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Mars, by virtue of its tenuous atmosphere and proximity to our solar system’s asteroid belt, is far more vulnerable than Earth to being struck by space rocks – one of the many differences between the two planetary neighbours.

Scientists are now gaining a fuller understanding of this Martian trait, with help from NASA’s robotic InSight lander. Researchers on Monday described how InSight detected seismic and acoustic waves from the impact of four meteorites and then calculated the location of the craters they left – the first such measurements anywhere other than Earth.

The researchers used observations from NASA’s Mars Reconnaissance Orbiter in space to confirm the crater locations.

“These seismic measurements give us a completely new tool for investigating Mars, or any other planet we can land a seismometer on,” said planetary geophysicist Bruce Banerdt of NASA’s Jet Propulsion Laboratory, the InSight mission’s principal investigator.

The space rocks InSight tracked – one landing in 2020 and the other three in 2021 – were relatively modest in size, estimated to weigh up to about 440 pounds (200kg), with diameters of up to about 20 inches (50cm) and leaving craters of up to about 24 feet (7.2meters) wide. They landed between 53 miles (85km) and 180 miles (290km) from InSight’s location. One exploded into at least three pieces that each gouged their own craters.

“We can connect a known source type, location and size to what the seismic signal looks like. We can apply this information to better understand InSight’s entire catalog of seismic events, and use the results on other planets and moons, too,” said Brown University planetary scientist Ingrid Daubar, a co-author of the study published in the journal Nature Geoscience.

The researchers believe that now the seismic signature of such impacts has been discovered they expect to find more contained in InSight’s data, going back to 2018.

The three-legged InSight – its name is short for Interior Exploration Using Seismic Investigations, Geodesy and Heat Transport – landed in 2018 in a vast and relatively flat plain just north of the Martian equator called Elysium Planitia.

“The moon is also a target for future meteor impact detection,” said planetary scientist and study lead author Raphael Garcia of the University of Toulouse’s ISAE-SUPAERO institute of aeronautics and space.

“And it may be the same sensors will do it, because the spare sensors of InSight are currently integrated in the Farside Seismic Suite instrument for a flight to the moon in 2025,” Garcia added, referring to an instrument due to be placed near the lunar south pole on the side of the moon permanently facing away from Earth.

Mars is about twice as likely as Earth to have its atmosphere hit by a meteoroid – the name for a space rock before it strikes the surface. However, Earth has a much thicker atmosphere that protects the planet.

“So meteoroids usually break up and disintegrate in the Earth’s atmosphere, forming fireballs that only rarely reach the surface to form a crater. In comparison on Mars, hundreds of impact craters are forming somewhere on the planet’s surface every year,” Daubar said.

The Martian atmosphere is only about 1 percent as thick as Earth’s. The asteroid belt, an abundant source of space rocks, is located between Mars and Jupiter.

The scientific goals set for InSight ahead of the mission were to investigate the internal structure and processes of Mars, as well as studying seismic activity and meteorite impacts.

InSight’s seismometer instrument established that Mars is seismically active, detecting more than 1,300 marsquakes. In research published last year, seismic waves detected by InSight helped decipher the internal structure of Mars, including the first estimates of the size of its large liquid metal core, thickness of its crust, and nature of its mantle.

© Thomson Reuters 2022

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Crystalline Ice Discovered in Space: New Study Reveals Hidden Order in Cosmic Ice

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July 15, 2025

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Crystalline Ice Discovered in Space: New Study Reveals Hidden Order in Cosmic Ice

Water ice coats many outer solar system bodies – from Jupiter’s icy moon Ganymede (above) to interstellar dust. On Earth, ice freezes into a neat crystal lattice, but in the deep cold of space it was assumed to form a completely amorphous (glassy) solid. A new study by University College London and Cambridge scientists challenges this picture. Their computer simulations and X-ray tests on cosmic “low-density” ice suggest it actually contains tiny crystalline grains. In some models roughly 20–25% of the ice was in crystal form, overturning the long-held view that space ice is entirely structureless.

Simulations reveal hidden nanocrystals

According to the paper, computer simulations of space ice showed it contains nanocrystals. In one approach, researchers cooled virtual water to –120 °C at different rates to form model “ice cubes.” Depending on the cooling speed, the simulated ice ranged from fully amorphous to partly ordered. Structures with roughly 16–19% of the molecules in tiny crystal clusters best matched published X-ray data for low-density ice. In another simulation, thousands of nanometer-sized ice grains were packed together and then the remaining water molecules were randomized. This produced ice about 25% crystalline, yet still reproduced the known diffraction pattern.

In laboratory experiments the team also made actual low-density amorphous ice by vapor deposition and gentle compression. When these samples were slowly warmed to crystallize, the resulting ice showed a “memory” of its formation method.

Implications for planets and origins of life

The findings give “a good idea of what the most common form of ice in the Universe looks like at an atomic level,” which is important for models of planet and galaxy formation. They also bear on theories of life’s origins. Partly crystalline ice has less internal space to trap organic molecules, potentially making it a less efficient vehicle for amino acids or other prebiotic compounds. However, Dr. Davies notes that pockets of fully amorphous ice still exist, so cosmic dust grains and cometary ices could continue to harbor organic ingredients in those disordered regions.

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space ice, amorphous ice, crystalline ice, UCL, University of Cambridge, nanocrystals, planetary science, origins of life, X-ray diffraction, space research, Physical Review B

NASA Deploys High-Tech Aircraft to Support Texas Flood Relief and Recovery Efforts



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Axiom Space’s Ax-4 Crew Returns from ISS Aboard SpaceX Dragon Grace After Record Research Mission

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July 15, 2025

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Axiom Space’s Ax-4 Crew Returns from ISS Aboard SpaceX Dragon Grace After Record Research Mission

The latest mission of Axiom Space with the four astronauts has found their stay aboard the International Space Station (ISS). SpaceX Crew Dragon capsule called Grace, unboarded from the ISS on July 14, 2025, carrying the quartet on the last leg of Ax-4 mission at 4:45 p.m. IST. It safely manoeuvred away from the orbit’s lab, which was the crew’s home for more than 2.5 weeks. Further, it performed the deorbit burn series and is on the path to come back to Earth at around 3:00 p.m. IST.

Ax-4 Mission Wraps Up After Extended ISS Stay and Record-Setting Research

As per NASA, The former NASA astronaut Peggy Whitson is the commander, and the other crew members are pilot Shubhanshu Shukla and mission specialist Sławosz Uznański-Wiśniewski and Tibor Kapu. it is the first spaceflight for all three. However, its fifth mission for Whitson to orbit is recorded as 695 cumulative days.

The mission is an extension of the Houston-based company’s previous crewed flights, and is for research and science investigations which aim for the understanding of microgravity milieu. So far, Ax-4 has conducted 60 experiments and tech demos with contributions from 31 countries, as well as a number of public outreach events, and has broken the record as it continues to refine the orbital operations.

SpaceX Dragon Capsule Grace Returns via Pacific Splashdown

The mission was launched on a SpaceX Falcon 9 rocket on June 26, 2025, from NASA’s Kennedy Space Centre, in Florida, and the crew was scheduled to stay aboard the space station for almost two weeks. This mission lasted four days longer than predicted. Departure started this morning, and now the crew and Dragon are on a 22.5-hour path on course for splashing down in the Pacific Ocean till the end of the day.

This will be the second West Coast crew recovery of SpaceX, while the first was of the Crew-9 ISS mission during March. SpaceX completely shifted to the Pacific Ocean, rather than the Gulf or the Atlantic, after the events of debris from Dragon’s trunk and crashing back to Earth. This new reentry minimises the chance of debris, said the representatives of SpaceX.

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NASA Deploys High-Tech Aircraft to Support Texas Flood Relief and Recovery Efforts

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July 15, 2025

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NASA Deploys High-Tech Aircraft to Support Texas Flood Relief and Recovery Efforts

NASA deployed two aircrafts to help state and local authorities in the continuing recovery operations, in response to the flood near Kerrville, Texas. The aircrafts are from NASA’s Disasters Response Coordination System, and is activated to support the emergency response for flood and is closely working with the Texas Division of Emergency Management, the humanitarian groups Save the Children and GiveDirectly, and the Federal Emergency Management Agency. Persistent cloud-cover over there has made it quite difficult to capture the clear satellite images.

NASA Deploys Aircraft with Advanced Sensors for Texas Flood Response

As reported by NASA, if this can be done, the NASA’s Airborne Science Program can concur a series of flights to fetch observations of te impacted areas. NASA is sharing this data with emergency response teams to inform the search and rescue efforts and help in resource allocation and decision making. WB-57 aircraft departed from Ellington Field on July 8, 2025 for conducting aerial surveys. The aircraft is loaded with the DyNAMITE which is known as Day/Night Airborne Motion Imager for Terrestrial Environments sensor.

Real-Time Data and Imagery Aid Emergency Teams and Flood Recovery Efforts

The DyNAMITE views the Guadalupe River and many miles of the surrounding area, and provides high-resolution imagery which is important to evaluate the damage and support coordination of the foundation-based recovery efforts. This system enables the real-time data collection and analysis, which enhances the situational awareness and enhancing emergency response times.

Further, the agency’s Uninhabited Aerial Vehicle Syntehtic Aperture Radar (UAVSAR) aboard the Gulfstream III. UAVSAR is managed by Jet Propulsion Laboratory in Southern California and is planning to collect the observations over the Guadalupe, San Gabriel, and Colorado river basins on three weekdays, Wednesday, Thursday, and Friday. It can penetrate the vegetation to see water that sensors are unable to detect. The goal of the team is to characterise the flood extent of flood and help the understanding of the damage amount within communities.

Further, the Disasters are being coordinated with FEMA, the local responders and the Texas Division of Emergency Management for ensuring the data is quickly delivered to the decision making people on the ground. The data is being shared on the NASA Disasters Mapping Portal as soon as it is available.

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