Space News & Blog Articles

In May 2027, NASA's Nancy Grace Roman Space Telescope will launch to space. Appropriately named after the "Mother of Hubble," the telescope will use its 2.4-meter (7.9 ft) wide field of view primary mirror and advanced instruments to investigate the deeper mysteries of the cosmos. Roman will spend 75% of its observing time over its five-year primary mission conducting three core community surveys selected by the scientific community. Among them, Roman will conduct a High-Latitude Time-Domain Survey (HLTDS) to detect tens of thousands of type Ia supernovae.

Sometimes inspiration can strike from the most unexpected places. It can result in a cross-pollination between ideas commonly used in one field but applied to a completely different one. That might have been the case with a recent paper on lightsail design from researchers at the University of Nottingham that used techniques typically used in video games to develop a new and improved structure of a lightsail.

How do tidal forces determine a planet’s orbital evolution, specifically planets in the habitable zone? This is what a recently submitted study hopes to address as an international team of researchers investigated how tidal forces far more powerful than experienced on Earth could influence orbital evolution of habitable zone planets with highly eccentric orbits around low-mass stars. This study has the potential to help researchers better understand the formation and evolution of exoplanets, specifically regarding where we could find life beyond Earth.

Interactions between supernovae and black holes must be exceedingly rare. But that's the only explanation for a very strange explosion found with the Zwicky Transient Facility. In July 2023, the ZTF spotted strange light signals about 730 million light-years from Earth, and AI helped astronomers unravel what they were seeing.

The Three Body Problem isn’t just the name of a viral Netflix series or a Hugo Award winning sci-fi book. It also represents a really problem in astrodynamics - and one that can cause headaches to mission planners in terms of its complexity, but also one that offers the promise of an easier way to enter stable orbits that might otherwise be possible. A new paper from researchers at the Beijing Institute of Technology shows one way those orbital maneuvers might be enhanced while exploring planetary systems - by using a gravity assist from its moons.

In 2020, the Japan Aerospace Exploration Agency's (JAXA) Hayabusa2 spacecraft completed its primary mission when it returned samples of asteroid Ryugu to Earth. In 2023, NASA's OSIRIS-REx also completed its primary mission by returning samples of asteroid Bennu to Earth. Scientists in labs around the world have been studying those samples and have uncovered some surprises.

In the past decade, astronomers have witnessed three interstellar objects (ISOs) passing through the Solar System. This included the enigmatic 'Oumuamua in 2017, the interstellar comet 2I/Borisov in 2019, and 3I/ATLAS in July 2025. This latest object also appears to be a comet based on recent observations that showed it was actively releasing water vapor as it neared the Sun. The detection of these objects, which were previously theorized but never observed, has piqued interest in the origins of ISOs, their dynamics, and where they may be headed once they leave the Solar System.

Exoplanet habitability depends on a whole host of factors, with liquid water at the top of the list. It also needs a stable atmosphere, the right chemistry, and possibly even things like plate tectonics or other geological activity. Planetary magnetic fields are a critical part of the formula, too, but detecting them from Earth's surface is difficult.

Compact, reflective, easy to manufacture mirrors are a critical component for advancing astronomical technology in space. Mirrors are a key component in most telescopes, though they are notoriously hard to manufacture with the necessary precision, especially at large scales. A new paper from researchers in the UK uses additive manufacturing to make a thin, flexible, and lightweight mirror out of aluminum and analyzes its properties to see if it will be useful in applications such as CubeSats.

In the 1960s, astronomers theorized that the Universe was filled with a mysterious mass that did not interact normally with light, which they named "Dark Matter." This theoretical matter is believed to constitute 80% of the Universe's mass, largely in the form of "halos" surrounding galaxies and galaxy clusters. However, even after six decades of searching, scientists have still not found the particle that constitutes this mass. Many candidates have been proposed in that time, including Weakly-Interacting Massive Particles (WIMPs), primordial black holes, and ultralight particles known as "axions."

We already know a decent amount about how planets form, but moon formation is another process entirely, and one we’re not as familiar with. Scientists think they understand how the most important Moon in our solar system (our own) formed, but its violent birth is not the norm, and can’t explain larger moon systems like the Galilean moons around Jupiter. A new book chapter (which was also released as a pre-print paper) from Yuhito Shibaike and Yann Alibert from the University of Bern discusses the differing ideas surrounding the formation of large moon systems, especially the Galileans, and how we might someday be able to differentiate them.

China completes the first tethered test of the Lanyue lunar lander.

Taking a walk is great for inspiration. There have been numerous studies about how people think more clearly on walks, and how new ideas come to them more frequently while doing so. That’s part of the reason some of the most famous minds in history included a daily walk in their schedule. Just such an inspiration must have happened recently to Nicholas Heinz, a scientist at NASA’s Jet Propulsion Laboratory (JPL) in California. On a hike in Arizona he found a rock that could be used as an analog of a unique one found by the Perseverance rover on Mars - and decided to take it back to his lab to study it.

Answers to some of cosmology's most pressing questions are obscured by simple dust. It concerns the Cosmic Noon, a period of time that began around two billion years after the Big Bang, when nearly all galaxies experienced a burst of growth and rapid star formation. Galaxies formed stars at rates 10 to 100 times higher than today, and they became more massive through mergers with other galaxies. Dark matter haloes grew rapidly during this time as well. Astronomers want to understand how galaxies grow and evolve, and the Cosmic Noon and its high star formation rate (SFR) and rapid growth is a critical stage in galactic evolution.

The European research project called "gEICko" aims to develop satellites that can literally stick to space junk and drag it safely out of orbit. The secret lies in synthetic materials that mimic the microscopic structures on the feet of gecko, which allow these remarkable reptiles to cling to virtually any surface using molecular forces called van der Waals interactions.

Imagine the entire universe suddenly blazing with light in a flash that lasted just a brief moment in time and then vanishing, leaving behind the most massive black holes ever discovered. This dramatic scenario forms the heart of a new theory that could solve one of astronomy's biggest mysteries about supermassive black holes and how they got so enormous so quickly after the Big Bang.

The connection between greenhouse gases and space weather might seem surprising, but it illustrates just how interconnected Earth's atmospheric layers really are. While carbon dioxide warms the lower atmosphere by trapping heat, it has the opposite effect in the thin regions of the upper atmosphere, roughly 300-400 miles above Earth's surface. At these extreme altitudes, carbon dioxide actually cools the atmosphere by radiating heat directly into space, causing the air to become significantly less dense over time.

The Event Horizon Telescope (EHT) established a reputation worldwide in 2019 when it released the first-ever image of a black hole. This was made possible by the science of Very Long Baseline Interferometry (VLBI), a technique in which multiple instruments collect light to create a complete picture of what an object looks like. In this case, the image was of the supermassive black hole (SMBH) at the center of Messier 87, a massive galaxy 55 million light-years from Earth. This was followed by images of the relativistic jets emanating from two bright galaxies, and of Sagitarius A*, the SMBH at the center of the Milky Way.

Our Moon is a seismically active world with a long history of quakes stretching back to its early history. It turns out those quakes can and will affect the safety of permanent base structures for anybody planning to explore and inhabit the Moon. That's one conclusion from a study of quakes along the Lee-Lincoln fault in the Taurus-Littrow valley where the Apollo 17 astronauts landed in 1972. “The global distribution of young thrust faults like the Lee-Lincoln fault, their potential to be still active and the potential to form new thrust faults from ongoing contraction should be considered when planning the location and assessing stability of permanent outposts on the Moon,” said Smithsonian senior scientist emeritus Thomas R. Watters, lead author of the paper.

The James Webb Space Telescope has revealed many wonders of the early universe, but few discoveries have puzzled astronomers more than some mysterious "little red dots." These tiny, brilliant galaxies appear scattered across deep space images like cosmic breadcrumbs, challenging everything scientists thought they knew about how galaxies formed in the early universe.

When global events set our minds to wondering if humanity has what it takes to persist, it's natural to wonder about other worlds, other life, other intelligent species, and if those others might be better suited to survive whatever Great Filters they face. Those are fanciful thoughts, but there's an underpinning of nuts-and-bolts thinking to them. It starts with identifying which planets in habitable zones around other stars might actually be habitable.