Copernical Team
NASA Embarks on a New Lunar Science Era with Artemis III Mission Instruments
NASA has announced the selection of three pioneering scientific instruments for the Artemis III mission, marking a significant step towards advancing lunar exploration and research. These instruments, set for deployment by astronauts on the Moon's South Pole, aim to shed light on the lunar environment, the Moon's interior structures, and strategies for sustaining long-term human presence on the Eutelsat and Sat One Launch Satellite Services in Australasia for Enhanced Connectivity
Eutelsat, in collaboration with Sat One, has commenced the delivery of satellite-based services to remote and maritime regions in Australia and New Zealand, marking a significant step towards improved connectivity in these areas. This initiative leverages the capabilities of the OneWeb Low Earth Orbit (LEO) satellite constellation, enabling high-speed, low-latency communication solutions for a v ESA's SMOS and Swarm Satellites Uncover the Magnitude of a Solar Storm's Impact on Earth
Over the recent weekend, a significant celestial event unfolded as the Sun unleashed an extraordinary amount of electromagnetic radiation towards Earth. This solar activity not only produced the awe-inspiring aurora borealis, lighting up the night sky in a dazzling display of colors but also brought to the forefront the capabilities of the European Space Agency's (ESA) two unassuming satellites: Berkeley to Spearhead $300M UV Mapping Mission
NASA's decision to launch an ambitious space telescope mission in 2030, with a budget of $300 million, marks a significant leap in our understanding of the ultraviolet universe. The mission, named UVEX (UltraViolet EXplorer), will be the first to perform a comprehensive survey of the ultraviolet (UV) sky, offering new insights into the evolution of galaxies and stars over time.
Managed by Astronomers Uncover the Legacy of a 12th Century Supernova with Multi-Telescope Observations
In 1181, observers from different parts of the world were captivated by the appearance of a new 'star' in the constellation Cassiopeia, an event now identified as a rare supernova explosion. Visible for 185 days, this supernova shone with the brightness of Saturn, embedding itself in historical records.
The search for the remnants of this celestial phenomenon has puzzled astronomers for ce Ariane 6's Maiden Voyage Marks a New Era for European Space Missions with YPSat Onboard
Europe's newest rocket soon launches, taking with it many space missions each with a unique objective, destination and team at home, cheering them on. Whether launching new satellites to look back and study Earth, peer out to deep space or test important new technologies in orbit, Ariane 6's first flight will showcase the versatility and flexibility of this impressive, heavy-lift launcher. ESA and NASA team up to study solar wind
In the run up to April’s total solar eclipse, ESA-led Solar Orbiter and NASA-led Parker Solar Probe are both at their closest approach to the Sun. Tomorrow, they are taking the opportunity to join hands in studying the driving rain of plasma that streams from the Sun, fills the Solar System, and causes dazzlement and destruction at Earth.
Japan moon probe survives second lunar night
Japan's moon lander woke up after unexpectedly surviving a second frigid, two-week lunar night and transmitted new images back to Earth, the country's space agency said Thursday.
The unmanned Smart Lander for Investigating Moon (SLIM) probe touched down in January, making Japan only the fifth nation to reach the lunar surface without crashing.
But the lightweight spacecraft landed at a wonky angle that left its solar panels facing the wrong way.
The Japan Aerospace Exploration Agency announced the probe's latest surprise awakening in a post on X, formerly Twitter.
"We received a response from SLIM last night and confirmed that SLIM had successfully completed its second overnight," it said.
A black-and-white photo of the rocky surface of a crater accompanied the post on SLIM's official account.
Schools in the path of April's total solar eclipse prepare for a natural teaching moment
Seventh-grade student Henry Cohen bounced side to side in time to the Beatles' "Here Comes the Sun" playing in teacher Nancy Morris' classroom, swinging his arms open and closed across the planets pictured on his T-shirt.
Henry and other classmates at Cleveland's Riverside School were on their feet, dancing during a session of activities tied to April's total solar eclipse. Second-graders invited in for the lessons sat cross-legged on the floor, laughing as they modeled newly decorated eclipse viewing glasses. Dioramas with softball-sized model earths and moons and flashlight "suns" occupied desks and shelves around the room.
Henry said his shirt reflected his love of space, which he called "a cool mystery." The eclipse, he said, "is a one in a million chance and I'm glad I get to be here for it."
For schools in or near the path of totality of the April 8 eclipse, the event has inspired lessons in science, literacy and culture. Some schools also are organizing group viewings for students to experience the awe of daytime darkness and learn about the astronomy behind it together.
Imaging turbulence within solar transients for the first time
The Wide-field Imager for Parker Solar Probe (WISPR) Science Team, led by the U.S. Naval Research Laboratory (NRL), captured the development of turbulence as a Coronal Mass Ejection (CME) interacted with the ambient solar wind in the circumsolar space. This discovery is reported in the Astrophysical Journal.
Taking advantage of its unique location inside the sun's atmosphere, the NRL-built WISPR telescope on NASA's Parker Solar Probe (PSP) mission, operated by the Johns Hopkins University Applied Physics Laboratory (JHUAPL), captured in unparalleled detail the interaction between a CME and the background ambient solar wind.
To the surprise of the WISPR team, images from one of the telescopes showed what seemed like turbulent eddies, so-called Kelvin-Helmholtz instabilities (KHI). Such structures have been imaged in the terrestrial atmosphere as trains of crescent wave-like clouds and are the results of strong wind shear between the upper and lower levels of the cloud.