Category Astronomy/Space

The Role of Magnetic fields in Star Formation

The role of magnetic fields in star formation

A false-color far-infrared image of the star forming region W43; the contours are for molecular gas density. The subregion MM1 located just left of center in not conspicuous in the image but is the site of massive star formation and fragmentation. A new study has mapped the magnetic fields in this region, and found they are not strong enough to prevent further gravitational collapse. Credit: ESA/Herschel and L.Q. Nguyen et al

Star forming molecular clump W43-MM1 is very massive and dense, containing about 2100 solar masses of material in a region only 1/3 of a light year across (for comparison, the nearest star to the Sun is a bit over four light years away)...

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White Dwarf Lashes Red Dwarf with Mystery Ray

This artist's impression shows the strange object AR Scorpii. In this unique double star a rapidly spinning white dwarf star (right) powers electrons up to almost the speed of light. These high energy particles release blasts of radiation that lash the companion red dwarf star (left) and cause the entire system to pulse dramatically every 1.97 minutes with radiation ranging from the ultraviolet to radio. Credit: M. Garlick/University of Warwick, ESA/Hubble

This artist’s impression shows the strange object AR Scorpii. In this unique double star a rapidly spinning white dwarf star (right) powers electrons up to almost the speed of light. These high energy particles release blasts of radiation that lash the companion red dwarf star (left) and cause the entire system to pulse dramatically every 1.97 minutes with radiation ranging from the ultraviolet to radio. Credit: M. Garlick/University of Warwick, ESA/Hubble

Astronomers using Hubble along with other telescopes on the ground and in space, have discovered a new type of exotic binary star: in the system AR Scorpii a rapidly spinning white dwarf star is powering electrons up to almost the speed of light...

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Jupiter’s Great Red Spot Heats planet’s Upper Atmosphere

Close-up of Jupiter's Great Red Spot. Credit: NASA/JPL

Close-up of Jupiter’s Great Red Spot. Credit: NASA/JPL

Scientists answer elusive question in new study. Researchers from Boston University’s (BU) Center for Space Physics report today in Nature that Jupiter’s Great Red Spot may provide the mysterious source of energy required to heat the planet’s upper atmosphere to the unusually high values observed.

Sunlight reaching Earth efficiently heats the terrestrial atmosphere at altitudes well above the surface – even at 250 miles high, for example, where the International Space Station orbits. Jupiter is >5X more distant from the Sun, and yet its upper atmosphere has temperatures, on average, comparable to those found at Earth...

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Puzzling Paucity of Large Craters on Dwarf Planet Ceres

The top of this false-color image includes a grazing view of Kerwan, Ceres' largest impact crater. This well-preserved crater is 280 km (175 miles) wide and is well defined with red-yellow high-elevation rims and a deep central depression shown in blue. Kerwan gradually degrades as one moves toward the center of the image into an 800-km (500-mile) wide, 4-km (2.5-mile) deep depression (in green) called Vendimia Planitia. This depression is possibly what's left of one of the largest craters from Ceres' earliest collisional history. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

The top of this false-color image includes a grazing view of Kerwan, Ceres’ largest impact crater. This well-preserved crater is 280 km (175 miles) wide and is well defined with red-yellow high-elevation rims and a deep central depression shown in blue. Kerwan gradually degrades as one moves toward the center of the image into an 800-km (500-mile) wide, 4-km (2.5-mile) deep depression (in green) called Vendimia Planitia. This depression is possibly what’s left of one of the largest craters from Ceres’ earliest collisional history. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Dwarf planet may continuously refresh its surface...

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