A Magnetohydrodynamic Drive Could Lead to Fuel Stations on Mars

Graphic depiction of Magnetohydrodynamic Drive for Hydrogen and Oxygen Production in Mars Transfer. Credit: Alvaro Romero-Calvo

Within the next fifteen years, NASA, China, and SpaceX plan to send the first crewed missions to Mars. In all three cases, these missions are meant to culminate in the creation of surface habitats that will allow for many returns and – quite possibly – permanent human settlements. This presents numerous challenges, one of the greatest of which is the need for plenty of breathable air and propellant. Both can be manufactured through electrolysis, where electromagnetic fields are applied to water (H2O) to create oxygen gas (O2) and liquid hydrogen (LH2).

While Mars has ample deposits of water ice on its surface that make this feasible, existing technological solutions fall short of the reliability and efficiency levels required for space exploration. Fortunately, a team of researchers from Georgia Tech has proposed a “Magnetohydrodynamic Drive for Hydrogen and Oxygen Production in Mars Transfer” that combines multiple functionalities into a system with no moving parts. This system could revolutionize spacecraft propulsion and was selected by NASA’s Innovative Advanced Concepts (NIAC) program for Phase I development.

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The Seeming Impossibility of Life

This is an artist's illustration showing the timeline of the early universe showing some key time periods. On the left is the early day of the Universe, where the intense heat prevented much from happening. After that is the release of the CMB once the Universe cooled a little. After that, in yellow, is the Neutral Universe, the time before stars formed. The hydrogen atoms in the Neutral Universe should have given off radio waves that we can detect here on Earth. Image Credit: ESA – C. Carreau
This is an artist's illustration showing the timeline of the early universe showing some key time periods. On the left is the early day of the Universe, where the intense heat prevented much from happening. After that is the release of the CMB once the Universe cooled a little. After that, in yellow, is the neutral Universe, the time before stars formed. The hydrogen atoms in the neutral Universe should have given off radio waves that we can detect here on Earth. Image Credit: ESA – C. Carreau

The number of near misses, false starts, and legitimate disasters that have befallen our species since the day we took our first upright steps all those generations ago is too large to count and could honestly take up this entire book. I’ll give us humans this much, though: we’re survivors, through and through.

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Water Vapor Found in the Atmosphere of a Small Exoplanet

Artist's impression of GJ 9827 d, which is the smallest exoplanet ever found to potentially possess water in its atmosphere. (Credit: NASA, ESA, Leah Hustak and Ralf Crawford (STScI))

A recent study published in The Astrophysucal Journal Letters discusses the detection of water within the atmosphere of GJ 9827 d, which is a Neptune-like exoplanet located approximately 97 light-years from Earth, using NASA’s Hubble Space Telescope (HST), and is the smallest exoplanet to date where water has been detected in its atmosphere. This study was conducted by an international team of researchers and holds the potential to identify exoplanets throughout the Milky Way Galaxy which possess water within their atmospheres, along with highlighting the most accurate methods to identify the water, as well.

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The Space-Based Gravitational Wave Observatory LISA Gets the Green Light

An artist's concept of how LISA will work to detect gravitational waves from orbit in space. Courtesy ESA.
An artist's concept of how LISA will work to detect gravitational waves from orbit in space. Courtesy ESA.

The science of studying gravitational waves just got a big boost thanks to the European Space Agency. Its science program committee just approved the Laser Interferometer Space Antenna—affectionately known as LISA—for official planning and building. That means gravitational wave astronomers will take their next steps to capture information about gravity waves from space.

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Perseverance is Definitely Inside an Ancient Lake on Mars

Aerial view of Jezero Crater on Mars
Jezero Crater on Mars. Credit: NASA/JPL-Caltech/ASU

The search for life on alien worlds has captivated us for hundreds of years. In some respect, the search for life has expanded to the search for water since it is not unreasonable to assume if there is water then there is a good chance there is life too. When NASA selected the landing site for Perseverance, they were looking for such a body of water and settled upon the Jezero Crater. Images from orbiters reveal a crater that looks like it has been filled with water in the past but further investigations were needed to confirm. Now it seems, Perseverance has risen to the challenge. 

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Japan’s SLIM Lander Finds Power Even Though It’s Face Down

Photo of the SLIM lander on the surface of the Moon - showing it tipped onto its side.
Photo of SLIM Lander

The Moon is a bit of a hot bed for exploration of late.  The Japanese agency JAXA have been getting in on the act but their SLIM lander fell on its side with its solar panels pointing toward the ground. Until today, JAXA thought that was it but today it seems that they have managed to re-established contact again.

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This is How Astronauts Would Escape from the Artemis II Launch Pad

KSC Emergency Escape Baskets

Space exploration is a tricky and at times, dangerous business. The safety of the crews is of paramount importance and escape technology is always factored into spacecraft design. Whilst Artemis I did not require such provisions when it launched Artemis II with astronauts on board is being prepared with a ski-lift style escape system to take them far away from the launch pad. 

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Did We Find Exomoons or Not? The Question Lingers.

Does Kepler-1708b have an exomoon? Scientists disagree. Image Credit: NASA

Do exoplanets have exomoons? It would be extraordinary if they didn’t, but as with all things, we don’t know until we know. Astronomers thought they may have found exomoons several years ago around two exoplanets: Kepler-1625b and Kepler-1708b. Did they?

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Atmosphere Pressure Changes Could Explain Mars Methane

New simulations are helping inform the Curiosity rover’s ongoing sampling campaign. Credit:NASA/JPL-Caltech/MSSS

One ongoing mystery on Mars is the sporadic detection of atmospheric methane. Since 1999 detections have been made by Earth-based observatories, orbital missions, and on the surface by the Curiosity Rover. However, other missions and observatories have not detected methane at all, and even when detected, the abundances appear to fluctuate seasonally or even daily.

So, where does this intermittent methane come from? A group of scientists have proposed an interesting theory: the methane is being sucked out of the ground by changes in pressure in the Martian atmosphere. The researchers simulated how methane moves underground on Mars through networks of underground fractures and found that seasonal changes can force the methane onto the surface for a short time.

In their paper, published in the Journal of Geophysical Research: Planets, the scientists say their simulations predict short-lived methane pulses prior to sunrise for Mars’ upcoming northern summer period, which is a candidate time frame for Curiosity’s next atmospheric sampling campaign.

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Another Explanation for K2-18b? A Gas-Rich Mini-Neptune with No Habitable Surface

Artist depiction of the mini-Neptune K2-18 b. Credit: NASA, CSA, ESA, J. Olmstead (STScI), N. Madhusudhan (Cambridge University)

Exoplanet K2-18b is garnering a lot of attention. James Webb Space Telescope spectroscopy shows it has carbon and methane in its atmosphere. Those results, along with other observations, suggest the planet could be a long-hypothesized ‘Hycean World.’ But new research counters that.

Instead, the planet could be a gaseous mini-Neptune.

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