“Doesn’t Make Any Sense” – Star Pair That Shouldn’t Exist Shocks Astronomers
Astronomers at the European Southern Observatory have revealed that the peculiar characteristics of the HD 148937 star system, including a magnetic star and its young…
Stellar evolution is the process by which a star undergoes a sequence of radical changes during its lifetime. Depending on the mass of the star, its life cycle can span from a few million years for the most massive stars to trillions of years for the least massive ones. The journey begins with the gravitational collapse of a cloud of gas and dust, leading to the formation of a protostar when the core temperature gets high enough to start nuclear fusion. In this phase, hydrogen nuclei fuse to form helium, releasing energy that makes the star shine.
Astronomers at the European Southern Observatory have revealed that the peculiar characteristics of the HD 148937 star system, including a magnetic star and its young…
Astronomers have verified that variations in the chemical makeup of binary stars originate from the initial phases of their formation. Recent research using the Gemini…
Advanced observations by the JWST indicate that early galaxies matured faster and were less chaotic, challenging previous theories of galaxy evolution. New research has revealed…
Utilizing sophisticated simulation technology, researchers from UNIGE, Northwestern University, and the University of Florida have shed light on the enigmatic nature of these celestial “beasts.”…
Stars serve as the fundamental building blocks of galaxies and, by extension, the entire observable universe. Among the diverse spectrum of stars, those with a…
Astronomers have taken a significant step forward in uncovering the mysteries of the cosmic dawn. A collection of 350 radio telescopes located in the Karoo…
New research sheds light on the chemical formation of the universe. An international team of researchers stumbled upon an exploding supernova in a distant spiral…
Planetary nebulae are formed when red giant stars reach the end of their helium fuel supply and eject their outer layers, becoming hot and dense…
The fate of galaxies is determined by the initial mass distribution at the birth of a new population of stars in the diverse and vast…
The latest data from HERA improves the search for cosmic dawn radiation and tests theories of galaxy formation. An array of 350 radio telescopes located…
Recent findings indicate that a significant number of stars exhibit irregularities in their cores. Scientists have discovered a method to examine the internal workings of…
The impending demise of Kepler-1658b as it orbits its aging star offers an opportunity for scientists to gain insight into the fate of other planets…
First-of-its-kind experimental evidence contradicts traditional theories about the emission and absorption of radiation by plasmas. While solids, liquids, and gases are familiar states of matter,…
Compact, massive triple star system detected by University of Copenhagen researchers. Earlier this year, researchers revealed the discovery of an extraordinarily compact “one-of-a-kind” system of…
At the end of its life, a red supergiant star explodes in a hydrogen-rich supernova. By comparing observation results to simulation models, an international research…
New work from Carnegie’s Jonathan Gagné and the American Museum of Natural History’s Jacqueline Faherty identified nearly a thousand potential members and 31 confirmed members…
For the first time, astronomers have detected a signal from stars emerging in the early universe. Using a radio antenna not much larger than a…
An international team of astronomers led by the Max Planck Institute for Astronomy (MPIA) has made a surprising discovery about the birthplace of groups of…