Connect with us

Published

on

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


(This story has not been edited by NDTV staff and is auto-generated from a syndicated feed.)

Affiliate links may be automatically generated – see our ethics statement for details.

Continue Reading

Science

NASA Hubble Space Telescope Helps Confirm the First Solitary Black Hole

Published

on

By

NASA Hubble Space Telescope Helps Confirm the First Solitary Black Hole

For the first time, the existence of a lone black hole has been confirmed by scientists. This black hole has no star orbiting it. According to the statement by Kailash Sahu, astronomer at the Space Telescope Science Institute in Baltimore, “it’s the only one so far”. The discovery made headlines in the year 2022, when Sahu and his Team claimed a dark object was moving through the constellation Sagittarius. However, another team of researchers disputed the claims by identifying the object as a neutron star.

About the Discovery

This discovery came into the light three years ago. All the stellar-mass black holes are accompanied by stars that betray their presence and race around an invisible star, along with three times the sun’s mass. Such a procedure indicates the presence of black holes rather than a neutron star.

On the contrary, the solitary black holes are expected to be common, but are very hard to find. Likewise, the one in Sagittarius was identified while passing through the dim background star and additionally shifting its position due to the black hole’s gravity. Recently, Sahu’s efforts were reported in the Astrophysical Journal, about the new observations from NASA’s Hubble Space Telescope, confirming the presence of a lone black hole in Sagittarious.

Black Hole Key Findings

Although the passage occurred first in the year 2011, the original discovery relied on the Hubble measurements from the year 2011 to 2017. However, the new data has been gained from the Hubble observations from the year 2021 to 2022, accompanied by the data received from the Gaia Spacecraft.

How Big is a Black Hole?

The ideal size of this lone black home is seven times as huge as the sun. In recent observations, a different team of scientists revisited the project and identified the size as massive as six times that of the sun. The theories of the scientists match with that of Sahu’s observation.

The research continues for detecting the black holes in Sagittarius. Located at a distance of 5,000 light years away from Earth, this solitary black hole is yet to be observed from different aspects. The astronomer, Sahu, hopes to find more lone black holes with the effective use of the Nancy Grace Roman Space Telescope, which is set to launch in the year 2027.

Continue Reading

Science

Mars’ Carbonate Mystery and Ancient Atmosphere Deciphered

Published

on

By

Mars’ Carbonate Mystery and Ancient Atmosphere Deciphered

The evolution of Mars and its ancient atmosphere has been a prominent research topic for scientists. NASA’s Curiosity Mars rover could potentially be the ultimate solution for the temperature and other details about the planet. As per the assumptions made by the researchers, Mars’s atmosphere was crafted with a thick layer of carbon dioxide whereas the surface comprised liquid water. Likewise, the presence of carbonate minerals on the planet would be the result of a potential reaction between water, carbon dioxide, and Martian rocks, researchers say.

Presence of Siderite Detected

Recently reported in the April paper of Science, the presence of siderite has been discovered within the sulfate-rich rocky layers of Mount Sharp on Mars. The discovery was made at three of Curiosity’s drill sites.

According to the lead author and Associate Professor at the University of Calgary, Canada, Benjamin Tutolo, “The discovery of abundant siderite in Gale Crater represents both a surprising and important breakthrough in our understanding of the geologic and atmospheric evolution of Mars”.

About the Drilling Process

To achieve an understanding of the chemical and mineral makeup at the surface of Mars, Curiosity drills three to four centimeters down into the subsurface. Further, the powdered rock samples are then dropped into the CheMin instrument. This instrument analyses the rocks and soil via X-ray diffraction. The CheMin instrument is driven by NASA’s Ames Research Centre in California’s Silicon Valley.

The data analysis of the discovery was conducted by scientists at the Astromaterials Research and Exploration Science (ARES) Division at NASA Johnson Space Center in Houston.

Potential Findings and Atmosphere at Mars

The discovery of this carbonate mineral could potentially be hiding other minerals beneath the surface, in near-infrared satellite analysis. The possible presence of carbonates in sulfate-rich layers across Mars may result in the amount of carbon dioxide, which will be ideal to support the liquid water and create conditions warm enough to sustain water. Also, the scientists doubt the existence of other carbonates, or maybe they might have vanished from space.

To Conclude

The missions and analyses are still undergoing, and they will continue the research in the future. The findings can be confirmed post-research on the sulfate-rice area on the red planet. As the findings arrive, they will help us understand the transformation of the planet and will offer clarity on the ancient atmosphere.

Note: Curiosity is a part of NASA’s Mars Exploration Program (MEP) portfolio. It was built by NASA’s Jet Propulsion Laboratory, managed by Caltech in Pasadena, California. The mission is successfully led by JPL on behalf of NASA’s Science Mission Directorate in Washington.

Continue Reading

Science

JWST Might Have Revealed New Signs of Alien Life on Nearby Exoplanet

Published

on

By

JWST Might Have Revealed New Signs of Alien Life on Nearby Exoplanet

Scientists discovered suitable biosignature gases for alien life on planet K2-18b. On K2-18b, NASA’s James Webb Space Telescope (JWST) noticed dimethyl sulfide (DMS), a chemical primarily produced by living creatures on Earth. Notably, the exoplanet is nine times the size of our planet and exists in the habitable zone of its planetary system. As exoplanets pass in front of their home stars, the team probes planetary atmospheres using JWST’s Mid-Infrared Instrument (MIRI). Based on its size and other properties, astronomers think K2-18b is a “Hycean” world—that is, one with a large liquid-water ocean and a hydrogen-rich atmosphere.

Although the researchers estimate concentrations of more than 10 parts per million by volume on Earth, they are less than one part per billion. However, further research is required to confirm and expand on their findings.

NASA’s Webb Telescope Finds Possible Life Signs on Exoplanet K2-18b

According to a new study, which was published in The Astrophysical Journal Letters, chemical proof of life on the far-off exoplanet K2-18b has come from NASA’s James Webb Space Telescope. Rare on other planets or moons, these signals, which point to the presence of dimethyl sulfide and dimethyl disulfide, are found in marine plants and bacteria on Earth.

Because K2-18b boasts a hydrogen-rich atmosphere and a planet-wide ocean, researchers classify it as a “hycean world.” Methane and carbon dioxide, found in the planet’s atmosphere in 2023, were the first carbon-based compounds found in the habitable zone of an exoplanet. Though the levels had minimal statistical significance, the researchers also found likely DMS signals, therefore confounding DMS diagnosis. The results underline the possibilities of life on exoplanets.

JWST Data Hints at High Sulfur Levels on Exoplanet, Life or Not

MIRI observations from the JWST expose features in planetary atmospheres that point to DMS or DMDS helping to explain them. Scientists estimate that atmospheric DMS and DMDS levels could be substantially greater than on Earth, that is, above 10 parts per million. Differentiating DMS from DMDS requires more data. Scientists want to investigate undiscovered chemical processes involving no living entities able to generate DMS and DMDS from nothing.

Continue Reading

Trending