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Japan Prepares to Launch Spacecraft to Collect Samples From Martian Moon Phobos
Japan's space agency JAXA is set to launch the MMX spacecraft on a new H-3 rocket, aiming to make the world's first attempt to bring samples back from Phobos, one of Mars' two small moons. Scientists hope the mission will reveal how Phobos and its sibling Deimos formed, and perhaps shed light on the origins of life in the solar system. The launch comes as the United States, China and others consider sending astronauts to Mars. MMX project manager Yasuhiro Kawakatsu said the samples could help scientists judge whether a Martian moon could serve as a base for a future crewed mission. Some scientists think the moons are debris from a large object that struck Mars, while others say they are asteroids from elsewhere.
Key facts
- The mission is expected to take five years in total.
- The spacecraft reaches the Mars region a year after launch, then studies Phobos for three years.
- MMX is due to return to Earth in 2031 with samples in a heat-protected capsule.
- JAXA aims to collect at least 10 grams of soil from two sampling attempts.
- Material from Mars is expected to make up about 0.1% of the Phobos material collected.
Commentary
Sources: U.S. News & World Report
2
NASA's Roman Space Telescope Performs Nearly 30% Better Than Predicted
NASA's Nancy Grace Roman Space Telescope is performing better than scientists anticipated after engineers completed a series of tests and precision adjustments. Following the activation of the Wide Field Instrument in September, teams checked its detectors, filter wheel, calibration LEDs, alignment mechanism and thermal control system, then refined the telescope's overall optical alignment. Goddard engineers said the mirrors were already positioned with remarkable accuracy before launch, so only minor corrections were needed. The sharper focus matters because the Wide Field Instrument underpins the surveys needed for the mission's dark matter and dark energy goals. Work on the Coronagraph Instrument, which had been slightly out of focus, is continuing, with a light-blocking test planned in the coming weeks.
Key facts
- The Wide Field Instrument's image quality is nearly 30% better than engineers predicted.
- Optical error was measured at 63 nanometers RMS, below the 90-nanometer pre-launch requirement.
- The Wide Field Instrument has 18 detectors, each roughly the size of a sticky note.
- Engineers moved the secondary mirror by about one-sixteenth of a human hair's diameter.
- Roman launched on August 30 with optics that were already closely aligned before the adjustments.
Commentary
Sources: Science Daily
3
NASA data reveals hidden El Niño-driven fires burning beneath the Amazon rainforest
Severe drought linked to El Niño is fuelling wildfires across the Brazilian Amazon, with smoke engulfing Manaus, where schools shut down, public events were canceled and children's sports leagues suspended activities. NASA's Douglas Morton describes the fires as a cascade of tropical blazes that began with peat fires in Indonesia and has now reached the Amazon, which he called the second domino to fall. Many of the larger Amazon blazes began as deliberate land-management fires that escaped into the parched understory. NASA's Shane Coffield is using VIIRS satellite data to find fires that standard monitoring misses, particularly on smoky days when detections fall even as burning continues.
Key facts
- Manaus rainfall was 95 percent below normal in August and 60 percent below in September, per Brazil's meteorology institute.
- Coffield says satellites identified about 40 percent more fires near Santarém than FIRMS active fire counts show.
- Fine particulate matter in Manaus exceeded 135 micrograms per cubic meter, city officials reported.
- Lightning causes less than 1 percent of fires in the Amazon region, according to Morton.
- Fire activity is expected to shift northward in November and December 2026, then southward by August and September 2027.
Commentary
Sources: Science Daily
4
Webb telescope reveals extreme weather on brown dwarf SIMP 0136, 20 light-years away
Researchers at Trinity College Dublin used NASA's James Webb Space Telescope to study SIMP 0136, a brown dwarf about 20 light-years from Earth previously associated with northern-lights-like phenomena. Using Principal Component Analysis on how the object's light changed as it rotated, the team found that nearly all of its atmospheric variability could be explained by two dominant components, consistent with temperature changes and the vertical structure of clouds. They also identified three recurring weather states that come into and out of view as the object turns, forming a shifting patchwork of hotter, thinner-cloud regions and cooler, thicker-cloud regions. The findings, published in Astronomy & Astrophysics, suggest the atmosphere follows a consistent underlying set of processes. Lead author Merle Schrader said the drivers persist over more than a dozen rotations. The team says the method could help astronomers prioritise features for more complex modelling of brown dwarfs and giant exoplanets.
Key facts
- Trinity College Dublin researchers used NASA's James Webb Space Telescope to study SIMP 0136.
- Two dominant components explain nearly all of SIMP 0136's observed atmospheric variability.
- Researchers identified three recurring weather states that appear and disappear as the brown dwarf rotates.
- The findings were published in Astronomy & Astrophysics.
- SIMP 0136 lies about 20 light-years from Earth.
Commentary
Sources: Science Daily
5
Researchers synthesise diamondiyne, a porous 3D carbon material proposed 35 years ago
A team from the University of Gothenburg, Chalmers University of Technology and Stockholm University has synthesised diamondiyne, a porous three-dimensional carbon material first described theoretically 35 years ago. The team reported the work in Angewandte Chemie International Edition on September 14, 2026. The material combines single and triple carbon-carbon bonds in a diamond-like network, and forms as crystalline regions within amorphous carbon films. The researchers made it with a cascade reaction at the interface between two liquids, using a protected precursor and copper(II) fluoride. The team says the method establishes a route to making this elusive structure, while its practical uses remain to be explored and have not been demonstrated.
Key facts
- Diamondiyne was synthesised by researchers from the University of Gothenburg, Chalmers and Stockholm University.
- The study was published in Angewandte Chemie International Edition on September 14, 2026.
- The material was first described theoretically 35 years ago and combines single and triple carbon bonds.
- Films reached up to 2.5 centimetres in diameter, with thickness from a few to tens of nanometres.
- A separate computational study predicted Young's moduli of 19.1 GPa and 75.5 GPa for the experimentally realised 2f-unsym phase.
Commentary
Sources: The Times of India