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Three-Billion Light-Year Galaxy Chain Could Overturn Cosmology

Over 500 Mysterious Fast Radio Bursts Detected From Distant Space

New Type of Radio Telescope Detects Over 500 Mysterious Fast Radio Bursts From Distant Space

Milky Way Houses 8,292 Recently Discovered Stellar Streams

Tuesday, 19 January, 2021 - 07:00 A view of the Milky Way from an area of Puyehue National Park near Osorno City, Chile, May 8, 2008. Reuters. Cairo - Hazem Badr A research team from the Northwestern University discovered that a stellar stream in the Milky Way galaxy- to which belongs our planet- houses a large cluster of stars that were born at the same time and travel in the same direction. While researchers have long known that stars form in groups, most known clusters are spherical in shape. Only recently have astrophysicists started to find new patterns in the sky. They believe long strings of stars were once tight clusters, gradually ripped apart and stretched by tidal forces.

Astronomers dissect the anatomy of planetary nebulae using Hubble Space Telescope images

 E-Mail IMAGE: On the left is an image of the Jewel Bug Nebula (NGC 7027) captured by the Hubble Space Telescope in 2019 and released in 2020. Further analysis by researchers produced. view more  Credit: STScI, Alyssa Pagan Images of two iconic planetary nebulae taken by the Hubble Space Telescope are revealing new information about how they develop their dramatic features. Researchers from Rochester Institute of Technology and Green Bank Observatory presented new findings about the Butterfly Nebula (NGC 6302) and the Jewel Bug Nebula (NGC 7027) at the 237th meeting of the American Astronomical Society on Friday, Jan. 15. Hubble s Wide Field Camera 3 observed the nebulae in 2019 and early 2020 using its full, panchromatic capabilities, and the astronomers involved in the project have been using emission line images from near-ultraviolet to near-infrared light to learn more about their properties. The studies were first-of-their-kind panchromatic imaging surveys desig

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