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Astronomy / Space Science - 15.11.2018
Astronomy / Space Science - 14.11.2018
Physics - Astronomy / Space Science - 05.10.2018
Astronomy / Space Science - 25.07.2018
Astronomy / Space Science - 12.07.2018
Chemistry - Astronomy / Space Science - 28.06.2018
Astronomy / Space Science - 17.06.2018
Astronomy / Space Science - 20.04.2018
Astronomy / Space Science - 06.04.2018
Astronomy/Space Science
Results 1 - 9 of 9.
Our stellar neighbourhood expands
Astronomers from the Observatory of the University of Hamburg were involved in the discovery of a new planet. As part of an international research team led by the Institut de Cičncies de l'Espai (ICE, CSIC), they have found a planet in orbit of Barnard's star. Barnard's star is a so-called red dwarf and after the Alpha-Centauri triple stellar system the second closest star to the Sun.
Astronomers from the Observatory of the University of Hamburg were involved in the discovery of a new planet. As part of an international research team led by the Institut de Cičncies de l'Espai (ICE, CSIC), they have found a planet in orbit of Barnard's star. Barnard's star is a so-called red dwarf and after the Alpha-Centauri triple stellar system the second closest star to the Sun.
Newly discovered planet sets Barnard’s Star in motion
International team unveils Super Earth at second closest star to the Earth. Scientists have discovered a planet in the orbit of Barnard's Star, which is about six light years from us. They assume that the planet, which has about 3.2 times as much mass as Earth, orbits the star. This was discovered by an international team involving the University of Göttingen.
International team unveils Super Earth at second closest star to the Earth. Scientists have discovered a planet in the orbit of Barnard's Star, which is about six light years from us. They assume that the planet, which has about 3.2 times as much mass as Earth, orbits the star. This was discovered by an international team involving the University of Göttingen.
Mission Cassini: Nano Dust Rain from Saturn’s Rings
Findings Published in "Science" No 260/2018 from Oct 05, 2018 Nanometer-sized particles of dust are whirling in the gap between the planet Saturn and its rings, as shown by experiments following the grand finale of the Cassini spacecraft, which burned out in 2017. The particles consist of water ice and silicates, and according to the latest measurements, they come from Saturn's rings.
Findings Published in "Science" No 260/2018 from Oct 05, 2018 Nanometer-sized particles of dust are whirling in the gap between the planet Saturn and its rings, as shown by experiments following the grand finale of the Cassini spacecraft, which burned out in 2017. The particles consist of water ice and silicates, and according to the latest measurements, they come from Saturn's rings.
How to Weigh Stars With Gravitational Lensing
Using data from Gaia astrometry satellite, astronomers at Heidelberg University investigated the movement of millions of stars in the Milky Way galaxy. For the first time, they were able to predict the approach of two stars with extreme precision and to forecast characteristic effects of relativistic light deflection that can be used to precisely measure the mass of stars.
Using data from Gaia astrometry satellite, astronomers at Heidelberg University investigated the movement of millions of stars in the Milky Way galaxy. For the first time, they were able to predict the approach of two stars with extreme precision and to forecast characteristic effects of relativistic light deflection that can be used to precisely measure the mass of stars.
First evidence on the source of extragalactic particles
Research news For the first time ever, scientists have determined the cosmic origin of highest-energy neutrinos. A research group led by Prof. Elisa Resconi from the Technical University of Munich (TUM), provides an important piece of evidence that the particles detected by the IceCube neutrino telescope at the South Pole originate from a galaxy four billion light-years away from Earth.
Research news For the first time ever, scientists have determined the cosmic origin of highest-energy neutrinos. A research group led by Prof. Elisa Resconi from the Technical University of Munich (TUM), provides an important piece of evidence that the particles detected by the IceCube neutrino telescope at the South Pole originate from a galaxy four billion light-years away from Earth.
Complex Organic Molecules On Saturn’s Moon Enceladus
Under its icy crust, Saturn's moon Enceladus conceals an global ocean of liquid water. A detector on the Cassini space probe detected ice particles propelled from Enceladus that contain high concentrations of organic substances. They exhibit the structures typical of highly complex macromolecular compounds.
Under its icy crust, Saturn's moon Enceladus conceals an global ocean of liquid water. A detector on the Cassini space probe detected ice particles propelled from Enceladus that contain high concentrations of organic substances. They exhibit the structures typical of highly complex macromolecular compounds.
Antarctic ice cap melting faster and faster
Research news Melting ice in the Antarctic has resulted in a 7.6 millimeter rise in the global sea level since 1992. Three millimeters of this increase were recorded in the last five years alone, according to a comprehensive study conducted with the participation of scientists from the Technical University of Munich (TUM).
Research news Melting ice in the Antarctic has resulted in a 7.6 millimeter rise in the global sea level since 1992. Three millimeters of this increase were recorded in the last five years alone, according to a comprehensive study conducted with the participation of scientists from the Technical University of Munich (TUM).
Stars Are Born in Loose Groupings
Based on previously published data from the Gaia Mission, researchers at Heidelberg University have derived the conditions under which stars form. The Gaia satellite is measuring the three-dimensional positions and motions of stars in the Milky Way with unprecedented accuracy. Using these data, Dr Jacob Ward and Dr Diederik Kruijssen determined the positions, distances and speeds of a large number of young massive stars within 18 nearby loose stellar groupings.
Based on previously published data from the Gaia Mission, researchers at Heidelberg University have derived the conditions under which stars form. The Gaia satellite is measuring the three-dimensional positions and motions of stars in the Milky Way with unprecedented accuracy. Using these data, Dr Jacob Ward and Dr Diederik Kruijssen determined the positions, distances and speeds of a large number of young massive stars within 18 nearby loose stellar groupings.
Globular Clusters as Relics of Star Formation in the Early Universe
The globular clusters that surround our Milky Way are nearly as old as the universe itself. Computer simulations conducted by a team led by Dr Joel Pfeffer of Liverpool John Moores University (United Kingdom) and Dr Diederik Kruijssen of Heidelberg University suggest that these ancient star clusters were formed via the same mechanisms as our home galaxy's new-born stars, which makes them natural relics of star formation in the early universe.
The globular clusters that surround our Milky Way are nearly as old as the universe itself. Computer simulations conducted by a team led by Dr Joel Pfeffer of Liverpool John Moores University (United Kingdom) and Dr Diederik Kruijssen of Heidelberg University suggest that these ancient star clusters were formed via the same mechanisms as our home galaxy's new-born stars, which makes them natural relics of star formation in the early universe.