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Two organic compounds essential for living organisms have been found in samples retrieved from the asteroid Ryugu, buttressing the notion that some ingredients crucial for the advent of life arrived on Earth aboard rocks from space billions of years ago.

Scientists said on Tuesday they detected uracil and niacin in rocks obtained by the Japanese Space Agency’s Hayabusa2 spacecraft from two sites on Ryugu in 2019. Uracil is one of the chemical building blocks for RNA, a molecule carrying directions for building and operating living organisms. Niacin, also called Vitamin B3 or nicotinic acid, is vital for their metabolism.

The Ryugu samples, which looked like dark-gray rubble, were transported 155 million miles (250 million km) back to Earth and returned to our planet’s surface in a sealed capsule that landed in 2020 in Australia’s remote outback for analysis in Japan.

Scientists long have pondered about the conditions necessary for life to arise after Earth formed about 4.5 billion years ago. The new findings fit well with the hypothesis that bodies like comets, asteroids and meteorites that bombarded early Earth seeded the young planet with compounds that helped pave the way for the first microbes.

Scientists previously detected key organic molecules in carbon-rich meteorites found on Earth. But there was the question of whether these space rocks had been contaminated by exposure to the Earth’s environment after landing.

“Our key finding is that uracil and niacin, both of which are of biological significance, are indeed present in extraterrestrial environments and they may have been provided to the early Earth as a component of asteroids and meteorites. We suspect they had a role in prebiotic evolution on Earth and possibly for the emergence of first life,” said astrochemist Yasuhiro Oba of Hokkaido University in Japan, lead author of the research published in the journal Nature Communications.

“These molecules on Ryugu were recovered in a pristine extraterrestrial setting,” Oba said. “It was directly sampled on the asteroid Ryugu and returned to Earth, and finally to laboratories without any contact with terrestrial contaminants.”

RNA, short for ribonucleic acid, would not be possible without uracil. RNA, a molecule present in all living cells, is vital in coding, regulation and activity of genes. RNA has structural similarities to DNA, a molecule that carries an organism’s genetic blueprint.

Niacin is important in underpinning metabolism and can help produce the “energy” that powers living organisms.

The researchers extracted uracil, niacin and some other organic compounds in the Ryugu samples by soaking the material in hot water and then performing analyses called liquid chromatography and high-resolution mass spectrometry.

Organic astrochemist and study co-author Yoshinori Takano of the Japan Agency for Marine-Earth Science and Technology (JAMSTEC) said he is now looking forward to the results of analyses on samples being returned to Earth in September from another asteroid. The U.S. space agency NASA during its OSIRIS-REx mission collected samples in 2020 from the asteroid Bennu.

Oba said uracil and niacin were found at both landing sites on Ryugu, which is about a half-mile (900 meters) in diameter and is classified as a near-Earth asteroid. The concentrations of the compounds were higher at one of the sites than the other.

The sample from the site with the lower concentrations was derived from surface material more susceptible to degradation induced by energetic particles darting through space, Oba said. The sample from the other site was mainly derived from subsurface material more protected from degradation, Oba added.

Asteroids are rocky primordial bodies that formed in the early solar system. The researchers suggest that the organic compounds found on Ryugu may have been formed with the help of chemical reactions caused by starlight in icy materials residing in interstellar space.

© Thomson Reuters 2023

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NASA Solves Black Hole Jet X-ray Mystery with IXPE’s Polarization Powers

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May 9, 2025

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NASA Solves Black Hole Jet X-ray Mystery with IXPE’s Polarization Powers

The blazar BL Lacertae, a giant black hole with jets, facing the earth, have made scientists curious about how X-rays are generated in such extreme conditions for a while. NASA’s Imaging X-ray Polarimetry Explorer or IXPE now might have been able to solve the mystery. By a collaboration with radio and optical telescopes and using polarisation measurements of X-ray, IXPE’s produced results indicates that the interaction between fast-moving electrons and photons might be the reason for X-ray emission in such conditions.

Evidence of Compton Scattering

According to the IXPE’s findings, high optical to X-ray polarization ratio indicates that Compton scattering might be the mechanism of X-ray generation. There are two possible and competing explanations of X-ray emission in blazar jets. One saying if the X-rays in the black hole jets are highly polarised, then the X-rays are generated from interactions between photons while the other says a low polarisation indicates X-ray formation by electron-photon interaction.

Leveraging IXPE’s unique X-ray polarisation measuring ability, scientists conducted a focused observation on BL Lac in November 2023. During this period, BL Lac’s optical polarization peaked at 47.5%, the highest recorded for any blazar. Yet IXPE found the X-ray polarization to be much lower, capped at 7.6%. This contrast supports the Compton scattering and possibly irradicates the photon-based explanation.

Milestone for blazar studies

“This was one of the biggest mysteries about supermassive black hole jets,” said Iván Agudo, lead author of the study and astronomer at the Instituto de Astrofísica de Andalucía – CSIC in Spain. The discovery validates IXPE’s mission, launched in December 2021 to study X-ray polarization.

Astrophysicist Enrico Costa, called it one of IXPE’s most significant achievements. Yet, this is just the beginning. Project scientist Steven Ehlert noted the need to observe more blazars, as their emissions vary over time. With IXPE, astronomers are now better equipped to explore these powerful cosmic jets.

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SpaceX Falcon 9 Successfully Launches 28 Starlink Satellites to Orbit From Florida

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May 9, 2025

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SpaceX Falcon 9 Successfully Launches 28 Starlink Satellites to Orbit From Florida

SpaceX continued its rapid-fire Starlink deployment campaign on Tuesday night (May 6), lofting 28 more internet satellites to orbit atop a Falcon 9 rocket from Florida’s Cape Canaveral Space Force Station. The launch itself took place at 9:17 p.m. EDT (0117 GMT on May 7) from Launch Complex-40, marking the company’s 53rd Falcon 9 launch of 2025 and the 36th dedicated Starlink mission this year. The payload offers worldwide internet connectivity by adding to SpaceX’s swiftly expanding array of over 7,200 Starlink satellites in low Earth orbit.

As per a Space.com report, B1085, the reusable first-stage booster, executed a perfect main engine cut about 2.5 minutes after launch, then stage separation and a retrograde burn to stop its descent. Roughly eight minutes after launch, B1085 successfully landed on the autonomous drone ship, stationed in the Atlantic Ocean. The mission was the seventh flight for this particular booster, which had previously supported two other Starlink missions.

The Falcon 9‘s upper stage continued into orbit and deployed the 28 Starlink satellites roughly one hour after launch. These newly deployed units will spend several days adjusting their positions before integrating into the broader Starlink network, which now blankets most of the globe except the polar regions. Each satellite, compact but equipped with large solar arrays, forms part of the larger web responsible for delivering high-speed satellite internet.

The May 6 launch demonstrates how quickly SpaceX is moving to meet its broadband goals. In addition to Falcon 9 missions, the company has performed two Starship test flights this year to demonstrate development progress in both satellite launch and heavy-lift capability.

An expanding constellation would finally bring reliable internet coverage to remote locations around the world. The drive to offer a reliable internet connection to remote sites globally reflects a commitment to putting the world more in reach.

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Asteroid Vesta May Be a Fragment of a Lost Planet, Say Scientists

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May 9, 2025

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Asteroid Vesta May Be a Fragment of a Lost Planet, Say Scientists

Asteroid Vesta, long considered a stalled protoplanet, may actually be a massive fragment of a larger world that once existed in our solar system. New findings based on gravity-field mapping and spin-rate data suggest Vesta lacks the dense core typically found in differentiated planetary bodies. The discovery challenges previous assumptions, drawn from NASA’s Dawn mission in 2012, that classified Vesta as an embryonic planet. Now, scientists report that Vesta might have been ejected from a differentiated world in a massive collision 4.5 billion years ago, upending ideas about the development of planets and asteroids.

New Gravity Data Suggests Vesta Is Debris from a Destroyed Planet, Not a Protoplanet

As per a new study published in Nature Astronomy on April 23, 2025, Vesta does not quite match the former model. Refined calibration methods polished the radio Doppler signals, confirming the absence of a metal-rich core, which was inconsistent with earlier work. Seth Jacobson of Michigan State University, who led the research, stated the new interpretation marks a major shift in planetary science. While Vesta’s basaltic, volcanic surface still indicates geological activity, its internal uniformity contradicts the expectations of a body that once underwent full differentiation.

This paradox has caused scientists to reconsider the asteroid’s heritage. One scenario is that Vesta started to differentiate but never got very far. But data from meteorites called howardite-eucrite-diogenites (HEDs), thought to have come from Vesta, show no signs of such incomplete differentiation. Jacobson and his team instead favour the explanation that Vesta was formed from material blasted off a fully developed planet during an ancient planetary collision, which could also illustrate its volcanic surface without requiring it to have a dense core.

The results not only question Vesta’s identity but also suggest a possibility of a more general theory: that other asteroids could also be pieces of shattered planets. NASA’s Psyche and ESA’s Hera missions, planned for the next decades, intend to do such gravity investigations, which could ultimately confirm this new view. Jacobson noted that Vesta’s composition could even hint at a shared origin with Earth or other early planets, a hypothesis that may reshape asteroid science entirely.

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