The Combination of Oxygen and Methane Could Reveal the Presence of Life on Another World

Artist’s impression of a Super-Earth orbiting a Sun-like star. Credit: ESO

In searching for life in the Universe, a field known as astrobiology, scientists rely on Earth as a template for biological and evolutionary processes. This includes searching for Earth analogs, rocky planets that orbit within their parent star’s habitable zone (HZ) and have atmospheres composed of nitrogen, oxygen, and carbon dioxide. However, Earth’s atmosphere has evolved considerably over time from a toxic plume of nitrogen, carbon dioxide, and traces of volcanic gas. Over time, the emergence of photosynthetic organisms caused a transition, leading to the atmosphere we see today.

The last 500 million years, known as the Phanerozoic Eon, have been particularly significant for the evolution of Earth’s atmosphere and terrestrial species. This period saw a significant rise in oxygen content and the emergence of animals, dinosaurs, and embryophyta (land plants). Unfortunately, the resulting transmission spectra are missing in our search for signs of life in exoplanet atmospheres. To address this gap, a team of Cornell researchers created a simulation of the atmosphere during the Phanerozoic Eon, which could have significant implications in the search for life on extrasolar planets.

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An Exoplanet so Hot it has Clouds Made of Quartz

Artist illustration showing what WASP-17 b could look like based on data obtained from a myriad of ground- and space-based telescopes, including NASA’s Hubble, Webb, and the retired Spitzer space telescopes. This most recent study used MIRI (Webb’s Mid-Infrared Instrument) to identify nanocrystals of quartz within the clouds WASP-17 b. (Credit: NASA, ESA, CSA, and R. Crawford (STScI))

A recent study published in The Astrophysical Journal Letters used data obtained by the James Webb Space Telescope’s (JWST) Mid-Infrared Instrument (MIRI) to identify the presence of quartz nanocrystals in the upper atmosphere of WASP-17 b, an exoplanet whose mass and radius are approximately 0.78 and 1.87 that of Jupiter, respectively, and is located approximately 1,324 light-years from Earth. WASP-17 b is classified as a “puffy” hot Jupiter due to its 3.7-day orbital period, meaning the extreme temperatures could cause unique chemical processes to occur within its atmosphere, but the astronomers were still surprised by the findings.

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Spaceflight is Polluting the Atmosphere with Metal

NASA’s Space Launch System rocket carrying the Orion spacecraft launches on the Artemis I flight test, Wednesday, Nov. 16, 2022. Credit: NASA/Joel Kowsky

Humans can’t seem to interact with the environment at all without fouling it in some way. From plastic bags in the ocean’s deepest regions to soot on Himalayan glaciers, our waste is finding its way into Earth’s most difficult-to-reach places.

Now, we can add metals in the stratosphere to this ignominious list.

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A Hypervelocity Experiment Mimics the Surface Conditions of Ceres

Dwarf planet Ceres is the largest object in the asteroid belt between Mars and Jupiter. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA, taken by Dawn Framing Camera
Dwarf planet Ceres is the largest object in the asteroid belt between Mars and Jupiter. NASA's Dawn mission found complex organic molecules on Ceres. Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA, taken by Dawn Framing Camera

It might be oxymoronic to say that the more we find out about something, the more mysterious it becomes. But if that’s true of anything in our Solar System, it might be true about Ceres, the largest body in the main asteroid belt.

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A Machine Learning Algorithm Finds its First Supernova

Plenty of recent mainstream news articles have touted AI’s ability to assist in the process of scientific discovery. But most of them predicted that it could take years or even decades to see the full effect. Astronomy seems ahead of the curve, though, with the announcement of a new AI system developed by researchers at Northwestern University and elsewhere that can now autonomously detect and classify supernovae.

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Comet Encke and the Halloween Fireballs of 2023

Encke
Comet Encke (left) versus the Tadpoles (NGC 1893) on August 24th, 2023. Image credit: Dan Bartlett.

Will Comet 2/P Encke and the Taurid meteors ‘trick’ or ‘treat’ observers this year?

October and November are always great months to watch for meteors, and 2023 is no exception. This year provides a special reason to be vigilant, as the source of the infamous November Taurid Fireballs Comet 2P Encke reaches perihelion for 2023 on October 22nd, at 0.34 Astronomical Units (AU) from the Sun.

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Can We Find the Heaviest Elements in Asteroids?

Asteroids are out there, and some pose a threat to Earth. How will we react when we determine that one's coming for us? Credit: N. Bartmann (ESA/Webb), ESO/M. Kornmesser and S. Brunier, N. Risinger (skysurvey.org)

One of the reasons that asteroid mining is such a popular idea among industrialists is that they holds large quantities of heavy elements. NASA’s Psyche spacecraft just launched this week, headed for an asteroid that holds ten to thirty quintillion U.S dollars worth of rare-earth elements and other heavy metals. During our planet’s formation, the heavier of these elements tended to sink deep into the Earth, making them hard to find. But even in small asteroids, these heavy elements might be much more common and accessible. Since we rely on these rare-earth elements for our modern society, metal-rich asteroids such as Psyche are worth checking out.

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Building Roads Out of Moon Dust

This illustration shows an interlocking paved surface around a Moon base. Image Credit: ESA

Astronauts will face a host of obstacles when they visit the Moon again. There’s powerful radiation, wild temperature swings, and challenging gravity to deal with. There’s also dust and lots of it. Moondust was a hazard for the Apollo astronauts, and future lunar astronauts will have to contend with it, too.

What if they turn some of that dust into solid surfaces to drive on?

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Protostars Can Siphon Material from Far Away

The B5 complex (red and green; radio images taken with the VLA and GBT) seen within its neighborhood, embedded in dust (blue) as seen with ESA’s Herschel Space Observatory, in infrared light. Scientists studied the protostar being fed by two streamers. Credit: B. Saxton (NRAO/AUI/NSF); ESA
The Barnard 5 complex (red and green; radio images taken with the VLA and GBT) seen within its neighborhood, embedded in dust (blue) as seen with ESA’s Herschel Space Observatory, in infrared light. Scientists studied the protostar being fed by two streamers. Credit: B. Saxton (NRAO/AUI/NSF); ESA

When stars are born, they do it inside a molecular cloud. Astronomers long assumed that the “crèche” supplied all the nutrients that protostars needed to form. However, it turns out they get help from outside the nest.

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A Monster Solar Storm Struck Earth 14,300 Years Ago

Illustration of a solar flare striking Earth. Credit: NASA

The Sun is such a stable presence in our lives that we often take it for granted. Few things are as certain sure as the rising of the Sun each morning, and the cycles of the seasons mark the years of our lives. But the Sun is a star, and stars can sometimes be unpredictable. They can emit powerful solar flares and powerful X-rays. With our deep dependence on technology and electricity, the Sun poses a small but real risk to our civilization. As a recent study shows, the Sun has had some extremely powerful flares in recent cosmic times.

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