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rogue-worlds-may-give-clues-as-to-how-stars-form https://www.astronomy.com/tags/stars/page/4/ Stars | Page 4 of 66 | Astronomy.com https://www.astronomy.com/uploads/2024/08/NGC-1333-by-JWST-1568x882.jpg InStock USD 1.00 1.00 exoplanets stars article ASY 2024-08-28 2024-08-28 151576
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Stars

Exoplanets, Stars

Rogue worlds may give clues as to how stars form

Winter Constellations
Observing, Stars

Five almost-famous stars worth gazing at

The constellation Orion the Hunter hosts two of the 10 brightest stars in the sky, Betelgeuse and Rigel. At magnitude 0.5 and 0.2, respectively, Betelgeuse (orange star at upper left) and Rigel (blue-white star at lower right) stand in stark contrast to many of the surrounding stars.
Observing

Why do astronomers measure stars in magnitudes?

NGC 2623 is a great example of what a pair of interacting galaxies looks like, 260 million light-years distant. Galaxies need mergers or other cosmic events to perturb different regions and trigger star formation and galaxy evolution.
Milky Way

Survivors from the Milky Way’s birth

Hubble image of variable star RS Puppis
Stars

How do Cepheid variables indicate distance?

NGC 4449
Galaxies, Science, Stars

Gemini North celebrates its 25th birthday with a glorious photo of NGC 4449

JWST image of the Serpens Nebula
Stars

In a first, JWST captures ultra-detailed image of aligned jets in the Serpens Nebula

The constellations Corona Borealis, Hercules, and more
Observing, Stars, Upcoming Events

How to see T Coronae Borealis, the ‘brightest nova of the generation’

Exoplanets, Science

The most common planets in the universe might be rich in carbon

Science

The oldest stars in the universe were swallowed by the Milky Way 

When stars “die,” they leave one of two objects behind. Massive stars explode as supernovae, creating remnants of gas and dust like the Crab Nebula (M1). Credit: ASA, ESA, J. Hester and A. Loll (Arizona State University)
Milky Way, Stars

How many stars die in the Milky Way each year?

The very center of globular cluster NGC 6397
Stars

How do globular clusters remain intact for so long?

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