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Images captured by NASA’s Curiosity rover have shown rare iridescent clouds drifting across the Martian sky. These formations, observed in the planet’s twilight, were seen at high altitudes where sunlight still reaches them despite nightfall on the surface. The images were taken on January 17, using one of the rover’s onboard cameras, with individual frames stitched together to create a time-lapse video. Scientists are analysing these cloud patterns to gain insights into Mars’ atmospheric processes and climate conditions.

Details of the Findings

A report from NASA’s Jet Propulsion Laboratory (JPL) detailed that these high-altitude clouds, composed of carbon dioxide ice, were seen floating between 60 and 80 kilometres above the surface. The cold temperatures at these heights cause the condensation of carbon dioxide, forming distinctive cloud structures. Some of the ice crystals were observed descending before evaporating at approximately 50 kilometres, where temperatures begin to rise.

As reported by space.com,that this is the fourth Martian year in which Curiosity has recorded these cloud formations. The phenomenon was first observed by NASA’s Pathfinder mission in 1997, which captured images from a location just north of the Martian equator.

Expert Analysis on Martian Clouds

In a statement to NASA’s JPL, Mark Lemmon, Atmospheric Scientist at the Space Science Institute in Colorado, remarked that the first sighting of these iridescent clouds was initially thought to be a colour anomaly. He highlighted that their seasonal recurrence has allowed researchers to predict their appearance and plan observations in advance.

Last year, scientists produced the most comprehensive cloud map of Mars, compiled from two decades of data gathered by the European Space Agency’s Mars Express orbiter. This study classified a range of cloud formations, including patterns not seen on Earth. Daniela Tirsch, Planetary Geologist at the German Aerospace Center, commented at the time that Martian clouds exhibit significant diversity.

Unanswered Questions About Cloud Formation

Observations have so far been limited to specific regions, with no twilight clouds detected by the Perseverance rover, which landed in Jezero Crater in 2021. This has led scientists to question what makes certain areas more conducive to their formation.

Lemmon explained that carbon dioxide was not expected to condense into ice at these altitudes, suggesting an unknown cooling mechanism at work. He pointed to atmospheric gravity waves as a possible factor, though their role in Martian weather patterns remains uncertain. Further studies are planned to better understand these cloud formations and their implications for the planet’s climate.

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Astronomers Discover Most Powerful Cosmic Explosions Since the Big Bang

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Astronomers Discover Most Powerful Cosmic Explosions Since the Big Bang

Astronomers have seen the most energetic cosmic explosions yet, a new class of eruptions termed “extreme nuclear transients” (ENTs). These rare events occur when stars at least three times more massive than our Sun are shredded by supermassive black holes. While such cataclysmic events have been known for years, recent flares detected in galactic centres revealed a brightness nearly ten times greater than typical tidal disruption events. The discovery offers new insight into black hole behaviour and energy release in the universe’s most extreme environments.

Extreme Flares Detected by Gaia and ZTF Reveal Most Energetic Black Hole Events Yet

As per a June 4 Science Advances report, lead researcher Jason Hinkle of the University of Hawaii’s Institute for Astronomy noticed two mysterious flares from galactic cores in 2016 and 2018, recorded by the European Space Agency‘s Gaia spacecraft. The scientists recognised them as ENTs because a third one, observed in 2020 by the Zwicky Transient Facility, has similar characteristics. These outbursts gave out more energy than supernovae did, and they lasted much longer than short bursts typically seen during tidal disruption events.

Tidal disruption events such as Gaia18cdj are associated with flares that are explosive and long-duration. These explosions are greater than 100 times as intense as supernovas and have been occurring for millions to billions of years. They make ENTs an uncommon, energetic, and long-lived event that cosmic explorers might use.

The ENTs’ brightness lets astronomers focus on distant galactic centres, as well as the feeding habits of black holes in the universe’s early days. “These flares are shining a light on the growth of supermassive black holes in the universe,” mentioned co-author Benjamin Shappee, a Hubble fellow at IfA. Their visibility on large scales provides a statistical tool for cosmological studies in the future.

Such findings are expanding what astrophysicists know about ENTs-but researchers stress that they’re not done wrapping their heads around these mysterious objects just yet. The results might also advance new models of how black holes and stars work together and how energy moves across galaxies. Given upcoming missions with better instruments, the discovery of more ENTs will help astronomers learn even more about these violent events in the cosmos.

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NASA’s IMAP Mission to Chart Solar System Boundary, Launching in 2025

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NASA’s IMAP Mission to Chart Solar System Boundary, Launching in 2025

NASA’s Interstellar Mapping and Acceleration Probe (IMAP) has started to get ready for the launch. It was removed from its shipping container on Thursday, May 29, after being transferred from the airlock into the high bay at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida. Its objective is to study the boundary of the solar system and how solar wind interacts with interstellar space. The mission is targeting launch no earlier than September 2025 from Launch Complex 39A.

About the new Mission

According to NASA’s blog, the IMAP mission will orbit the Sun at a location called Lagrange Point 1 (L1), which is about one million miles from Earth towards the Sun. From this location, IMAP can measure the local solar wind and scan the distant heliosphere without background from planets and their magnetic fields. The spacecraft will use 10 scientific instruments to study and map the heliosphere, a vast magnetic bubble surrounding the Sun that protects our solar system. As a modern-day space cartographer, IMAP will enhance our understanding of heliophysics and contribute valuable insights into space weather prediction.

At NASA’s Marshall Space Flight Center, IMAP went through thermal vacuum testing at the X-ray and Cryogenic facility that simulates harsh conditions and dramatic temperature changes to simulate the environment during launch, on the journey toward the Sun.

Pre-Launch Preparations

NASA technicians will now begin to load the IMAP spacecraft with propellant. It will be integrated with two additional satellites: the Carruthers Geocorona Observatory and NOAA’s Space Weather Follow On L1. All three spacecraft will be encapsulated together inside the protective payload fairing. Technicians then will transport the encapsulated spacecraft to a hangar at NASA Kennedy, where the team will integrate the spacecraft with its SpaceX Falcon 9 rocket.

IMAP is the fifth mission in NASA’s Solar Terrestrial Probes program portfolio. It is led by Princeton University professor David J. McComas with an international team of 25 partner institutions. The spacecraft was built and operated from The Johns Hopkins Applied Physics Laboratory.

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Rocket Lab Launches Private Earth-Observing Satellite Toward Orbit for BlackSky

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Rocket Lab Launches Private Earth-Observing Satellite Toward Orbit for BlackSky

Rocket Lab successfully launched a Gen-3 Earth-observing satellite for Virginia-based BlackSky on June 2, marking another step in private-sector space imaging. The mission, named Full Stream Ahead, lifted off aboard an Electron rocket from the company’s New Zealand launch complex at 7:57 p.m. EDT (11:57 a.m. NZST on June 3). The satellite is headed for a circular orbit 292 miles (470 kilometres) above Earth. Once in position, the satellite will bolster BlackSky’s constellation, which provides high-resolution images and AI-powered analytics for real-time Earth intelligence operations.

Rocket Lab Expands Role in Commercial Space With 65th Electron Launch and Growing Fleet

According to Rocket Lab, this was the second of four scheduled Electron launches for BlackSky in 2025 and the 10th overall Electron flight for the company, making it the most frequently used launcher in BlackSky’s deployment campaign. The Electron rocket’s successful liftoff also marks the seventh mission for Rocket Lab this year and the 65th total flight. The mission contributes to the increasing importance of tiny launchers in low Earth orbit servicing of commercial satellite clients.

Designed particularly for specialist small satellite launches, the 59-foot (18-metre) Electron spacecraft has become a pillar in the commercial space sector. The Gen-3 satellite it carries will improve BlackSky’s capacity to provide fast geospatial insights, which are in demand in the humanitarian, commercial, and military spheres.

The launch also highlights Rocket Lab’s broader ambitions. The company is testing a suborbital Electron variant known as HASTE, designed for hypersonic vehicle testing, and is concurrently developing a much larger rocket, Neutron. Anticipated to launch later this year, Neutron targets medium-lift missions, including possible human-rated flights in the future, and seeks to be partly reusable.

With back-to-back missions and expanding vehicle capability, Rocket Lab continues to position itself as a key player in the evolving private spaceflight industry.

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