Space News & Blog Articles

What type of lander could touch down on Jupiter’s volcanic moon, Io? This is what a recent paper presented at the AIAA 2025 Regional Student Conference hopes to address as a team of student engineers from Spartan Space Systems at San Jose State University investigated a novel concept for landing a spacecraft in Io, which is the most volcanically active planetary body in the solar system. This study has the potential to help scientists and engineers develop new mission concepts from all levels of academia and industry.

Launched in 2009, the Kepler Space Telescope revolutionized astronomy by discovering thousands of exoplanets in over 150,000 star systems. Kepler was specifically designed to detect Earth-sized planets by monitoring stars for periodic dips in brightness, which may result from planets passing in front of their star relative to the observer. Known as the Transit Method (or Transit Photometry), this technique has allowed astronomers to identify the majority of the more than 6,000 exoplanets in the current census. However, the method is not perfect and produces some false positives (initially as high as 5%–10%), which can sometimes be caused by other celestial objects.

Most people are familiar with the fact that the Earth spins on its axis once every day. The spin however, isn’t as steady as you might think. Like a spinning top slowing down, Earth’s axis wobbles, scribing out a circle on the night sky that currently points very close to the Pole Star in the northern hemisphere. The wobble occurs because Earth isn't a perfect sphere but bulges slightly at the equator. When the Sun and Moon pull on this bulge with their gravity, they create a force that tries to tilt Earth's axis. However, because Earth is already spinning, this tilting force doesn't simply tip the planet over. Instead, it causes the axis to trace out a slow circular wobble in the sky, much like a spinning top wobbles as it slows down. This wobble takes approximately 26,000 years to complete one full cycle.

Planets and moons are inseparable companions and while astronomers are unravelling the complexity of planet formation, moon formation remains mysterious. Our Solar System is fully formed, so to observe exoplanet and exomoon formation, we have to look to other stars. But while we're getting better at detecting exoplanets, detecting exomoons is much more challenging. Their small sizes relative to the exoplanets they orbit renders them practically invisible.

The KM3NeT Collaboration, a network of neutrino detectors based in the Mediterranean, announced in February that they had found the highest-energy neutrino detected to date. In a recent study, researchers from MIT proposed that this "ghost particle" could be the product of energetic Hawking Radiation emitted by a Primordial Black Holes (PBH) after it decayed outside our Solar System. If true, these findings could be the first evidence of the theoretical radiation Hawking proposed in 1974 by combining quantum field theory and General Relativity.

How will NASA’s upcoming Habitable Worlds Observatory (HWO) mission differentiate Earth-sized exoplanets from other exoplanets, specifically Earth-sized exoplanets within the habitable zone, also called exoEarths? This is what a recent study accepted for publication in The Astronomical Journal hopes to address as an international team of researchers investigated the potential future capabilities of HWO and what shortcomings need to be addressed for it to conduct groundbreaking science, specifically with discovering exoEarths.