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A study of the Ophiuchus star-forming complex has offered new insights into the conditions in which our own solar system was born.

The findings of the study were published in the journal Nature Astronomy.

A region of active star formation in the constellation Ophiuchus is giving astronomers new insights into the conditions in which our own solar system was born.

In particular, the study showed how our solar system may have become enriched with short-lived radioactive elements.

Evidence of this enrichment process has been around since the 1970s when scientists studying certain mineral inclusions in meteorites concluded that they were pristine remnants of the infant solar system and contained the decay products of short-lived radionuclides.

These radioactive elements could have been blown onto the nascent solar system by a nearby exploding star (a supernova) or by the strong stellar winds from a type of massive star known as a Wolf-Rayet star.

The authors of the new study used multi-wavelength observations of the Ophiuchus star-forming region, including spectacular new infrared data, to reveal interactions between the clouds of star-forming gas and radionuclides produced in a nearby cluster of young stars.

Their findings indicated that supernovas in the star cluster are the most likely source of short-lived radionuclides in the star-forming clouds.

“Our solar system was most likely formed in a giant molecular cloud together with a young stellar cluster, and one or more supernova events from some massive stars in this cluster contaminated the gas which turned into the sun and its planetary system,” said co-author Douglas N. C. Lin, professor emeritus of astronomy and astrophysics at UC Santa Cruz.

“Although this scenario has been suggested in the past, the strength of this paper is to use multi-wavelength observations and a sophisticated statistical analysis to deduce a quantitative measurement of the model’s likelihood,” he added.

First author John Forbes at the Flatiron Institute’s Center for Computational Astrophysics said data from space-based gamma-ray telescopes enable the detection of gamma rays emitted by the short-lived radionuclide aluminum-26.

“These are challenging observations. We can only convincingly detect it in two star-forming regions, and the best data are from the Ophiuchus complex,” he said.

The Ophiuchus cloud complex contains many dense protostellar cores in various stages of star formation and protoplanetary disk development, representing the earliest stages in the formation of a planetary system.

By combining imaging data in wavelengths ranging from millimetres to gamma rays, the researchers were able to visualise a flow of aluminum-26 from the nearby star cluster toward the Ophiuchus star-forming region.

“The enrichment process we’re seeing in Ophiuchus is consistent with what happened during the formation of the solar system 5 billion years ago,” Forbes said.

“Once we saw this nice example of how the process might happen, we set about trying to model the nearby star cluster that produced the radionuclides we see today in gamma rays,” he added.

Forbes developed a model that accounts for every massive star that could have existed in this region, including its mass, age, and probability of exploding as a supernova, and incorporates the potential yields of aluminum-26 from stellar winds and supernovas.

The model enabled him to determine the probabilities of different scenarios for the production of the aluminum-26 observed today.

“We now have enough information to say that there is a 59 per cent chance it is due to supernovas and a 68 per cent chance that it’s from multiple sources and not just one supernova,” Forbes said.

This type of statistical analysis assigns probabilities to scenarios that astronomers have been debating for the past 50 years, Lin noted.

“This is the new direction for astronomy, to quantify the likelihood,” he added.

The new findings also showed that the amount of short-lived radionuclides incorporated into newly forming star systems can vary widely.

“Many new star systems will be born with aluminum-26 abundances in line with our solar system, but the variation is huge – several orders of magnitude,” Forbes said.

“This matters for the early evolution of planetary systems since aluminum-26 is the main early heating source. More aluminum-26 probably means drier planets,” he added.

The infrared data, which enabled the team to peer through dusty clouds into the heart of the star-forming complex, was obtained by coauthor Joao Alves at the University of Vienna as part of the European Southern Observatory’s VISION survey of nearby stellar nurseries using the VISTA telescope in Chile.

“There is nothing special about Ophiuchus as a star formation region,” Alves said.

“It is just a typical configuration of gas and young massive stars, so our results should be representative of the enrichment of short-lived radioactive elements in star and planet formation across the Milky Way,” he concluded.

The team also used data from the European Space Agency’s (ESA) Herschel Space Observatory, the ESA’s Planck satellite, and NASA’s Compton Gamma Ray Observatory.


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NASA’s Perseverance Rover Observes Googly Eye Eclipse on Mars

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NASA's Perseverance Rover Observes Googly Eye Eclipse on Mars

NASA’s Perseverance rover which is positioned in the Jezero Crater on Mars, recently observed a remarkable celestial event as the moon Phobos drifted across the Sun. Captured on September 30, this moment offered a rare glimpse into Mars’ sky, where the unique “googly eye” effect of the eclipse unfolded for the rover’s Mastcam-Z camera. The video, released by NASA, illustrates the interplay of Martian moon orbits and provides valuable information on Phobos’ trajectory and its gradual shift towards Mars.

Unexpected Eclipse Creates ‘Googly Eye’ View on Mars

Perseverance, which has been observing Mars’ surface and sky since 2021, recorded the silhouette of Phobos moving rapidly across the Sun’s face from Mars’ western Jezero Crater. Phobos, the larger of Mars’ two moons, created a distinct “googly eye” visual effect as it partially blocked sunlight, a phenomenon not typically visible from Earth. The eclipse, captured on the mission’s 1,285th sol (Martian day), highlights Phobos’ swift orbit, which takes just 7.6 hours to complete a full circle around Mars. Due to its close orbit, Phobos regularly crosses Mars’ sky, allowing for these brief transits which last only about 30 seconds each.

Phobos’ Eerie Path and Future on Mars

Phobos, named by astronomer Asaph Hall in 1877 after the Greek deity associated with fear, measures about 27 kilometres at its widest. Unlike Earth’s larger moon, Phobos appears far smaller in the Martian sky. Its orbit brings it closer to Mars with time, which scientists predict will eventually cause Phobos to collide with the Martian surface within the next 50 million years. Past eclipses of Phobos, also recorded by other Mars rovers like Curiosity and Opportunity, continue to contribute essential data for understanding Mars’ moons and their shifting orbits.

Perseverance’s Mission and Future Mars Exploration

As part of NASA’s Mars 2020 mission, Perseverance focuses on exploring Martian geology and astrobiology. The mission, managed by NASA’s Jet Propulsion Laboratory (JPL), is the first to collect samples of Mars’ surface material, which are intended to be retrieved in future joint missions with the European Space Agency (ESA). Perseverance’s Mastcam-Z, developed with support from Arizona State University, Malin Space Science Systems, and the Niels Bohr Institute, plays a crucial role in gathering high-resolution imagery to support geological studies. This mission aligns with NASA’s broader objective of preparing for human exploration on Mars, beginning with the Artemis missions to the Moon.

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South Korea teams up with NASA to send solar research tool to ISS

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South Korea teams up with NASA to send solar research tool to ISS

South Korea’s space agency announced plans on Friday to launch a solar coronagraph to the International Space Station (ISS) in a collaborative mission with NASA. Developed as part of the Coronal Diagnostic Experiment (CODEX), this instrument is set to observe and gather data on the Sun’s corona and the solar wind as well as the stream of charged particles that flows from the Sun’s outer atmosphere. The CODEX device is scheduled to be launched aboard SpaceX’s Falcon 9 from Florida’s Kennedy Space Center on Monday, as reported by Yonhap News Agency.

Bilateral Project to Examine Solar Atmosphere

The CODEX project represents a very important collaboration between the Korea Aerospace Research Institute (KASA) and NASA, with CODEX marking a pioneering achievement as the world’s first coronagraph equipped to measure temperature, velocity, and density within the solar wind. Once aboard the ISS, CODEX will be mounted on the station’s express logistics carrier, allowing for approx 55 minutes of solar observation in each 90-minute orbit around Earth. This data is expected to enhance researchers’ understanding of the solar wind, potentially aiding in space weather forecasting efforts.

South Korea’s Expanded Cooperation with NASA

Alongside the CODEX project, South Korea and the United States have broadened their partnership in space exploration. KASA and NASA signed a statement of cooperation, focusing on research initiatives including the Artemis lunar exploration programme. KASA’s involvement with the Artemis project includes studies on sustainable lunar exploration and advancements in Mars mission preparations. With this agreement, South Korea has become the fifth nation to officially collaborate with NASA on such initiatives.

Pioneering Studies and Technological Advancements

Under the framework of this agreement, South Korea and the US will work together on a variety of feasibility studies related to lunar landers, as well as advancements in communication, navigation, and astronaut support systems. In addition, collaborative efforts will span lunar surface science, autonomous power, robotic systems, and cis-lunar space operations—the area between Earth and the Moon.

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NASA’s satellite reveals fascinating tsunami data in Greenland

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NASA's satellite reveals fascinating tsunami data in Greenland

An unprecedented nine-day tsunami following a significant rockslide in Greenland’s Dickson Fjord was recently recorded by the international Surface Water and Ocean Topography (SWOT) satellite, a collaborative mission by NASA and France’s Centre National d’Études Spatiales (CNES). The event, which took place in September 2023, saw a unique pattern of seismic waves resonate around the world, marking one of the rare instances where satellite data captured a prolonged natural phenomenon with such clarity.

Satellite’s Breakthrough Detection in Remote Fjord

As per a report by NASA, the rockslide unleashed over 25 million cubic meters of rock and ice into the fjord, displacing the water and creating a massive wave that moved rhythmically between the fjord walls every 90 seconds for nine consecutive days. NASA’s Jet Propulsion Laboratory scientist Josh Willis highlighted this as a first, saying, “SWOT’s technology allowed us to see the wave contours, something we couldn’t achieve before.” The water levels on the northern side of Dickson Fjord rose as high as 1.2 metres in contrast to the southern side, emphasising the powerful impact of the rockslide.

Advanced Technology for Global Hazard Monitoring

At an altitude of around 900 kilometres, SWOT utilises a Ka-band Radar Interferometer (KaRIn) to measure surface water height with precision. This technology captured the event’s effects in the confined fjord setting, which conventional altimeters could not do due to their larger footprint. Nadya Vinogradova Shiffer, a scientist at NASA Headquarters, noted that this capability highlights SWOT’s potential for monitoring hazards, contributing to preparedness and disaster risk reduction.

Innovative Partnership in Satellite Research

Since its launch in December 2022, SWOT has been instrumental in mapping global water levels. Developed with contributions from the Canadian and UK space agencies, NASA leads the mission’s U.S. operations, including the KaRIn instrument, with CNES managing various onboard systems and support. The data collected promises ongoing contributions to scientific understanding of Earth’s water dynamics.

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