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ScienceCasts Earth's Magnetosphere Elucidating The Black Holes The Surprising Power of a Solar Storm Weird Planets A Close Encounter With Jupiter Ancient remnants deep in the Kuiper belt The Super Fluid Core Of A Dead Neutron Star Massive Cloud On Collision Course With Milky Way Mysterious Objects at the Edge of the Electromagnetic Spectrum Big Mystery in the Perseus Cluster Spacecraft discovers thousands of doomed comets Close Encounter with Enceladus Amazing Moons The Sounds Of The InterStellar Space



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MXPlank News Letter - 2020-04-13
Blue straggler stars are blue, bright stars, with a higher mass than the average for a cluster, and they are expected to sink towards the centre of a star cluster over time.

Blue straggler stars are blue, bright stars, with a higher mass than the average for a cluster, and they are expected to sink towards the centre of a star cluster over time.

WR 25 and Tr16-244, at the bottom of the image, are located within the open cluster Trumpler 16. This cluster is embedded within the Carina Nebula, an immense cauldron of gas and dust that lies approximately 7500 light-years from Earth in the constellation of Carina, the Keel. At the top of the image, a peculiar nebula with the shape of a 'defiant' finger points towards WR25 and Tr16-244

WR 25 and Tr16-244, at the bottom of the image, are located within the open cluster Trumpler 16. This cluster is embedded within the Carina Nebula, an immense cauldron of gas and dust that lies approximately 7500 light-years from Earth in the constellation of Carina, the Keel

The exoplanet WASP-107b is a gas giant, orbiting a highly active K-type main sequence star.

The exoplanet WASP-107b is a gas giant, orbiting a highly active K-type main sequence star. The star is about 200 light-years from Earth. Using spectroscopy, scientists were able to find helium in the escaping atmosphere of the planet - the first detection of this element in the atmosphere of an exoplanet

This is a unique NASA/ESA Hubble Space Telescope view of the disk galaxy NGC 5866 tilted nearly edge-on to our line-of-sight

This is a unique NASA/ESA Hubble Space Telescope view of the disk galaxy NGC 5866 tilted nearly edge-on to our line-of-sight.Hubble's sharp vision reveals a crisp dust lane dividing the galaxy into two halves. The image highlights the galaxy's structure: a subtle, reddish bulge surrounding a bright nucleus, a blue disk of stars running parallel to the dust lane, and a transparent outer halo.