Space and astronomy news
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”
At the Kitt Peak National Observatory in Arizona, an instrument with 5,000 tiny robotic eyes scans the night sky. Every 20 minutes, the instrument and the telescope it’s attached to observe a new set of 5,000 galaxies. The instrument is called DESI—Dark Energy Survey Instrument—and once it’s completed its five-year mission, it’ll create the largest 3D map of the Universe ever created.
But scientists are getting access to DESI’s first data release and it suggests that dark energy may be evolving.
Continue reading “A New Map Shows the Universe’s Dark Energy May Be Evolving”
What is Dark Matter? We don’t know. At this stage of the game, scientists are busy trying to detect it and map out its presence and distribution throughout the Universe. Usually, that involves highly-engineered, sophisticated telescopes.
But a new approach involves a device so small it can sit on a kitchen table.
Continue reading “A New Tabletop Experiment to Search for Dark Matter”
If there’s a Holy Grail on Mars, it’s probably a specific type of rock: A rock so important that it holds convincing clues to Mars’ ancient habitability.
Perseverance might have just found it.
Continue reading “Perseverance Finds its Dream Rock”
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”
Scientists have been underutilizing a key resource we can use to help us understand Earth: animals. Our fellow Earthlings have a much different, and usually much more direct, relationship with the Earth. They move around the planet in ways and to places we don’t.
What can their movements tell us?
Continue reading “How Animal Movements Help Us Study the Planet”
The edge of the Solar System is defined by the heliosphere and its heliopause. The heliopause marks the region where the interstellar medium stops the outgoing solar wind. But only two spacecraft, Voyager 1 and Voyager 2, have ever travelled to the heliopause. As a result, scientists are uncertain about the heliopause’s extent and its other properties.
Some scientists are keen to learn more about this region and are developing a mission concept to explore it.
Continue reading “Want to Leave the Solar System? Here’s a Route to Take”
Like a pilgrim seeking wisdom, NASA’s MSL Curiosity has been working its way up Mt. Sharp, the dominant central feature in Gale Crater. Now, almost 12 years into its mission, the capable rover has reached an interesting feature that could tell them more about Mars and its watery history. It’s called the Gediz Vallis channel.
Continue reading “Curiosity has Reached an Ancient Debris Channel That Could Have Been Formed by Water”
There’s a population of planets that drifts through space untethered to any stars. They’re called rogue planets or free-floating planets (FFPs.) Some FFPs form as loners, never having enjoyed the company of a star. But most are ejected from solar systems somehow, and there are different ways that can happen.
One researcher set out to try to understand the FFP population and how they came to be.
rogue
Some stars are so massive and so energetic that they’re a million times brighter than the Sun. This type of star dominated the early Universe, playing a key role in its development and evolution. The first of its kind are all gone now, but the modern Universe still forms stars of this type.
These hot, blue stars emit powerful ultraviolet energy that the Hubble can detect from its perch in Low-Earth Orbit.
Continue reading “The Hubble Aims Its Powerful Ultraviolet Eye at Super-Hot Stars”