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QUANTUM PHYSICS & ELECTRONICS NEWS
YEAR - 2022
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.
Detailed images of the nearby star Beta Pictoris, taken by NASA
Flocculent spiral NGC 2841:Star formation is one of the most important processes in shaping the Universe
ROSAT's X-ray picture of a small cluster of galaxies known as the NGC 2300 group. The cluster lies 150 million light years from Earth in the direction of the northern constellation Cepheus.
This artist’s impression shows the super-Earth 55 Cancri e in front of its parent star. Using observations made with the NASA/ESA Hubble Space Telescope and new analytic software scientists were able to analyse the composition of its atmosphere.
This image shows a small section of the Veil Nebula, as it was observed by the NASA/ESA Hubble Space Telescope. This section of the outer shell of the famous supernova remnant is in a region known as
