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A SpaceX rocket in Florida stood poised for launch on Saturday carrying an orbital telescope built to shed light on mysterious cosmic phenomena known as dark energy and dark matter, unseen forces scientists say account for 95 percent of the known universe.

The telescope dubbed Euclid, a European Space Agency (ESA) instrument named for the ancient Greek mathematician called the “father of geometry,” was bundled inside the cargo bay of a Falcon 9 rocket set for blast-off around 11 am EDT (1500 GMT) from Cape Canaveral Space Force Station.

New insights from the $1.4 billion (roughly Rs. 11,500 crore) mission, designed to last at least six years, are expected to transform astrophysics and perhaps understanding of the very nature of gravity itself.

If all goes as planned, Euclid will be released after a short ride to space for a month-long voyage to its destination in solar orbit nearly 1 million miles (1.6 million km) from Earth – a position of gravitational stability between the Earth and sun called the Lagrange Point Two, or L2.

From there, Euclid is designed to explore the evolution of what astrophysicists refer to as the “dark universe,” using a wide-angle telescope to survey galaxies as far away as 10 billion light years from Earth across an immense expanse of the sky beyond our own Milky Way galaxy.

The 2-ton spacecraft is also equipped with instruments designed to measure the intensity and spectrums of infrared light from those galaxies in a way that will precisely determine their distances.

The mission focuses on two foundational components of the dark universe. One is dark matter, the invisible but theoretically influential cosmic scaffolding thought to give shape and texture to the cosmos. The other is dark energy, an equally enigmatic force believed to explain why expansion of the universe, as scientists learned in the 1990s, has long been accelerating.

The possibilities of the mission are reflected by the enormity of Euclid’s inquiry. Scientists estimate dark energy and dark matter together make up 95 percent of the cosmos, while ordinary matter that we can see accounts for just 5 percent.

European-led Mission

Euclid was designed and built entirely by ESA, with the US space agency, NASA, supplying photo detectors for its near-infrared instrument. The Euclid Consortium overall comprises more than 2,000 scientists from 13 European nations, the U.S., Canada and Japan.

A decade in the making, the mission originally was to have flown to space by way of a Russian Soyuz rocket. But launch plans were switched to SpaceX, the California-based venture of Elon Musk, after war erupted in Ukraine, and because no slot was immediately available from Europe’s Arianne rocket program.

While the James Webb Space Telescope launched by NASA late last year allows astronomers to zero in on particular objects from the early universe with unprecedented clarity, Euclid is intended to expose the hidden fabric and mechanics of the cosmos by meticulously charting an enormous swath of the observable universe in 3-D, more than 1 billion galaxies in all.

Dark matter and dark energy cannot be detected directly, but their properties “are encoded in the shapes and positions of the galaxies,” said astrophysicist Jason Rhodes, lead scientist for Euclid at NASA’s Jet Propulsion Laboratory near Los Angeles.

“Measuring the shapes and positions of galaxies allows us to infer the properties of dark matter and dark energy,” Rhodes said on Friday.

The data will be collected as Euclid maps the last 10 billion years of cosmic history across a third of the sky, gazing outward, and thus back in time, to an era of the universe astronomers call “cosmic noon,” when most stars were forming.

Observing subtle but distinct changes in the shapes and positions of galaxies over vast spans of time and space will reveal fine variations in cosmic acceleration, indirectly exposing the forces of dark energy, scientists say.

Euclid also will help reveal the nature of dark matter by measuring an effect called gravitational lensing, which produces faint distortions in galaxies’ visible shapes and is attributed to the presence of unseen material warping the fabric of space around it.

Through insights into dark energy and matter, scientists hope to better grasp the formation and distribution of galaxies across the so-called cosmic web of the universe.

Beyond Euclid’s primary objectives, it will provide “a gold mine for all fields of astronomy for several decades,” said Yannick Mellier, Euclid Consortium lead and astronomer at the Institut d’Astrophysique de Paris.

© Thomson Reuters 2023


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

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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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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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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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