Why JWST and Ariel Are Better Together

By Andy Tomaswick - February 12, 2026 03:04 PM UTC | Missions
Astronomers want to collect as much data as possible using as many systems as possible. Sometimes that requires coordination between instruments. The teams that run the James Webb Space Telescope (JWST) and the upcoming Atmospheric Remote-sensing Infrared Exoplanet Large-survey (Ariel) missions will have plenty of opportunity for that once both telescopes are online in the early 2030s. A new paper, available in pre-print on arXiv, from the Ariel-JWST Synergy Working Group details just how exactly the two systems can work together to better analyze exoplanets.
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The Balloon Mission Raising the Bar for Exoplanet Science

By Andy Tomaswick - February 12, 2026 12:32 PM UTC | Exoplanets
DOI: arXiv:2602.04840 | arXiv:2602.04840v1 Announce Type: new Abstract: The EXoplanet Climate Infrared TElescope (EXCITE) is a balloon-borne mission dedicated to measuring spectroscopic phase curves of hot Jupiter-type exoplanets. Phase curve measurements can be used to characterize an exoplanet's longitude-dependent atmospheric composition and energy circulation patterns. EXCITE carries a 0.5 m primary mirror and moderate resolution diffraction-limited spectrograph with spectral coverage from 0.8--3.5 um. EXCITE is...
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New Sungrazer Comet A1 MAPS Could Be Bright in Early April If It Survives Perihelion

By David Dickinson - February 11, 2026 05:28 PM UTC | Observing
In a clockwork predictable Universe, comets and how they will ultimately perform is always a big wild card. A new sungrazer comet discovered at the start of this year has given astronomers pause. C/2026 A1 MAPS could put on a memorable if brief show in early April, if it doesn’t join the long list of comets that failed to live up to expectations.
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The Radical Propulsion Needed to Catch the Solar Gravitational Lens

By Andy Tomaswick - February 11, 2026 01:18 PM UTC | Missions
Sending a mission to the Solar Gravitational Lens (SGL) is the most effective way of actually directly imaging a potentially habitable planet, as well as its atmosphere, and even possibly some of its cities. But, the SGL is somewhere around 650-900 AU away, making it almost 4 times farther than even Voyager 1 has traveled - and that’s the farthest anything human has made it so far. It will take Voyager 1 another 130+ years to reach the SGL, so obviously traditional propulsion methods won’t work to get any reasonably sized craft there in any reasonable timeframe. A new paper by an SGL mission’s most vocal proponent, Dr. Slava Turyshev of NASA’s Jet Propulsion Laboratory, walks through the different types of propulsion methods that might eventually get us there - and it looks like we would have a lot of work to do if we plan to do it anytime soon.
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Can Life Begin on a Moon Without a Sun?

By Andy Tomaswick - February 11, 2026 11:46 AM UTC | Exoplanets
Free-Floating Planets, or as they are more commonly known, Rogue Planets, wander interstellar space completely alone. Saying there might be a lot of them is a bit of an understatement. Recent estimates put the number of Rogue Planets at something equivalent to the number of stars in our galaxy. Some of them, undoubtedly, are accompanied by moons - and some of those might even be the size of Earth. A new paper, accepted for publication into the Monthly Notices of the Royal Astronomical Society, and also available in pre-print on arXiv, by David Dahlbüdding of the Ludwig Maximilian University of Munich and his co-authors, describes how some of those rogue exo-moons might even have liquid water on their surfaces.
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Hunting for the Lunar Debris Hiding Near Earth

By Andy Tomaswick - February 10, 2026 12:35 PM UTC | Observing
The Moon has a long history of being smacked by large rocks. Its pock-marked, cratered surface is evidence of that. Scientists expect that, as part of those impacts, some debris would be scattered into space - and that we should be able to track it down. But so far, there have been startlingly few discoveries of these Lunar-origin Asteroids (LOAs) despite their theoretical abundance. A new paper from Yixuan Wu and their colleagues at Tsinghua University explains why - and how the Vera Rubin Observatory might help with finding them.
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How a Single Martian Storm Triggered Massive Water Loss

By Andy Tomaswick - February 10, 2026 11:09 AM UTC | Planetary Science
Mars’ water disappeared somewhere, but scientists have been disagreeing for years about where exactly it went. Data from rovers like Perseverance and Curiosity, along with orbiting satellites such as the Mars Reconnaissance Orbiter and ExoMars have shown that Mars used to be a wet world with an active hydrodynamic cycle. Obviously it isn’t anymore, but where did all the water go? A new paper that collects data from at least six different instruments on three different spacecraft provides some additional insight into that question - by showing that dust storms push water into the Red Planet’s atmosphere, where it is actively destroyed, all year round.
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Research Reveals Why Tatooine Planets are Rare

By Matthew Williams - February 10, 2026 12:48 AM UTC | Exoplanets
Why are planets rarely found orbiting a pair of stars? UC Berkeley and American University of Beirut physicists find that general relativity makes the orbit of a tight binary pair precess. As the orbit shrinks because of tidal effects, the precesion increases. Eventually the precession matches the orbital precession of any circumbinary planet, creating a resonance that makes the planet’s orbit wildly eccentric. The planet either gets expelled from the system or is engulfed by one of the stars.
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A Dense Clump Of Dark Matter, Not A Supermassive Black Hole, Could Reside In The Milky Way's Center.

By Evan Gough - February 09, 2026 07:37 PM UTC | Milky Way
There's been widespread agreement that a supermassive black hole resides in the Milky Way's Center. But that may not be true. Researchers say that a dense clump of fermionic dark matter can also explain the motions of stars and gas clouds in the region. Crucially, it can also explain the famous Event Horizon Telescope image of the SMBH.
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Using Foldable Structures To Guide Microwaves

By Andy Tomaswick - February 09, 2026 03:26 PM UTC | Space Exploration
Origami and space exploration might not seem like they have much in common, but the traditional paper-folding technique solves one massive problem for space exploration missions - volume. Satellites and probes that launch in rocket housings are constrained by very restrictive requirements about their physical size, and options for assembling larger structures in orbit are limited to say the least. Anything that can fold up like an origami structure and then expand out to reach a fully functional size is welcome in the space community, and a new paper published in Communications Engineering by Xin Ning of the University of Illinois Urbana-Champaign (UIUC) and his lab describes a novel use case for the idea - electromagnetic waveguides.
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Decoding China’s New Space Philosophy

By Andy Tomaswick - February 09, 2026 02:23 PM UTC | Space Policy
A major theme in communist governments is the idea of central planning. Every five years, the central authorities in communist countries lay out their goals for the country over the course of the next five years, which can range from limiting infant mortality to increasing agricultural yield. China, the largest current polity ruled by communists, recently released its fifteenth five-year plan, which lays out its priorities for 2026-2030. This one, accompanied by a press release of the China Aerospace Science and Technology Corporation (CASC), the country’s state-owned giant aerospace corporation, has plenty of ambitious goals for its space sector.
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An International Team Uncovers What Powers Auroras

By Matthew Williams - February 08, 2026 07:47 PM UTC | Planetary Science
A new study co-led by the Department of Earth and Planetary Sciences at The University of Hong Kong (HKU) and the Department of Atmospheric and Oceanic Sciences at the University of California, Los Angeles (UCLA) reveals that plasma waves traveling along Earth’s magnetic field lines act like an invisible power source, fueling the stunning auroral displays we see in the sky.
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