Space News & Blog Articles

We’ve been getting plenty of spectacular images from the James Webb Space Telescope since it began operations last year. Fraser even covered everything we learned from it in a video a few weeks ago. But the news keeps coming, and recently a science team known as the Prime Extra-Galactic Areas for Reionization and Lensing Science (PEARLS) team released a series of four papers describing Webb’s observations of a galaxy cluster known as El Gordo (“the fat one” in Spanish). But what’s more – they also released another absolutely stunning picture.

On July 28th, the European Space Agency commanded its long-working Aeolus wind profile mission to re-enter Earth’s atmosphere. It did that and disintegrated into pieces over Antarctica. Of course, satellites do this often. But, Aeolus was different. It maneuvered its way into a safe re-entry profile, a first-of-its kind activity designed to avoid populated regions on Earth.

A coronal mass ejection erupted from the Sun on October 28th, 2021, spreading solar energetic particles (SEPs) across a volume of space measuring more than 250 million km (155.34 million mi) wide. This means that the event was felt on Earth, Mars, and the Moon, which was on the opposite side of the Sun at the time. It was also the first time that a solar event was measured simultaneously by robotic probes on Earth, Mars, and the Moon, which included ESA’s ExoMars Trace Gas Orbiter (TGO) and Eu:CROPIS orbiter, NASA’s Curiosity rover and Lunar Reconnaissance Orbiter (LRO), and China’s Chang’e-4 lander.

Brace yourselves for great JWST views of the iconic Ring Nebula (M57). An international team of astronomers just released a fantastic near-infrared image of the nebula, showing incredible details.

In the astronomy community, we typically this of light pollution as an overall negative. Much research points out its negative effect on our sleep and even our observational equipment. It also significantly impacts wildlife; however, according to a new paper from some Belgian, Swiss, and German researchers, not all of that impact is negative. 

You’ve just found the perfect work desk at a garage sale, and you measure it to see if it will fit in your apartment. You brought a tape measure to size it up and find it’s 180 cm. Perfect. But your friend also brought a tape measure, and they find it’s 182 cm, which would be a smidge too long. You don’t know which tape measure is right, so you have a conundrum. Astronomers also have a conundrum, and it’s known as the Hubble tension.

Researchers from the Chinese Academy of Sciences and the Chinese National Space Administration recently published a study in the journal Space: Science & Technology outlining how the upcoming Chang’e-7 mission, due to launch in 2026, will use a combination of orbital observations and in-situ analyses to help identify the location, amount, and dispersion of water-ice in the permanently-shadowed regions (PSRs) of the Moon, specifically at the lunar south pole.

At the heart of our galaxy, there is a monster black hole. Known as Sagittarius A*, it has a mass of 4.2 million Suns, and it’s only about 27,000 light-years from Earth. Sag A* is the closest supermassive black hole, and one of only two that we’ve observed directly. It is so close that we can even see stars closely orbiting it. Some of those stars we’ve been observing for more than 20 years, which means we have a very good handle on their orbits. We’ve used those orbits to determine the mass of Sag A*, but a new study looks at a different question: does our galaxy’s black hole have a companion?

The European Space Agency’s Gaia Observatory has been operating steadily at the Earth-Sun L2 Lagrange Point for almost a decade. As an astrometry mission, Gaia aims to gather data on the positions, proper motion, and velocity of stars, exoplanets, and objects in the Milky Way and tens of thousands of neighboring galaxies. By the end of its primary mission (scheduled to end in 2025), Gaia will have observed an estimated 1 billion astronomical objects, leading to the creation of the most precise 3D space catalog ever made.

For astronomers, the only thing better than new data is more new data. And we seem to be in a golden age of data gathering. We’ve gushed over the latest images from the James Webb Space Telescope and Hubble continues to make observations, but several new space telescopes are lesser known, such as Gaia, TESS, and Swift. And now a new space telescope enters the game, known as Euclid. Euclid is an infrared telescope launched last month by the European Space Agency (ESA). It took 11 years to design and build the telescope, and it has just taken test images with its two primary detectors.

So much in science is based on constraints. If scientists don’t understand something, they try to constrain it as much as possible so that more precise experiments can finally detect whatever the theorized phenomenon is. Dark matter is notoriously difficult in this regard, as it has evaded detection for over a century at this point, despite even more precise instruments trying to capture a glimpse of it. One of those instruments is the Super Cryogenic Dark Matter Search (SuperCDMS), run by the SLAC National Laboratory and located in northern Minnesota. To help further the cause, researchers looked at the data from the experiment while considering a few new possibilities, and while they didn’t find any evidence of dark matter, they helped tighten the constraints even more.

The Mars Sample Return (MSR) has been going through a rough patch lately. We recently reported on reports coming out about Congress restricting its budget and potential cost overruns. However, like any good government program, progress continues toward the goal of bringing samples until there is a clear order to stop or the money drives up. That wasn’t the case back in March and April when NASA successfully tested two engines that will be used in the Mars Ascent Vehicle (MAV).

A pair of studies published in JGR: Planets and Science Advances discuss new findings from NASA’s James Webb Space Telescope (JWST) regarding Jupiter’s first and third Galilean Moons, Io and Ganymede, and more specifically, how the massive Jupiter is influencing activity on these two small worlds. For Io, whose mass is about 21 percent larger than Earth’s Moon, the researchers made the first discovery of sulfur monoxide (SO) gas on the volcanically active moon. For Ganymede, which is the largest moon in the solar system and boasts twice the mass of the Earth’s Moon, the researchers made the first discovery of hydrogen peroxide, which exists in Ganymede’s polar regions.

It probably comes as no surprise to people suffering through drastic weather this year that our planet is heating up. Climate change is the culprit and researchers continue to look for ways to mitigate its effects. A scientist at the University of Hawai’i suggests a novel approach: create a giant solar shade in space to block enough sunlight to counter climate change.

Aliens are big in the news recently, fueled by congressional hearings about Unidentified Anomalous Phenomena (UAPs), formally known as UFOs. But while the idea of aliens visiting Earth may be exciting, the better bet is still the idea that aliens might exist on distant worlds. We already know potentially habitable planets are common and intelligent life has arisen on at least one world, so why not many? But after 60 years of searching for evidence of extraterrestrials “out there,” we’ve found nothing. So what does that tell us?

Venus and Earth have several things in common. Both are terrestrial planets composed of silicate minerals and metals that are differentiated between a rocky mantle and crust and a metal core. Like Earth, Venus orbits within our Sun’s circumsolar habitable zone (HZ), though Venus skirts the inner edge of it. And according to a growing body of evidence, Venus has active volcanoes on its surface that contribute to atmospheric phenomena (like lightning). However, that’s where the similarities end, and some rather stark differences set in.

Humanity has been on an asteroid-finding spree as of late. Those close to Earth, known as Near Earth Objects (NEOs), have been particularly interesting for two reasons. One is they offer potentially lucrative economic opportunities with asteroid mining. The other is they are potentially devastating if they hit the Earth, so we’d like to find them with some advance warning. Those that fall into the latter category are known as potentially hazardous asteroids, or PHAs. Now, thanks to some ingenious programmers from the University of Washington, we have a new algorithm to detect them.

It’s every space mission’s nightmare: losing contact with the spacecraft. In the best case, you recover it right away. Worst case, you never hear from your hardware again. On July 21, controllers lost contact with Voyager 2, out in the depths of space. Now they’re waiting for a reset to catch Voyager 2’s next message when it “phones home”.

A collaboration of engineers from NASA and academia recently tested hybrid printed electronic circuits near the edge of space, also known as the Kármán line. The space-readiness test was demonstrated on the Suborbital Technology Experiment Carrier-9, or (SubTEC-9), sounding rocket mission, which was launched from NASA’s Wallops Flight Facility on April 25 and reached an altitude of approximately 174 kilometers (108 miles), which lasted only a few minutes before the rocket descended to the ground via parachute.

In 2026, the European Space Agency (ESA) will launch its next-generation exoplanet-hunting mission, the PLAnetary Transits and Oscillations of stars (PLATO). This mission will scan over 245,000 main-sequence F, G, and K-type (yellow-white, yellow, and orange) stars using the Transit Method to look for possible Earth-like planets orbiting Solar analogs. In keeping with the “low-hanging fruit” approach (aka. follow the water), these planets are considered strong candidates for habitability since they are most likely to have all the conditions that gave rise to life here on Earth.

Supermassive black holes haunt the cores of many galaxies. Yet for all we know about black holes (not nearly enough!), the big ones remain a mystery, particularly when they began forming. Interestingly, astronomers see them in the early epochs of cosmic history. That raises the question: how did they get so big when the Universe was still just a baby?