Tuesday, July 7, 2026

Another Success for Hayabusa 2 as it Completes a Flyby of Asteroid Torifune

JAXA's Hayabusa 2 spacecraft has delivered our first closeup image of asteroid Torifune. The image clearly shows that the asteroid is a contact binary made of a pair of once separate asteroids that joined together. Image Credit: JAXA, The University of Tokyo, Chiba Institute of Technology, Institute of Science Tokyo, AIST, Paris Observatory, IAC.

JAXA's Hayabusa 2 has completed its flyby of asteroid Torifune. The spacecraft came within about 800 meters of the asteroid's surface. Though the spacecraft is travelling very rapidly, making navigation challenging, it was still able to capture clear images of the asteroid's boulder-strewn surface. Based on ground-based observations, scientists suspected that Torifune was a contact binary asteroid, and these images confirm it.



The Euclid Space Telescope Has Found 31 New Ancient Quasars, Including the Most Ancient One Ever Found

This artist's illustration shows a quasar, an extremely luminous AGN powered by a supermassive black hole. The Euclid space telescope has found 31 new quasars in the high-redshift Universe, which can be used to probe dark matter distribution in the early Universe. Image Credit: ESA. Licence: CC BY-SA 3.0 IGO or ESA Standard Licence

Euclid is only 1.5 years into its Euclid Wide Survey and has found 31 new quasars from the Universe's first 800 million years. Though the Survey isn't specifically aimed at finding ancient quasars, it's proving to be remarkably effective at it. This large sample of quasars will help with the study of ancient galaxies and supermassive black holes.



Astronomers Using Chandra Data Produce the Most Detailed View of the M87 Jet in X-rays

The powerful jet emanating from the supermassive black hole at the center of the M87 galaxy. Credit: NASA/ESA/STScI

Combining data from NASA's Chandra X-ray Observatory with advanced image-processing techniques to produce the sharpest X-ray view yet of the relativistic jet from M87's supermassive black hole.



Galaxy Mergers Aren't Always Obvious

The JWST's Mid-Infrared Instrument (MIRI) captured this image of the galaxy Centaurus A. MIRI revealed otherwise hidden structures and dust in the galaxy, including looping patterns and filaments. These are evidence of a past collision. The image also shows the galaxy's supermassive black hole, which is actively feeding and luminous. Image Credit: NASA, ESA, CSA, STScI. Image Processing: A. Pagan (STScI), J. Depasquale (STScI), M. Garcia Marin (ESA Office at STScI)

Mergers are a part of a galaxy's life in this Universe. Though clear signs of these mergers fade over hundreds of millions of years, evidence is still present, yet obscured, in the galaxies that experience them. The powerful JWST has made it possible to find this evidence, and it did so recently for Centaurus A.



Monday, July 6, 2026

University Team Proposed Retractable, Pressurized Tunnels for Missions to Mars

![System Concept of Operations for the HATCH concept. Credit: BLiSS team/NTRS](/article_images/Screenshot_2026-07-04_at_18-23-20_UMich_BLiSS_XHab_LATCH_Final_Rpt_1.pdf_20260706_175317.png) *System Concept of Operations for the HATCH concept. Credit: BLiSS team/NTRS*

As part of NASA's Moon to Mars eXploration Systems and Habitation (M2M X-Hab) 2026 Academic Innovation Challenge, a University of Michigan team proposed an actuated, pressurized tunnel system that would save countless hours of work and preparation by connecting the astronaut's habitat with other surface elements.



Andromeda's Newest Dwarf Galaxy is Extremely Dim

Andromeda XXXVI (And 36) is shown in red in this image. It's one of many dwarf galaxies found around Andromeda, or M31, in the center of the image. And 36 is about 12.5 billion years old and is about 390,000 light years away from Andromeda. Image Credit: Sakowska et al. 2026. A&A.

Astronomers have discovered an extremely low-mass and dim dwarf galaxy around Andromeda. Called And 35, it's an Ultra-Faint Dwarf Galaxy (UFDG) and so far, the researchers have detected only 46 of its stars. Lambda-CDM predicts that there should be many UFDGs around galaxies like Andromeda and the Milky Way, so finding more of them is important.



New Horizons Watches the Solar Wind as it Slows Down

An artist's conception of the heliosphere, the bubble generated by the Sun's magnetic field and envelopes the solar system. The Sun generates the solar wind that flows out past the planets. Credit: NASA's Goddard Space Flight Center Conceptual Image Lab

Where does the Solar System end and interstellar space begin? That's a question scientists have been working to answer using spacecraft traveling out beyond the Sun's influence. A team of researchers from the Southwest Research Institute led by Heather Elliott, is using the Solar Wind around Pluto instrument onboard New Horizons to track the solar wind in the outer reachers of the Solar System.