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.

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.

NASA’s Jet Propulsion Laboratory, commercial companies, and academic institutions together are developing the first space-based quantum sensors for gravitational measurement. Two groups of very cold rubidium atoms will be used as weights for the Quantum Gravity Gradiometer Pathfinder (QGGPf) instrument, ensuring accurate measurements over long periods. Measuring gravity with a volume of 0.3 cubic yards (0.25 cubic meters) and weighing just over 275 pounds (125 kg), the instrument will be smaller and lighter than conventional space-based gravity instruments.

Quantum sensors offer enormous promise for sensitivity; estimates suggest they could be as much as ten times more sensitive in tracking gravity than conventional sensors. Approved to begin at the end of the decade, the technology validation project aims to test novel atomic-scale atomic manipulation of interactions between light and matter. To progress the sensor head technology and the laser optical system, NASA is working with small companies. The QGGPf instrument could lead to planetary science and fundamental physics applications.

NASA’s Quantum Gravity Sensor to Reveal Earth’s Subsurface

According to a NASA post, the Jet Propulsion Laboratory, private companies, and academic institutions are developing the first space-based quantum sensor for measuring gravity. This mission, supported by NASA’s Earth Science Technology Office (ESTO), will pave the way for groundbreaking observations of everything from petroleum reserves to global supplies of fresh water. Its gravitational field is dynamic and changing every day as geologic processes distribute mass throughout its surface. Sensitive instruments called gravity gradiometers can map the subtleties of Earth’s gravitational field and link them to belowground structures such as mineral deposits and aquifers.

The Quantum Gravity Gradiometer Pathfinder (QGGPf) instrument will use two clouds of ultracold rubidium atoms as test masses. The difference in acceleration between these matter waves will measure the difference in acceleration between these matter waves to locate gravitational anomalies. This system allows for space-based gravity measurements to remain accurate over long periods and is smaller and lighter than traditional space-based gravity instruments.

NASA Tests Atomic-Scale Tech to Advance Space Sensors and Earth Science

The main purpose of this technology validation mission is to test a collection of novel technologies for manipulating interactions between light and matter at the atomic scale. With JPL partnering with AOSense and Infleqtion to enhance sensor head technology and NASA’s Goddard Space Flight Center working with Vector Atomic to advance the laser optical system, the project involves notable partnerships between NASA and a few quantum-focused entrepreneurs.

Ultimately, the findings of this Pathfinder project might increase our capacity to explore Earth, understand far-off worlds, and value the role gravity plays in creating the universe.