Universe Today

January 31, 2024February 1, 2024 by Evan Gough

Betelgeuse. Before, During and After the Great Dimming

Image showing Betelgeuse (top left) and the dense nebulae of the Orion molecular cloud complex (Rogelio Bernal Andreo) — Orion and the molecular cloud covering the region. Betelgeuse is the red star in the upper left. (Credit : Rogelio Bernal Andreo)

When a prominent star in the night sky suddenly dims, it generates a lot of interest. That’s what happened with the red supergiant star Betelgeuse between November 2019 and May 2020. Betelgeuse will eventually explode as a supernova. Was the dimming a signal that the explosion was imminent?

No, and new research helps explain why.

January 31, 2024January 31, 2024 by Brian Koberlein

Even Early Galaxies Grew Hand-in-Hand With Their Supermassive Black Holes

An artist’s impression of a quasar. Credit: NASA / ESA / J. Olmsted, STScI

Within almost every galaxy there is a supermassive black hole. This by itself implies some kind of formative connection between the two. We have also observed how gas and dust within a galaxy can drive the growth of galactic black holes, and how the dynamics of black holes can both drive star formation or hinder it depending on how active a black hole is. But one area where astronomers still have little information is how galaxies and their black holes interacted in the early Universe. Did black holes drive the formation of galaxies, or did early galaxies fuel the growth of black holes? A recent study suggests the two evolved hand in hand.

January 30, 2024January 30, 2024 by Laurence Tognetti

Astrobiology: Why study it? How to study it? What are the challenges?

Universe Today has proudly examined the importance of studying impact craters, planetary surfaces, and exoplanets, and what they can teach scientists and the public about finding life beyond Earth. Impact craters both shape these planetary surfaces and hold the power to create or destroy life, and we learned how exoplanets are changing our views of planetary formation and evolution, including how and where we might find life in the cosmos. Here, we will discuss how these disciplines contribute to the field responsible for finding life beyond Earth, known as astrobiology. We will discuss why scientists study astrobiology, also known as astrobiologists, challenges of studying astrobiology, and how students can pursue studying astrobiology, as well. So, why is it so important to study astrobiology?

January 30, 2024January 30, 2024 by Evan Gough

Webb Directly Images Two Planets Orbiting White Dwarfs

Artist's rendition of a white dwarf from the surface of an orbiting exoplanet. Astronomers have found two giant planet candidates orbiting two white dwarfs. More proof that giant planets can surve their stars' red giant phases. Image Credit: Madden/Cornell University

In several billion years, our Sun will become a white dwarf. What will happen to Jupiter and Saturn when the Sun transitions to become a stellar remnant? Life could go on, though the giant planets will likely drift further away from the Sun.

January 30, 2024January 30, 2024 by Carolyn Collins Petersen

The Aftermath of a Recent Galactic Merger

The Gemini South telescope view of NGC 4753, a peculiar galaxy thought to have experienced a galactic merger. Courtesy International Gemini Observatory/NOIRLab/NSF/AURA

NGC 4753 is a prime example of what happens after a galactic merger. It looks like a twisted mess, with dust lanes looping around the massive galactic nucleus. Astronomers long wondered what happened to this galaxy, and with a sharp new image created by the Gemini South telescope, they can finally explain its tortured past.

January 30, 2024January 30, 2024 by Evan Gough

Feast Your Eyes on 19 Face-On Spiral Galaxies Seen by Webb

These Webb images are part of a large, long-standing project, the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) program, which is supported by more than 150 astronomers worldwide. Before Webb took these images, PHANGS was already brimming with data from NASA’s Hubble Space Telescope, the Very Large Telescope’s Multi-Unit Spectroscopic Explorer, and the Atacama Large Millimeter/submillimeter Array, including observations in ultraviolet, visible, and radio light. Webb’s near- and mid-infrared contributions have provided several new puzzle pieces. Image Credit: NASA/ESA/CSA

If you’re fascinated by Nature, these images of spiral galaxies won’t help you escape your fascination.

These images show incredible detail in 19 spirals, imaged face-on by the JWST. The galactic arms with their multitudes of stars are lit up in infrared light, as are the dense galactic cores, where supermassive black holes reside.

January 30, 2024January 30, 2024 by Matt Williams

A Magnetohydrodynamic Drive Could Lead to Fuel Stations on Mars

Graphic depiction of Magnetohydrodynamic Drive for Hydrogen and Oxygen Production in Mars Transfer. Credit: Alvaro Romero-Calvo

Within the next fifteen years, NASA, China, and SpaceX plan to send the first crewed missions to Mars. In all three cases, these missions are meant to culminate in the creation of surface habitats that will allow for many returns and – quite possibly – permanent human settlements. This presents numerous challenges, one of the greatest of which is the need for plenty of breathable air and propellant. Both can be manufactured through electrolysis, where electromagnetic fields are applied to water (H₂O) to create oxygen gas (O₂) and liquid hydrogen (LH₂).

While Mars has ample deposits of water ice on its surface that make this feasible, existing technological solutions fall short of the reliability and efficiency levels required for space exploration. Fortunately, a team of researchers from Georgia Tech has proposed a “Magnetohydrodynamic Drive for Hydrogen and Oxygen Production in Mars Transfer” that combines multiple functionalities into a system with no moving parts. This system could revolutionize spacecraft propulsion and was selected by NASA’s Innovative Advanced Concepts (NIAC) program for Phase I development.

January 30, 2024January 23, 2024 by Paul M. Sutter

The Seeming Impossibility of Life

This is an artist's illustration showing the timeline of the early universe showing some key time periods. On the left is the early day of the Universe, where the intense heat prevented much from happening. After that is the release of the CMB once the Universe cooled a little. After that, in yellow, is the Neutral Universe, the time before stars formed. The hydrogen atoms in the Neutral Universe should have given off radio waves that we can detect here on Earth. Image Credit: ESA – C. Carreau — This is an artist's illustration showing the timeline of the early universe showing some key time periods. On the left is the early day of the Universe, where the intense heat prevented much from happening. After that is the release of the CMB once the Universe cooled a little. After that, in yellow, is the neutral Universe, the time before stars formed. The hydrogen atoms in the neutral Universe should have given off radio waves that we can detect here on Earth. Image Credit: ESA – C. Carreau

The number of near misses, false starts, and legitimate disasters that have befallen our species since the day we took our first upright steps all those generations ago is too large to count and could honestly take up this entire book. I’ll give us humans this much, though: we’re survivors, through and through.

January 29, 2024January 29, 2024 by Laurence Tognetti

Water Vapor Found in the Atmosphere of a Small Exoplanet

Artist's impression of GJ 9827 d, which is the smallest exoplanet ever found to potentially possess water in its atmosphere. (Credit: NASA, ESA, Leah Hustak and Ralf Crawford (STScI))

A recent study published in The Astrophysucal Journal Letters discusses the detection of water within the atmosphere of GJ 9827 d, which is a Neptune-like exoplanet located approximately 97 light-years from Earth, using NASA’s Hubble Space Telescope (HST), and is the smallest exoplanet to date where water has been detected in its atmosphere. This study was conducted by an international team of researchers and holds the potential to identify exoplanets throughout the Milky Way Galaxy which possess water within their atmospheres, along with highlighting the most accurate methods to identify the water, as well.

January 29, 2024January 29, 2024 by Carolyn Collins Petersen

The Space-Based Gravitational Wave Observatory LISA Gets the Green Light

An artist's concept of how LISA will work to detect gravitational waves from orbit in space. Courtesy ESA.

The science of studying gravitational waves just got a big boost thanks to the European Space Agency. Its science program committee just approved the Laser Interferometer Space Antenna—affectionately known as LISA—for official planning and building. That means gravitational wave astronomers will take their next steps to capture information about gravity waves from space.