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A shock flash breaking out of a dusty red supergiant

Shock-breakout emission is light that arises when a shockwave, generated by the core-collapse explosion of a massive star, passes through its outer envelope. Hitherto, the earliest detection of such a signal was at several hours after the explosion1, although a few others had been reported2–7. The temporal evolution of early light curves should provide insights into the shock propagation, including explosion asymmetry and environment in the vicinity, but this has been hampered by the lack of multiwavelength observations. Here we report the instant multiband observations of a type II supernova (SN 2023ixf) in the galaxy M101 (at a distance of 6.85 ± 0.15 Mpc; ref. 8), beginning at about 1.4 h after the explosion. The exploding star was a red supergiant with a radius of about 440 solar radii. The light curves evolved rapidly, on timescales of 1−2 h, and appeared unusually fainter and redder than predicted by the models9–11 within ....

United States , American Astronomical Society Meeting Abstracts , Pipeline For The Antarctic Survey Telescope , Sloan Digital Sky , Antarctic Survey Telescope , Photometric All Sky Survey , Hubble Space Telescope , Discovery Report , Name Server Discovery Report , Name Server Astronote , East Asian , Eruption Time , Discovery Images , Astropy Project , Automated Photometry , Latest Data , Survey Telescope , Space Sci , All Sky Survey , Gaia Data Release , Multi Band Photometric Follow Up , Discovery Forced Photometry , Sloan Digital Sky Survey , Gamma Ray Bursters , Milky Way ,

A super-massive Neptune-sized planet

Neptune-sized planets exhibit a wide range of compositions and densities, depending on factors related to their formation and evolution history, such as the distance from their host stars and atmospheric escape processes. They can vary from relatively low-density planets with thick hydrogen–helium atmospheres1,2 to higher-density planets with a substantial amount of water or a rocky interior with a thinner atmosphere, such as HD 95338 b (ref. 3), TOI-849 b (ref. 4) and TOI-2196 b (ref. 5). The discovery of exoplanets in the hot-Neptune desert6, a region close to the host stars with a deficit of Neptune-sized planets, provides insights into the formation and evolution of planetary systems, including the existence of this region itself. Here we show observations of the transiting planet TOI-1853 b, which has a radius of 3.46 ± 0.08 Earth radii and orbits a dwarf star every 1.24 days. This planet has a mass of 73 ....

United States , Collier Cameron , Telescopio Carlos , Monte Carlo , Exoplanet Community Early Release Science Program , Ames Research Center , Photometric All Sky Survey , Mission Conference , International Astronomical Union , Sloan Digital Sky , Plato Mission Conference , Kepler Science Operations Center , Meeting Of The American Astronomical Society , Program Working Group Tfop Wg Sub , Smithsonian Institution , Astrophysics Source Code Library , Gaia Early Data Release , Protoplanetary Cloud , Interest Catalog , Kepler Data Processing Handbook , Research Center , Observing Program Working Group , Sub Group , American Astronomical Society , Cumbres Observatory , Space Sci ,

Astronomers Stunned by Uncommon Polar Ring Galaxy, Labeling it as One of the Most Magnificent Sightings

Astronomers Stunned by Uncommon Polar Ring Galaxy, Labeling it as One of the Most Magnificent Sightings
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Western Australia , Penny Sackett , Linda Sparke , Magda Arnaboldi , Hi Parkes All Sky Survey , Monthly Notices Of The Royal Astronomical Society , Volume Hi Survey , Milky Way , Square Kilometre Array Pathfinder , Monthly Notices , Royal Astronomical , Australia Telescope Compact Array , New South , All Sky Survey , Local Volume ,