Thursday, April 9, 2026

Scientists Spot a Solar Flare With Surprising Spectral Behavior

The Sun as it appeared in H-alpha on September 18, 2022. Solar physicists used the Daniel K. Inouye solar telescope to zero in on the active region at the lower right on September 19, 2022, at the end of a very busy week of solar activity. Courtesy CESAR Helios Observatory.

On August 19, 2022, astronomers using the Daniel K. Inouye Solar Telescope (DKIST) on the Hawaiian island of Maui caught the fading remnants of a C-class solar flare. Their observations showed something unusual: very strong spectral fingerprints of calcium II H and hydrogen-epsilon lines. It was the first time these two light signatures were seen in great detail during a flare. According to computer models, those lines were stronger than expected and play a not well-understood role in how flares heat the solar atmosphere where they occur.



NASA Releases Images of Artemis II's Flight Behind the Moon

Earthset captured through the Orion spacecraft window at 6:41 p.m. EDT, April 6, 2026, during the Artemis II crew’s flyby of the Moon. Credit: NASA

The first flyby images of the Moon captured by NASA’s Artemis II astronauts during their historic test flight reveal some regions no human has seen, including a rare in-space solar eclipse. Released Tuesday, astronauts captured the images April 6 during the mission’s seven-hour flyby of the lunar far side, showing humanity’s return to the Moon’s […]



A Baby Star Blows A Giant Gaseous Ring

This artist's illustration shows the young protostar MC 27 and its protostellar disk in the lower right. The large, 1,000 au ring of gas is shown, along with magnetic field lines penetrating the ring. Image Credit: Y. Nakamura, K. Tokuda et al. 2026. ApJL

Observing the Taurus Molecular Cloud, a research team led by Kyushu University has found that during the early growth period of a baby star, the protostellar disk blows magnetic flux 1,000 au in size and creates a giant, relatively warm ring. Describing these phenomena as a baby star’s “sneezes,” these expulsions of energy and gas help the star to properly develop.



Could We Actually Terraform Mars? A New Scientific Roadmap Lays Out the Blueprint—And the Risks

Realistic depiction of a terraformed Mars. Credit - Daein Ballard

Reading the Mars Trilogy by Kim Stanley Robinson brings the benefits and pitfalls of efforts to terraform the Red Planet into sharp relief. Since the 1970s, when Carl Sagan first suggested the possibility that we could make Mars more Earth-like, that process has been a staple of science fiction. But there’s always been a significant amount of humanity that thinks we shouldn’t. A new paper available in pre-print on arXiv from Edwin Kite of the University of Chicago and his co-authors skirts around the ethical and moral questions of whether we should and tries to take a long hard look at whether we can.



Wednesday, April 8, 2026

Webb's Picture of the Month Features Two Planet-Forming Disks and a Possible Planet

Two images of protoplanetary discs side-by-side, courtesy of the JWST. Credit: ESA/NASA/CSA/ESO/NAOJ/NRAO/G. DuchĂȘne/M. Villenave

Two images of protoplanetary disks side-by-side. The left image shows a dark horizontal band covering the star, with broad, colorful, conical outflows above and below it, and a narrow jet pointing directly up and down from the star. The right image shows the star within a yellow dusty disk, with scattered dust creating purple lobes above and below the disk. Each is on a black background with several galaxies or stars around it.



A Mercury Rover Could Explore the Planet by Sticking to the Terminator

A view of Mercury's Terminator region, as seen by NASA's MESSENGER probe. Credit: NASA/JPL-Caltech

A Mercury lander mission would create opportunities to sample unique geological features. However, extreme temperature fluctuations on Mercury’s surface pose challenges for exploration on the planetary surface. In a narrow region near the terminator, temperate conditions would allow a rover to run on solar power and collect data and surface samples without needing to withstand the extreme heat.



A New Class of Star: Merger Remnant

This artist's illustration shows two white dwarf stars merging. Usually, the merger creates a supernova, but new research concludes that two separate and unusual white dwarfs are best explained as merger remnants. The researchers say they are a new class of object. Image Credit: University of Warwick/Mark Garlick

In the vastness of the Universe, any new object with interesting properties can spur the search for similar objects, potentially establishing a new class of stars. In a paper published in Astronomy & Astrophysics and an arXiv preprint, researchers from the Institute of Science and Technology Austria (ISTA) describe two stellar remnants that share five properties, including X-ray emission, despite being isolated objects. According to the team, these two remnants are sufficient to define a new class of stars.