One of the challenges of searching for life in the Universe is that there is no single universal biosignature that could reveal its presence. Even if we could tell the difference between chemicals produced by living organisms and those from non-living sources like volcanoes, we're still making the assumption that alien life would resemble life on Earth. A new paper proposes that missions search for “energy-ordered resource stratification” which only happens when both self-replication and ecological competition are present.

The Japanese Aerospace Exploration Agency (JAXA) has performed revolutionary science with its Hayabusa and Hayabusa 2 missions

Multiple space agencies are looking to the Moon as a future destination for exploration and development. This will include the creation of permanent infrastructure that will enable regular crewed missions and possibly future settlers. It is also hoped that this infrastructure

The human perception of stars is that they are largely unchanging although of course in reality stars and their host galaxies do change over time, just very VERY slowly. When galaxies deplete their star forming materials, they traditionally become redder as short lived stars die while long lived dwarf stars persist for trillions of years. However, recent research challenges this understanding.

Random flashes of radiation in the sky are not all that unusual. A few years ago, once such flash was detected coming from a star that at the time, was believed to be from a star consuming a planet! The exact mechanism was unsure though for example; was it the star bloating up as a red giant and engulfing the planet or did the planet spiral in toward the star? The answer was until now, a little elusive. Observations from the James Webb Space Telescope showed the environment around the star didn’t match a red giant so it must have been the planet crashing into the star!

The two most prominent satellite galaxies of the Milky Way are the Large and Small Magellanic Clouds. A team of astronomers have recently tracked the movements of 7,000 stars in the Small Magellanic Cloud (SMC) and found that many of them are being pulled away towards the Large Magellanic Cloud! It seems the SMC is being pulled apart, perhaps leading to its eventual destruction as the tidal forces strip away its stars!

One of the things about astronomy that captivates me is that for every question we answer, we open up a whole bunch of other questions. Dark matter and dark energy are one such phenomenon that rather continues to confound us. There’s also the mystery of missing infrared light too but a team of astronomers think they may have found it! The team examined a region of sky using the Herschel Space Telescope and, by staking 141 images, found where individual dust-rich galaxies appeared blended together. The galaxies are absorbing starlight and re-emitting infrared radiation, and is this that may well account for the missing light.

Mars is a cold, dry desert, but it could be possible to rapidly increase the temperature of the planet by releasing particles into the atmosphere. Researchers investigated two possible chemicals: graphene or aluminum. With just two liters per second of release, we could double the Mars greenhouse effect, raising its temperature by +5 Kelvin in only 1.1 years. Once the chemical release is stopped, the planet would cool back to its normal state.

Thanks to the Apollo missions and countless robotic explorers, our understanding of the physical conditions, composition, and geological history of the Moon has advanced considerably. For example, analysis of lunar rocks, regolith, and seismic measurements of the Moon's

What can exozodiacal dust, also called exozodi, teach astronomers about identifying Earth-like exoplanets? This is what a recently submitted NASA white paper—which highlights key findings from the annual Architecture Concept Review—hopes to address as a team of researchers discussed how exozodi orbiting within a star’s habitable zone (HZ) could interfere with detecting Earth-like exoplanets. This study has the potential to help scientists better understand observational constraints of observing Earth-like exoplanets and what improvements could be made for future telescopes and instruments to overcome these constraints.