Connecting To The Server To Fetch The WebPage Elements!!....
MXPlank.com MXMail Submit Research Thesis Electronics - MicroControllers Contact us QuantumDDX.com

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



Search The Site







MXPlank News Letter - 2020-08-06
This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it’s beautiful arms which swirl like a whirlpool around its bright central region

This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it’s beautiful arms which swirl like a whirlpool around its bright central region

This Hubble image shows RS Puppis, a type of variable star known as a Cepheid variable. As variable stars go, Cepheids have comparatively long periods — RS Puppis, for example, varies in brightness by almost a factor of five every 40 or so days.</p> <p>RS Puppis is unusual; this variable star is shrouded by thick, dark clouds of dust enabling a phenomenon known as a light echo to be shown with stunning clarity

This Hubble image shows RS Puppis, a type of variable star known as a Cepheid variable. As variable stars go, Cepheids have comparatively long periods — RS Puppis, for example, varies in brightness by almost a factor of five every 40 or so days

30 Doradus is the brightest star-forming region in our galactic neighbourhood and home to the most massive stars ever seen.

30 Doradus is the brightest star-forming region in our galactic neighbourhood and home to the most massive stars ever seen. The nebula resides 170 000 light-years away in the Large Magellanic Cloud, a small, satellite galaxy of our Milky Way.

This new NASA/ESA Hubble Space Telescope image shows ghostly green filaments, lying within galaxy 2MASX J15100402+0740370.

This new NASA/ESA Hubble Space Telescope image shows ghostly green filaments, lying within galaxy 2MASX J15100402+0740370. This filament was illuminated by a blast of radiation from a quasar - a very luminous and compact region that surrounds the supermassive black hole at the centre of its host galaxy.