Category Astronomy/Space

Zooming in on Black Holes

As part of the first observations with the new GRAVITY instrument the team looked closely at the bright, young stars known as the Trapezium Cluster, located in the heart of the Orion star-forming region. Already, from these first data, GRAVITY made a discovery: one of the components of the cluster (Theta1 Orionis F) was found to be a double star for the first time. The brighter double star Theta1 Orionis C is also well seen. The background image comes from the ISAAC instrument on ESO's Very Large Telescope. The views of two of the stars from GRAVITY, shown as inserts, reveal far finer detail than could be detected with the NASA/ESA Hubble Space Telescope. Credit: ESO/GRAVITY consortium/NASA/ESA/M. McCaughrean

As part of the first observations with the new GRAVITY instrument the team looked closely at the bright, young stars known as the Trapezium Cluster, located in the heart of the Orion star-forming region. Already, from these first data, GRAVITY made a discovery: one of the components of the cluster (Theta1 Orionis F) was found to be a double star for the first time. The brighter double star Theta1 Orionis C is also well seen. The background image comes from the ISAAC instrument on ESO’s Very Large Telescope. The views of two of the stars from GRAVITY, shown as inserts, reveal far finer detail than could be detected with the NASA/ESA Hubble Space Telescope. Credit: ESO/GRAVITY consortium/NASA/ESA/M. McCaughrean

GRAVITY at ESO’s VLT successfully combined starlight using all 4 Auxiliary Telesc...

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Most Energetic Light ever Observed from a Few Kilometers Large Star

The neutron star (red sphere) with its strong magnetic field (white lines) spins around itself nearly 30 times per second injecting energetic electrons in the space region around it. The green and blue shaded regions depict different particle acceleration zones from where the detected photons could originate. The green zone lies in the vicinity of the pulsar's magnetosphere, whereas the blue zone could be as far as 100,000 km away from the pulsar. Credit: Patricia Carcelén Marco

The neutron star (red sphere) with its strong magnetic field (white lines) spins around itself nearly 30 times per second injecting energetic electrons in the space region around it. The green and blue shaded regions depict different particle acceleration zones from where the detected photons could originate. The green zone lies in the vicinity of the pulsar’s magnetosphere, whereas the blue zone could be as far as 100,000 km away from the pulsar. Credit: Patricia Carcelén Marco

Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) observatory has found the most energetic pulsed emission radiation ever detected from the neutron star in the center of the supernova of 1054 A.D. ie Crab pulsar. It is the corpse left over when the star that created the Crab nebula exploded as a supernova...

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New Images of Dwarf planet Ceres

Kupalo Crater from LAMO. Credit: NASA/JPL

Kupalo Crater from LAMO. Credit: NASA/JPL

Features on dwarf planet Ceres that piqued the interest of scientists throughout 2015 stand out in exquisite detail in the latest images from NASA’s Dawn spacecraft, which recently reached its lowest-ever altitude at Ceres. Dawn took new images near its current altitude of 240 miles from Ceres, between Dec. 19 and 23, 2015.

Kupalo Crater, one of the youngest craters on Ceres, shows off many fascinating attributes at the high image resolution of 120 feet per pixel. The crater has bright material exposed on its rim, which could be salts, and its flat floor likely formed from impact melt and debris. Researchers will be looking closely at whether this material is related to the “bright spots” of Occator Crater...

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The Formation of Carbon-Rich Molecules in Space

The Formation of Carbon-Rich Molecules in Space

A computer simulation of the formation of complex organic molecules in space. The spherical molecular structures forming on the graphene surface at 3000 K are similar in shape to fullerenes. The red atoms originated in the gas phase and the white atoms are from the surface. Credit: Marshall and Sadeghpour

The space between stars is not empty, but contains an abundance of diffuse material, about 5-10% of the total mass of our galaxy (excluding dark matter). Most of the material is gas, predominantly hydrogen, but with a small and important component in complex carbon-bearing molecules including ethene, benzene, propynal, methanol and other alcohols, cyanides, simple amino acids, and even larger molecules (polycyclic aromatic hydrocarbons and buckyballs) with 50 or more carbon atoms...

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