science Center at NASA’s Ames Research Center in California’s Silicon Valley.

Composite image of the Swan Nebula. SOFIA detected the blue areas (20 microns) near the center, revealing gas as it’s heated by massive stars located at the center and the green areas (37 microns) that trace dust as it’s warmed both by massive stars and nearby newborn stars. (NASA/SOFIA/De Buizer/Radomski/Lim; NASA/JPL-Caltech; ESA/Herschel)

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NASA’s Spitzer Telescope sees a Ghoulish Gourd

October 31, 2019 |

Pasadena, CA – A carved-out cloud of gas and dust looks like a celestial jack-o’-lantern in this image from NASA’s Spitzer Space Telescope.

A massive star – known as an O-type star and about 15 to 20 times heavier than the Sun – is likely responsible for sculpting this cosmic pumpkin. A recent study of the region suggests that the powerful outflow of radiation and particles from the star likely swept the surrounding dust and gas outward, creating deep gouges in this cloud, which is known as a nebula.

This high-contrast image from NASA’s Spitzer Space telescope shows a cloud of gas and dust carved out by a massive star. The picture highlights contours in the dust as well as the densest regions of the nebula, which appear brightest. (NASA/JPL-Caltech)

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NASA’s James Webb Telescope to peer into the Center of Milky Way Galaxy

October 15, 2019 |

Greenbelt, MD – The center of our galaxy is a crowded place: A black hole weighing 4 million times as much as our Sun is surrounded by millions of stars whipping around it at breakneck speeds. This extreme environment is bathed in intense ultraviolet light and X-ray radiation. Yet much of this activity is hidden from our view, obscured by vast swaths of interstellar dust.

NASA’s upcoming James Webb Space Telescope is designed to view the universe in infrared light, which is invisible to the human eye, but is very important for looking at astronomical objects hidden by dust.

The center of our Milky Way galaxy is hidden from the prying eyes of optical telescopes by clouds of obscuring dust and gas. But in this stunning vista, the Spitzer Space Telescope’s infrared cameras penetrate much of the dust, revealing the stars of the crowded galactic center region. The upcoming Webb telescope will offer a much-improved infrared view, teasing out fainter stars and sharper details. (NASA, JPL-Caltech, Susan Stolovy (SSC/Caltech) et al.)

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NASA Astronomers puzzle over age of distant Star

August 31, 2016 |

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

Pasadena, CA – For years, astronomers have puzzled over a massive star lodged deep in the Milky Way that shows conflicting signs of being extremely old and extremely young.

Researchers initially classified the star as elderly, perhaps a red supergiant. But a new study by a NASA-led team of researchers suggests that the object, labeled IRAS 19312+1950, might be something quite different — a protostar, a star still in the making.

“Astronomers recognized this object as noteworthy around the year 2000 and have been trying ever since to decide how far along its development is,” said Martin Cordiner, an astrochemist working at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. He is the lead author of a paper in the Astrophysical Journal describing the team’s findings, from observations made using NASA’s Spitzer Space Telescope and ESA’s Herschel Space Observatory.

An age-defying star called IRAS 19312+1950 exhibits features characteristic of a very young star and a very old star. It is the bright red star at the center of this image. (NASA/JPL-Caltech)

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Herschel Space Observatory searches for Massive Stars

March 31, 2013 |

Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory

Pasadena, CA – In this new view of a vast star-forming cloud called W3, the Herschel space observatory tells the story of how massive stars are born. Herschel is a European Space Agency mission with important NASA contributions.

W3 is a giant gas cloud containing an enormous stellar nursery, some 6,200 light-years away in the Perseus Arm, one of our Milky Way galaxy’s main spiral arms.

W3 is an enormous stellar nursery about 6,200 light-years away in the Perseus Arm, one of the Milky Way galaxy’s main spiral arms, which hosts both low- and high-mass star formation. In this image from the Herschel space observatory, the low-mass forming stars are seen as tiny yellow dots embedded in cool red filaments, while the highest-mass stars — with greater than eight times the mass of our sun — emit intense radiation, heating up the gas and dust around them and appearing here in blue. (Image credits: ESA/PACS & SPIRE consortia, A. Rivera-Ingraham & P.G. Martin, Univ. Toronto, HOBYS Key Programme (F. Motte))

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NASA reports Herschel space observatory finds youngest starts to date

March 20, 2013 |

Written by Whitney Clavin
NASA’s Jet Propulsion Laboratory

Pasadena, CA – Astronomers have found some of the youngest stars ever seen, thanks to the Herschel space observatory, a European Space Agency mission with important NASA contributions.

Observations from NASA’s Spitzer Space Telescope and the Atacama Pathfinder Experiment (APEX) telescope in Chile, a collaboration involving the Max Planck Institute for Radio Astronomy in Germany, the Onsala Space Observatory in Sweden, and the European Southern Observatory in Germany, contributed to the findings.

Astronomers have found some of the youngest stars ever seen thanks to the Herschel space observatory, a European Space Agency mission with important NASA contributions. Dense envelopes of gas and dust surround the fledging stars known as protostars, making their detection difficult until now. The discovery gives scientists a window into the earliest and least understood phases of star formation. (Image credit: NASA/ESA/ESO/JPL-Caltech/Max-Planck Institute for Astronomy)

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