Space and astronomy news
Astronomers have found the largest stellar mass black hole in the Milky Way so far. At 33 solar masses, it dwarfs the previous record-holder, Cygnus X-1, which has only 21 solar masses. Most stellar mass black holes have about 10 solar masses, making the new one—Gaia BH3—a true giant.
Continue reading “The Milky Way’s Most Massive Stellar Black Hole is Only 2,000 Light Years Away”
Astronomers routinely provide the ages of the stars they study. But the methods of measuring ages aren’t 100% accurate. Measuring the ages of distant stars is a difficult task.
The Nancy Grace Roman Space Telescope should make some progress.
Continue reading “Roman Will Learn the Ages of Hundreds of Thousands of Stars”
The region near the Milky Way’s centre is dominated by the supermassive black hole that resides there. Sagittarius A*’s overwhelming gravity creates a chaotic region where tightly packed, high-speed stars crash into one another like cars in a demolition derby.
These collisions and glancing blows change the stars forever. Some become strange, stripped-down, low-mass stars, while others gain new life.
Continue reading “The Stellar Demolition Derby in the Centre of the Galaxy”
The Large Magellanic Cloud (LMC) is the Milky Way’s most massive satellite galaxy. Because it’s so easily observed, astronomers have studied it intently. They’re interested in how star formation in the LMC might have been different than in the Milky Way.
A team of researchers zeroed in on the LMC’s most metal-deficient stars to find out how different.
Continue reading “The Large Magellanic Cloud isn’t Very Metal”
Every time a star forms, it represents an explosion of possibilities. Not for the star itself; its fate is governed by its mass. The possibilities it signifies are in the planets that form around it. Will some be rocky? Will they be in the habitable zone? Will there be life on any of the planets one day?
There’s a point in every solar system’s development when it can no longer form planets. No more planets can form because there’s no more gas and dust available, and the expanding planetary possibilities are truncated. But the total mass of a solar system’s planets never adds up to the total mass of gas and dust available around the young star.
What happens to the mass, and why can’t more planets form?
Continue reading “In a Distant Solar System, the JWST Sees the End of Planet Formation”
In the constellation of Orion, there is a brilliant bluish-white star. It marks the right foot of the starry hunter. It’s known as Rigel, and it is the most famous example of a blue supergiant star. Blue supergiants are more than 10,000 times brighter than the Sun, with masses 16 – 40 times greater. They are unstable and short-lived, so they should be rare in the galaxy. While they are rare, blue supergiants aren’t as rare as we would expect. A new study may have figured out why.
Continue reading “Merging Stars Can Lead to Blue Supergiants”![An artist's conception of a brown dwarf. A new study identifies CK Vulpeculae as the remnant of a collison between a brown dwarf and a white dwarf. Image: By NASA/JPL-Caltech (http://planetquest.jpl.nasa.gov/image/114) [Public domain], via Wikimedia Commons](https://www.universetoday.com/wp-content/uploads/2018/10/Artist’s_conception_of_a_brown_dwarf_like_2MASSJ22282889-431026-2000x1200.jpg)
The only thing worse than drifting through space for an eternity is doing it alone. Observations with the Hubble Space Telescope show that brown dwarfs that once had companions suffer that fate. Binary brown dwarfs that were once bound to each other tend to drift apart as time passes.
Continue reading “Brown Dwarf Pairs Drift Apart in Old Age”
That stars can eat planets is axiomatic. If a small enough planet gets too close to a large enough star, the planet loses. Its fate is sealed.
New research examines how many stars eat planets. Their conclusion? One in twelve stars has consumed at least one planet.
Continue reading “One in Twelve Stars Ate a Planet”
Stars shape their solar systems. It’s true of ours, and it’s true of others. But for some massive stars, their power to shape still-forming systems is fateful and final.
Continue reading “Massive Stars Have the Power to Shape Solar Systems”
Why would a young Sun-like star suddenly belch out a hugely bright flare? That’s what astronomers at Harvard Smithsonian Astrophysical Observatory want to know after they spotted such an outburst using a sensitive submillimeter-wave telescope. According to Joshua Bennett Lovell, leader of a team that observed the star’s activity, these kinds of flare events are rare in such young stars, particularly at millimeter wavelengths. So, what’s happening there?
Continue reading “Even Stars Like the Sun Can Unleash Savage Flares in Their Youth”