Space News & Blog Articles

For the first time, a spacecraft has detected acoustic and seismic waves from impacts on Mars. NASA’s InSight lander made the detections from four meteoroids that crashed on Mars in 2020 and 2021. Ever since the mission landed on the Red Planet in 2018, scientists have been hoping to be able to detect impacts with InSight’s seismometer, which was mainly designed to sense Marsquakes. But these impacts are the first the lander has detected.

An article published in Nature Astronomy makes a strong case to declare the orbital space around earth an ecologically protected environment. It was part of a submission to the US Court of Appeals in August last year and was filed by several organisations in response to license amendments granted by the FAA to SpaceX for Starlink satellites. To understand why this is so important, it may help to remember that orbital space is a “common” area, like “International Waters” in our oceans, so it is not currently protected by a single country or organization.

On March 25, 2022, the ESA/NASA Solar Orbiter spacecraft closed in on the Sun, getting ready to study it during a flyby. Its Metis coronagraph instrument, which blocks out the Sun so the spacecraft can study its outer atmosphere, recorded an image of something strange: a distorted, S-shaped “kink” in a small area of plasma flowing from the Sun. It was a magnetic solar switchback.

On September 12, Blue Origin New Shepard mission, NS-23, failed just over one minute into an uncrewed flight, forcing the escape system to eject its New Shepard upper stage capsule, which landed safely near the launch site. Several science experiments were being carried onboard with the original flight plan calling for the capsule to reach an altitude of a little more than 60 miles, which is internationally acknowledged as the edge of space. While the flight was uncrewed and the capsule made a successful soft landing after ejecting, the scenario could have been far more ill-favored if the flight had been crewed with tourists.

In 1916, Karl Schwarzchild theorized the existence of black holes as a resolution to Einstein’s field equations for his Theory of General Relativity. By the mid-20th century, astronomers began detecting black holes for the first time using indirect methods, which consisted of observing their effects on surrounding objects and space. Since the 1980s, scientists have studied supermassive black holes (SMBHs), which reside at the center of most massive galaxies in the Universe. And by April 2019, the Event Horizon Telescope (EHT) collaboration released the first image ever taken of an SMBH.

Europe plans to have its own reusable spacecraft for cargo and crewed missions to LEO and beyond. It’s called SUSIE (Smart Upper Stage for Innovative Exploration). At first glance, it may look like Europe’s answer to SpaceX’s Starship, but it’s not that simple.

Ever since robotic explorers began visiting the Red Planet during the 1960s and 70s, scientists have puzzled over Mars’ surface features. These included flow channels, valleys, lakebeds, and deltas that appear to have formed in the presence of water. Since then, dozens of missions have been sent to Mars to explore its atmosphere, surface, and climate to learn more about its warmer, wetter past. In particular, scientists want to know how long water flowed on the surface of Mars and whether it was persistent or periodic in nature.

Artificial intelligence can do more than paint planets as bowls of soup. It’s now helping researchers acquire better climate change data by teaching Earth observation satellites how to measure ice thickness in the Arctic year-round.

The early universe was a much different place than our own, and astronomers do not fully understand how baby stars grew up in that environment. And while instruments like the James Webb Space Telescope will pierce back into the earliest epochs of star formation, we don’t always have to work so hard – there may be clues closer to home.

Although we have found thousands of exoplanets in recent years, we really only have three methods of finding them. The first is to observe a star dimming slightly as a planet passes in front of it (transit method). The second is to measure the wobble of a star as an orbiting planet gives it a gravitational tug (Doppler method). The third is to observe the exoplanet directly. Now a new study in the Astrophysical Journal Letters has a fourth method.

Uh oh, NASA’s CAPSTONE mission is having problems, A New Shepard Flight fails, Betelgeuse was recently yellow, and of course, another amazing new image from Webb.

In a recent study submitted to High Energy Astrophysical Phenomena, a team of researchers from Japan discuss strategies to observe, and possibly predict precursor signatures for an explosion from Local Type II and Galactic supernovae (SNe). This study has the potential to help us better understand both how and when supernovae could occur throughout the universe, with supernovae being the plural form of supernova (SN). But just how important is it to detect supernovae before they actually happen?

Saturn is a world of surprises. The Voyager 1 and 2 flybys and later on, the Cassini mission, opened our collective eyes to intricate details in its rings and atmosphere. They also gave us up-close and personal looks at those amazing moons. But, one thing they didn’t show us was Saturn’s proposed moon Chrysalis. That’s because it doesn’t exist. Well, actually, it is there, but in the form of those dazzling rings.

If you want to learn about the history of the Sun, then look no further than the Moon. That’s the recommendation of a team of scientists who hope to harness future Artemis lunar missions to help understand the life history of our home star.

On Earth, we all know what changes our landscapes: water and wind erosion, tectonic activity, and volcanism. Today on Mars, wind-driven erosion is hard at work. Wind is an inexorable sculptor everywhere. And, it might have created places where planetary scientists and astrobiologists hunt for traces of primordial Martian life today.

Even after thirty years, and with next-generation telescopes (like the James Webb) hogging all the attention, the Hubble Space Telescope still manages to inspire. Recently, Hubble acquired a breathtaking image of NGC 1961, an intermediate spiral galaxy measuring 220,000 light years in diameter and located about 180 million light-years away in the constellation Camelopardalis. Intermediate spiral galaxies are so-named because they are between “barred” and “unbarred” spiral galaxies, which means they don’t have a well-defined bar of stars at their centers.

In April of this year, the first all-private astronaut mission to the International Space Station was successfully conducted when Axiom Space sent four non-NASA astronauts to space during the 17-day Axiom-1 Mission (Ax-1). Based on the endeavor’s success, NASA and Axiom Space have signed an agreement for the second such mission to the ISS, which will take place in the second quarter of 2023.

One of the fundamental questions in astronomy is how galaxies formed over 13 billion years ago and have evolved ever since. A common feature that astronomers have noted is that most galaxies appear to have supermassive black holes (SMBHs) at their center – like Sagittarius A*, the ~4 million solar mass SMBH at the center of the Milky Way. These monster black holes occasionally swallow up nearby gas, dust, and stars and emit excess energy as powerful relativistic jets. This phenomenon, where the center of a galaxy outshines the stars in the disk, is known as an Active Galactic Nucleus (AGN) or quasar.

Scientists with NASA’s Perseverance Mars rover said today that the rover has collected several “tantalizing” organic rock samples from an ancient river delta on the Red Planet. These samples have now been stowed for a planned future mission that hopes to retrieve the specimens and bring them back to Earth for the first-ever sample return from Mars.

Astronomers have long believed that supernovae and stellar winds drive outflows from galaxies known as superwinds. New research suggests that they may instead be due to a ring of nuclear fire.

On July 12th, 2022, NASA released the first images acquired by the James Webb Space Telescope, which were taken during its first six months of operation. Among its many scientific objectives, Webb will search for smaller, rocky planets that orbit closer to their suns – especially dimmer M-type (red dwarf) stars, the most common in the Universe. This will help astronomers complete the census of exoplanets and gain a better understanding of the types of worlds that exist out there. In particular, astronomers are curious about how many terrestrial planets in our galaxy are actually “water worlds.”