Space.com on MSN
The Milky Way may be hiding a big secret at its heart: an extremely magnetic dead star
Astronomers suspect the heart of the Milky Way may be hiding a big secret: a rapidly spinning, highly magnetic, neutron ...
Space.com on MSN
Why don't more Tatooine-like exoplanets exist in our Milky Way galaxy? Astronomers might have an answer
Astronomers may finally understand why planets orbiting two suns, the real-world equivalents of the "Star Wars" planet ...
The universe contains billions of galaxies, each filled with stars, dust and mystery. Here are 12 incredible galaxies, ...
Morning Overview on MSN
Does the Milky Way really wobble through space like a giant spinning top?
The Milky Way is not the serene, flat disc that textbook illustrations suggest. Astronomers have confirmed that the outer ...
During the survey, researchers identified a promising 8.19-millisecond pulsar (MSP) candidate located close to Sagittarius A*, the supermassive black hole at the center of our galaxy.
Scientists scanning the heart of the Milky Way have spotted a tantalizing signal: a possible ultra-fast pulsar spinning every 8.19 milliseconds near Sagittarius A*, the supermassive black hole at our ...
The Milky Way owes its iconic name not to modern astrophysics but to an Ancient Greek myth involving Zeus, Hera, and a splash of divine milk.
When you gaze up at the night sky, you’re looking back in time. Light from the stars takes years, sometimes millennia, to ...
Space on MSN
How our galaxy's black hole was captured
Caltech’s Katie Bouman explains how the Event Horizon Telescope Collaboration captured the first imager of the Sagittarius A* Supermassive black hole at the core of the Milky Way galaxy - Milky Way vs ...
In late winter, the zodiacal light is visible in the evening in the Northern Hemisphere (false dusk) and in the pre-dawn ...
Saul Hernandez, a New Mexico State University senior studying physics and linguistics with a minor in astronomy, has turned ...
Intense radiation emitted by active supermassive black holes—thought to reside at the center of most, if not all, galaxies—can slow star growth not just in their host galaxy, but also in galaxies ...
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