Getting back to the Moon is the primary goal of NASA’s Artemis program, but what do we do once we get there? That is the challenge tackled by a group of students at the University of Illinois Urbana-Champaign, who wrote a proposal for a lunar infrastructure module they call the Trans-lunar Hub for Exploration, ISRU, and Advancement – or THEIA, after the proposed object that crashed into the Earth that created the Moon as we know it today. Their submission was part of the NASA Revolutionary Aerospace Systems Concepts – Academic Linkage project, where teams from various academic institutions submitted papers focusing on the theme of Sustained Lunar Evolution for 2024.
Continue reading “A Long-Term Lunar Infrastructure Hub Named After the Object That Created the Moon”New Study of Supernovae Data Suggests That Dark Energy is an Illusion
Dark energy is central to our modern understanding of cosmology. In the standard model, dark energy is what drives the expansion of the Universe. In general relativity, it’s described by a cosmological constant, making dark energy part of the structure of space and time. But as we’ve gathered more observational evidence, there are a few problems with our model. For one, the rate of cosmic expansion we observe depends on the observational method we use, known as the Hubble tension problem. For another, while we assume dark energy is uniform throughout the cosmos, there are some hints suggesting that might not be true. Now a new study argues we’ve got the whole thing wrong. Dark energy, the authors argue, doesn’t exist.
Continue reading “New Study of Supernovae Data Suggests That Dark Energy is an Illusion”New Glenn Completes a Hotfire Test. Next… Flight?
Blue Origin has achieved an important milestone with its New Glenn NG-1 rocket, successfully completing a 24-second hotfire of the rocket’s BE-4 engines in preparation for an expected test flight in the coming days.
Continue reading “New Glenn Completes a Hotfire Test. Next… Flight?”A Young Exoplanet's Atmosphere Doesn't Match its Birthplace
If the modern age of astronomy could be summarized in a few words, it would probably be “the age of shifting paradigms.” Thanks to next-generation telescopes, instruments, and machine learning, astronomers are conducting deeper investigations into cosmological mysteries, making discoveries, and shattering preconceived notions. This includes how systems of planets form around new stars, which scientists have traditionally explained using the Nebular Hypothesis. This theory states that star systems form from clouds of gas and dust (nebulae) that experience gravitational collapse, creating a new star.
The remaining gas and dust then settle into a protoplanetary disk around the new star, which gradually coalesces to create planets. Naturally, astronomers theorize that the composition of the planets would match that of the disk itself. However, when examining a still-developing exoplanet in a distant star system, a team of astronomers uncovered a mismatch between the gases in the planet’s atmosphere and those within the disk. These findings indicate that the relationship between a protoplanetary disk and the planets they form might be more complicated.
Continue reading “A Young Exoplanet's Atmosphere Doesn't Match its Birthplace”The Quadrantid Meteors and More Ring in 2025
This Weekend: Catch the Quadrantids at their annual peak, Earth at perihelion and the Moon blotting out Saturn.
Ready for another amazing year of skywatching? The very first weekend of 2025 offers up a flurry of wintertime astronomy events, eluding a swift meteor shower, a January ‘SuperSun,’ and a lunar planetary pair up at dusk.
Continue reading “The Quadrantid Meteors and More Ring in 2025”A New Mission Watches Meteoroids Hit the Far Side of the Moon
Sometimes, it’s hard to remember that Earth is constantly being bombarded by literally tons of space debris daily. The larger bits form what we know as shooting stars, and most burn up in the atmosphere. Still, throughout our planet’s history, giant versions have caused devastation unlike anything else seen on this planet. Tracking these types of objects is typically done from the Earth, but a new mission set out by researchers in Italy has a novel idea – why not try to learn more about potential impactors by watching them hit the far side of the Moon?
Continue reading “A New Mission Watches Meteoroids Hit the Far Side of the Moon”Even Stars Can Get the Hiccups
Stars come in all manner of sizes and temperatures. Many of the massive ones are nearing the end of their lives and at some point in the next few million years, will detonate as supernova explosions. Observing the early stages of these events is tricky though as we can never be sure when they will go pop! It would be great if we could narrow down the timeframe to help hone our search. One theorised phase is that massive stars can ‘hiccup’ with its core expanding and contracting rapidly. This is known as ‘pulsational pair-instability’ and finally a team of astronomers have actually caught a star having the hiccups!
Hotter White Dwarfs Get Puffier
When our Sun dies, it will turn into a white dwarf. They are a common aspect of stellar evolution and a team of researchers have now turned their attention onto them. They have just completed a survey of 26,000 white dwarfs and confirmed a long-predicted theory that the hotter the star, the puffier it is! This new study will help us to understand white dwarfs and the processes that drive them.
NASA to Probe the Secrets of the Lunar Regolith
Gaze up at the Moon on any night and you will see a barren world displaying all manner of shades of grey. Aside from the obvious craters and lunar maria, the surface of the Moon is covered in the fine, dusty lunar regolith. The Apollo astronauts in the 60’s and 70’s learned that it was electromagnetically charged and was very abrasive posing a problem for mechanical equipment. Now a new payload on the Commercial Lunar Payload Services initiative will explore the regolith even further.
NOIRLab Launches Collection of Hi-Res Images of 88 IAU-recognized Constellations
Located in Tuscon, Arizona, the National Optical-Infrared Astronomy Research Laboratory (NOIRLab) is a national facility consisting of four observatories that provide astronomers affiliated with any US institution with access to observing time. As part of its mission to advance astronomy and science education, NOIRLab recently announced the release of the 88 Constellations Project, a collection of free, high-resolution, downloadable images of all IAU-recognized constellations. This project is an educational archive that is free for all and includes the largest open-source all-sky photo of the night sky.
Continue reading “NOIRLab Launches Collection of Hi-Res Images of 88 IAU-recognized Constellations”