Category Astronomy/Space

Researchers discover a Chemically Primitive Dwarf Star in the Galactic Halo

OSIRIS medium-resolution spectrum of J0815+4729 (black line) and the best fit obtained with FERRE (red line). Credit: Aguado et al., 2017.

OSIRIS medium-resolution spectrum of J0815+4729 (black line) and the best fit obtained with FERRE (red line). Credit: Aguado et al., 2017.

Spanish astronomers have identified a new carbon-rich ultra metal-poor unevolved star in the halo of the Milky Way galaxy. The newly found star, designated J0815+4729, could be the most iron-poor unevolved star known to date. Chemically primitive metal-poor stars are important for studying the conditions in the early universe. Thus, astronomers are interested in identifying more stars of this type and deriving their chemical abundances. Large sample of such stars could be helpful in improving our knowledge about stellar formation and evolution.

Recently, a team led by David S...

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Genes in Space-3 successfully Identifies unknown Microbes in space

NASA astronaut Peggy Whitson performed the Genes in Space-3 investigation aboard the space station using the miniPCR and MinION, developed for previously flown investigations. Credits: NASA

NASA astronaut Peggy Whitson performed the Genes in Space-3 investigation aboard the space station using the miniPCR and MinION, developed for previously flown investigations. Credits: NASA

Being able to identify microbes in real time aboard the International Space Station, without having to send them back to Earth for identification first, would be revolutionary for the world of microbiology and space exploration. The Genes in Space-3 team turned that possibility into a reality this year, when it completed the first-ever sample-to-sequence process entirely aboard ISS. Results from their investigation were published in Scientific Reports.

The ability to identify microbes in space could aid in the ability to diagnose and treat astronaut ailments in real time, as well as assisting in the ide...

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Multiwavelength Image of the ‘Toothbrush’ Galaxy Cluster

A multiwavelength false-color image of the "Toothbrush" cluster of galaxies, 1RXS J0603.3+4214. The intensity in red shows the radio emission, blue is X -ray, and the background color composite is optical emission. Astronomers studying the cluster with new radio observations combined with other wavelengths have been able to confirm the galaxy merger scenario and estimate the magnetic field strength in the shocks. Credit: van Weeren et al.

A multiwavelength false-color image of the “Toothbrush” cluster of galaxies, 1RXS J0603.3+4214. The intensity in red shows the radio emission, blue is X -ray, and the background color composite is optical emission. Astronomers studying the cluster with new radio observations combined with other wavelengths have been able to confirm the galaxy merger scenario and estimate the magnetic field strength in the shocks. Credit: van Weeren et al.

Most galaxies lie in clusters containing from a few to thousands of objects. Our Milky Way, for example, belongs to a cluster of about fifty galaxies called the Local Group whose other large member is the Andromeda galaxy about 2.3 million light-years away...

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HATSouth discovers 4 ‘Hot Jupiter’ Exoplanets

Phase-folded unbinned HATSouth light curves for HATS-50 (upper left), HATS-51 (upper right), HATS-52 (lower left) and HATS-53 (lower right). In each case we show two panels. The top panel shows the full light curve, while the bottom panel shows the light curve zoomed-in on the transit. The solid lines show the model fits to the light curves. The dark filled circles in the bottom panels show the light curves binned in phase with a bin size of 0.002. Credit: Henning et al. 2017.

Phase-folded unbinned HATSouth light curves for HATS-50 (upper left), HATS-51 (upper right), HATS-52 (lower left) and HATS-53 (lower right). In each case we show two panels. The top panel shows the full light curve, while the bottom panel shows the light curve zoomed-in on the transit. The solid lines show the model fits to the light curves. The dark filled circles in the bottom panels show the light curves binned in phase with a bin size of 0.002. Credit: Henning et al. 2017.

An international team of astronomers reports the discovery of four new ‘hot Jupiter’ extrasolar worlds by the HATSouth survey. The newly found exoplanets received designations HATS-50b through HATS-53b...

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