Saturday, March 14, 2026

NASA's DART Mission Also Changed Didymos' Orbit Around Sun

This image of asteroids Didymos, left, and Dimorphos was captured by NASA’s DART mission a few seconds before the spacecraft smashed into Dimorphos on Sept. 26th, 2022. Credit: NASA/Johns Hopkins APL

The spacecraft changed the binary system’s orbit, confirming that a kinetic impactor can be an effective planetary defense technique for deflecting a near-Earth object.



Is the Universe Defective? Part 1: The Good Old Days

Credit: ESA and the Planck Collaboration

Every time you flip a light switch, or check the time, or feel the sodium ions wiggling in your brain — don’t think about that one too much—you’re assuming something fundamental. You’re assuming the universe is a finished product. A completed work. You think the Big Bang happened, the forces of nature settled into their seats, and we’ve been cruising on a smooth, predictable ride ever since.



The Universe's Most Powerful Particle Accelerators Were Here All Along

Cutaway drawing of two radiation belts around Earth; the inner belt (red) dominated by protons and the outer one (blue) by electrons. (Credit : JHUAPL, NASA)

Every planet with a magnetic field has a radiation belt, a region of space where charged particles get trapped and flung around at extraordinary speeds. Earth has two of them, and they've been puzzling scientists for decades. Now, a physicist at the University of Helsinki has built a model that defines a universal upper limit to just how energetic those belts can ever get. The answer applies not just to Earth, but to every planet in the Solar System, every gas giant, and even the strange objects sitting halfway between planets and stars.



Friday, March 13, 2026

A Glorious Spiral of Star Formation

This is the spiral galaxy NGC 5134, captured by the JWST in both near-infrared and mid-infrared. Images of nearby spiral galaxies like this one are important for studying star formation. The image is the ESA's Picture of the Month. Image Credit: ESA/Webb, NASA & CSA, A. Leroy

Stars peek through the dusty, winding arms of NGC 5134, a spiral galaxy located 65 million light-years away, in this Feb. 20, 2026, image from NASA’s James Webb Space Telescope. Webb’s Mid-Infrared Instrument collects the mid-infrared light emitted by the warm dust speckled through the galaxy’s clouds, tracing the clumps and strands of dusty gas. The telescope’s Near Infrared Camera records shorter-wavelength near-infrared light, mostly from the stars and star clusters that dot the galaxy’s spiral arms. The image helps researchers understand star formation in spiral galaxies. Image Credit: ESA/Webb, NASA & CSA, A. Leroy



Why Are Interstellar Comets So Weird? Part 4: We Finally Turned On the Porch Lights

Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/AURA/H. Stockebrand

So that's all nice. But why now? That's the question everyone asks. We went decades — centuries, millennia really — without seeing a single rock that didn't have a "Made in the Solar System" sticker on it. Then, in the span of less than ten years, we get the Big Three: 'Oumuamua, Borisov, and now 3I/ATLAS.



Thursday, March 12, 2026

ESA's Mars orbiters watch solar superstorm hit the Red Planet

Images of the 2024 solar storm captured by NASA's Solar Dynamics Observatory's instruments, developed by the ESA/NASA. The bright spots to the right of the Sun are Jupiter and Venus. Credit: NASA/ESA

What happens when a solar superstorm hits Mars? Thanks to the European Space Agency’s Mars orbiters, we now know: glitching spacecraft and a supercharged upper atmosphere.



This Isn't Just Another Rocky World Orbiting a Red Dwarf. This One's Special

This artist's illustration shows an exoplanet orbiting a dim red dwarf star. There are many unanswered questions about the survival of atmospheres on rocky world around M-dwarfs like this. Astronomers have found a red dwarf with an orbiting rocky exoplanet that is so well-understood it can serve as a benchmark for studies of exoplanet atmospheres. NASA/ ESA/ CSA/ Joseph Olmsted (STScI)/ Webb Space Telescope.

Rocky planets are found in abundance around M-type stars (red dwarfs), so finding another one doesn't always generate headlines. But an international team of astronomers say that one recent M-dwarf rocky planet found by TESS is especially noteworthy. This one can serve as a benchmark for comparative studies of this type of exoplanet and their at-risk atmospheres.