Category Astronomy/Space

Chorus of Black holes Radiates X-rays

Chorus of black holes radiates X-rays

The blue dots in this field of galaxies, known as the COSMOS field, show galaxies that contain supermassive black holes emitting high-energy X-rays. They were detected by NASA’s Nuclear Spectroscopic Array, or NuSTAR, which spotted 32 such black holes in this field and has observed hundreds across the whole sky so far. The other colored dots are galaxies that host black holes emitting lower-energy X-rays, and were spotted by NASA’s Chandra X-ray Observatory. Chandra data show X-rays with energies between 0.5 to 7 kiloelectron volts, while NuSTAR data show X-rays between 8 to 24 kiloelectron volts. Credit: NASA/JPL-Caltech

Supermassive black holes do not give off any of their own light but many black holes pull in, or accrete, surrounding material, and emit powerful bursts of X-rays...

Read More

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)...

Read More

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...

Read More

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...

Read More