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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 - 2020-12-01
Just weeks after NASA astronauts repaired the Hubble Space Telescope in December 1999, the Hubble Heritage Project snapped this picture of NGC 1999, a nebula in the constellation Orion

Just weeks after NASA astronauts repaired the Hubble Space Telescope in December 1999, the Hubble Heritage Project snapped this picture of NGC 1999, a nebula in the constellation Orion

Far away in the Ursa Major constellation is a swirling galaxy that would not look out of place on a coffee made by a starry-eyed barista. NGC 3895 is a barred spiral galaxy that was first spotted by William Herschel in 1790 and was later observed by the NASA/ESA Hubble Space Telescope.

Far away in the Ursa Major constellation is a swirling galaxy that would not look out of place on a coffee made by a starry-eyed barista. NGC 3895 is a barred spiral galaxy that was first spotted by William Herschel in 1790 and was later observed by the NASA/ESA Hubble Space Telescope

This image shows NGC 121, a globular cluster in the constellation of Tucana (The Toucan)

This image shows NGC 121, a



The behemoth galaxy NGC 1275, also known as Perseus A, lies at the centre of Perseus Galaxy Cluster. By combining multi-wavelength images into this single composite, the dynamics of the galaxy become visible.

The behemoth galaxy NGC 1275, also known as Perseus A, lies at the centre of Perseus Galaxy Cluster. By combining multi-wavelength images into this single composite, the dynamics of the galaxy become visible. Detail and structure from optical, radio and X-ray wavelengths have been combined for an aesthetically pleasing image which shows the violent events in the galaxy's heart. NGC 1275 is an active galaxy well-known for its radio source (Perseus A) and is a strong emitter of X-rays due to the presence of the supermassive black hole in its centre.