Pictures are the key to new insights in the field of astrophysics. Such images include simulations of cosmic events, which astrophysicists at UZH use to investigate how stars, planets and galaxies ...
NASA’s James Webb Space Telescope has captured the first detailed look at a carbon-rich disk surrounding the exoplanet CT Cha ...
A new study led by UNLV scientists sheds light on how planets, including Earth, formed in our galaxy—and why the life and ...
When it comes to science, a simple observation can upend everything you think you know, such is the case with one star ...
When a star is born, it doesn’t emerge in isolation. Instead, it forms inside a large, chaotic cloud of gas and dust. Around it, a flat disk of spinning material takes shape. This protoplanetary disk ...
Rogue planets do not orbit around a star, but instead wander through the galaxy aimlessly. NASA estimates there are billions ...
Warm Jupiters are rewriting the rules of planet formation - showing eccentric orbits that stay strangely aligned with their ...
A recent astronomical discovery has shaken long-held beliefs about how planets form. For decades, scientists thought that stars much smaller than our Sun couldn't form giant planets. That theory just ...
Besides being a point of light, a star is a luminous, spherical mass of plasma, enough to hold itself together under its own gravity. On its own, though, gravitational rounding isn't enough. What ...
JWST found a carbon-atmosphere planet orbiting a pulsar, challenging current models of how planets form. Scientific progress often comes from data that don’t fit our current understanding. This idea, ...
Molecular clouds are composed of gas and dust and serve a vital purpose in star formation. Eos, a crescent-shaped gas cloud, is located about 300 light years away from Earth and is the size of 40 ...
14hon MSN
Young sun-like star's dual-temperature plasma ejections offer clues to early planetary environments
Astronomers have used simultaneous ground-based and space-based observations to measure the temperature and velocity of gas ...
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