Category Astronomy/Space

Looking for Cosmic Superaccelerators

A prototype station of AugerPrime: Every water-Cherenkov detector containing 12,000 l of water is extended by a four-square-meter scintillation detector. Credit: Pierre Auger Collaboration

A prototype station of AugerPrime: Every water-Cherenkov detector containing 12,000 l of water is extended by a four-square-meter scintillation detector. Credit: Pierre Auger Collaboration

The Pierre Auger Observatory in Argentina, an international large-scale experiment to study cosmic rays, will be continued until 2025 and extended to “AugerPrime”. The observatory will be upgraded with new scintillation detectors for a more detailed measurement of gigantic air showers. This is required to identify cosmic objects that accelerate atomic particles up to highest energies.

The Pierre Auger Observatory in the province of Mendoza/Argentina is the world’s biggest and best known project for studying high-energy cosmic rays...

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Hubble Captures a Galactic Waltz

Hubble captures a galactic waltz

Credit: ESA/Hubble & NASA, Acknowledgement: Judy Schmidt

This curious galaxy—only known by the seemingly random jumble of letters and numbers 2MASX J16270254+4328340—has been captured by the NASA/ESA Hubble Space Telescope dancing the crazed dance of a galactic merger. The galaxy has merged with another galaxy leaving a fine mist, made of millions of stars, spewing from it in long trails.

Despite the apparent chaos, this snapshot of the gravitational tango was captured towards the event’s conclusion. This transforming galaxy is heading into old age with its star-forming days coming to an end. The true drama occurred earlier in the process, when the various clouds of gas within the two galaxies were so disturbed by the event that they collapsed, triggering an eruption of star formation...

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Aging Star’s Weight Loss Secret revealed

The star VY Canis Majoris is a red hypergiant, one of the largest known stars in the Milky Way. It is 30-40 times the mass of the Sun and 300 000 times more luminous. In its current state, the star would encompass the orbit of Jupiter, having expanded tremendously as it enters the final stages of its life. New observations of the star using the SPHERE instrument on the VLT have clearly revealed how the brilliant light of VY Canis Majoris lights up the clouds of material surrounding it and have allowed the properties of the component dust grains to be determined better than ever before. In this very close-up view from SPHERE the star itself is hidden behind an obscuring disc. The crosses are artefacts due to features in the instrument. Credit: ESO

The star VY Canis Majoris is a red hypergiant, one of the largest known stars in the Milky Way. It is 30-40 times the mass of the Sun and 300 000 times more luminous. In its current state, the star would encompass the orbit of Jupiter, having expanded tremendously as it enters the final stages of its life. New observations of the star using the SPHERE instrument on the VLT have clearly revealed how the brilliant light of VY Canis Majoris lights up the clouds of material surrounding it and have allowed the properties of the component dust grains to be determined better than ever before. In this very close-up view from SPHERE the star itself is hidden behind an obscuring disc. The crosses are artefacts due to features in the instrument. Credit: ESO

Giant star caught in the act of slimming do...

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Mars to lose its largest moon, Phobos, but gain a Ring

Mars could gain a ring in 10-20 million years when its moon Phobos is torn to shreds by tidal forces due to Mars' gravitational pull. Credit: Image by Tushar Mittal using Celestia 2001-2010, Celestia Development Team.

Mars could gain a ring in 10-20 million years when its moon Phobos is torn to shreds by tidal forces due to Mars’ gravitational pull. Credit: Image by Tushar Mittal using Celestia 2001-2010, Celestia Development Team.

In 10-20 million years, the moon will get so close to Mars that it’ll be shredded into a ring, eventually be torn apart by tidal forces and distributed in a ring around the planet, a study of the cohesiveness of Phobos has concluded. This would take about 10-20 million years, and the ring will persist for up to 100 million years before the dust falls into Mars’ atmosphere and burns up as ‘moon’ showers.

The loss is due to Phobos being highly fractured, with lots of pores and rubble...

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