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Scientists found living microbes in a 2-billion-year-old rock in South Africa, providing insights into early life on Earth and potentially aiding the search for life on Mars.

Researchers have discovered pockets of living microbes within a sealed fracture of a 2-billion-year-old rock from the Bushveld Igneous Complex in South Africa, an area known for its rich ore deposits. This is the oldest example of living microbes found within ancient rock to date.

To confirm that the microbes were indigenous to the ancient core sample and not caused by contamination during the retrieval and study process, the research team refined a technique they previously developed involving three types of imaging – infrared spectroscopy, electron microscopy, and fluorescent microscopy. These microbes could provide novel insights into the early evolution of life, and aid the search for extraterrestrial life in similarly aged rock samples brought back from Mars.

Researchers have developed a Martian atmospheric evolution model to propose a new theory about Mars’s past. Although Mars is currently a cold, dry planet, geological evidence suggests that liquid water existed there around 3 to 4 billion years ago. Where there is water, there is usually life. In their quest to answer the burning question about life on Mars, researchers at Tohoku University created a detailed model of organic matter production in the ancient Martian atmosphere.

Organic matter refers to the remains of living things such as plants and animals, or the byproduct of certain chemical reactions.

Whatever the case, the stable carbon isotope ratio (13C/12C) found in organic matter provides valuable clues about how these building blocks of life were originally formed, giving scientists a window into the past.

We often contemplate cyborgs, people enhanced by machines, but what would a civilization built upon cybernetics be like?

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In a new study, astronomers report novel evidence regarding the limits of planet formation, finding that after a certain point, planets larger than Earth have difficulty forming near low-metallicity stars.

Using the sun as a baseline, astronomers can measure when a star formed by determining its metallicity, or the level of heavy elements present within it. Metal-rich stars or nebulas formed relatively recently, while metal-poor objects were likely present during the early universe.

Previous studies found a weak connection between metallicity rates and planet formation, noting that as a star’s metallicity goes down, so, too, does planet formation for certain planet populations, like sub-Saturns or sub-Neptunes.

We may be looking for Martian life in the wrong places. The Viking life detection experiments might have inadvertently killed indigenous Martian life by applying too much water. Instead we should “follow the salt” to find life on Mars! See my blog on BigThink (with link to Nature Astronomy paper), Weblink through my webpage:


Posted on Big Think.

The Sun emitted a strong solar flare, peaking at 6:20 p.m. ET on Oct. 1, 2024. NASA’s Solar Dynamics Observatory, which watches the Sun constantly, captured an image of the event.

Solar flares are powerful bursts of energy. Flares and solar eruptions can impact radio communications, electric power grids, navigation signals, and pose risks to spacecraft and astronauts.

This flare is classified as an X7.1 flare. X-class denotes the most intense flares, while the number provides more information about its strength.