Compare Sand Dunes Across the Solar System, From Venus to Pluto

"Furrowed" dunes around Mars South Pole. Credit: NASA/JPL-Caltech/University of Arizona

One of the most interesting things we can learn from studying the planets and bodies of our Solar System is how much they have in common. Mars has polar ice caps and features that formed in the presence of water. Venus is similar to Earth in size, mass, and composition and may have once been covered in oceans. And countless icy bodies in the Solar System experience volcanism and have active plate tectonics, except with ice and water instead of hot silicate magma. Another thing they have in common, which may surprise you, is sand dunes!

According to a new study by researchers from Monash University and the University of Pennsylvania, multiple planets in our Solar System have sand dunes on their surfaces – just in different forms! These features further indicate that the mechanisms for dune formation are ubiquitous throughout the Solar System. These findings could lead to new methods for assessing the surface conditions of planets and moons and could have significant implications for future robotic and crewed missions to study them up-close.

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The Dream of Faster-than-Light (FTL) Travel: Dr. Harold “Sonny” White and Limitless Space

Ever since astronomers found that Earth and the Solar System are not unique in the cosmos, humanity has dreamed of the day when we might explore nearby stars and settle extrasolar planets. Unfortunately, the laws of physics impose strict limitations on how fast things can travel in our Universe, otherwise known as Einstein’s General Theory of Relativity. Per this theory, the speed of light is constant and absolute, and objects approaching it will experience an increase in their inertial mass (thereby requiring more mass to accelerate further).

While no object can ever reach or exceed the speed of light, there may be a loophole that allows for Faster-Than-Light (FTL) travel. It’s known as the Alcubierre Warp Metric, which describes a warp field that contracts spacetime in front of a spacecraft and expands it behind. This would allow the spacecraft to effectively travel faster than the speed of light while not violating Relativity or causality. For more than a decade, Dr. Harold “Sonny” White has been investigating this theory in the hopes of bringing it closer to reality.

Previously, Dr. White pursued the development of an Alcubierre Warp Drive with his colleagues at the Advanced Propulsion Physics Research Laboratory (NASA Eagleworks) at NASA’s Johnson Space Center. In 2020, he began working with engineers and scientists at the Limitless Space Institute, a non-profit organization dedicated to education, outreach, research grants, and the development of advanced propulsion methods – which they hope will culminate in the creation of the first warp drive!

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A new Quantum Technique Could Enable Telescopes the Size of Planet Earth

These annotated images, obtained with the GRAVITY instrument on ESO’s Very Large Telescope Interferometer (VLTI) between March and July 2021, show stars orbiting very close to Sgr A*, the supermassive black hole at the heart of the Milky Way. One of these stars, named S29, was observed as it was making its closest approach to the black hole at 13 billion kilometres, just 90 times the distance between the Sun and Earth. Another star, named S300, was detected for the first time in the new VLTI observations. To obtain the new images, the astronomers used a machine-learning technique, called Information Field Theory. They made a model of how the real sources may look, simulated how GRAVITY would see them, and compared this simulation with GRAVITY observations. This allowed them to find and track stars around Sagittarius A* with unparalleled depth and accuracy.

There’s a revolution underway in astronomy. In fact, you might say there are several. In the past ten years, exoplanet studies have advanced considerably, gravitational wave astronomy has emerged as a new field, and the first images of supermassive black holes (SMBHs) have been captured. A related field, interferometry, has also advanced incredibly thanks to highly-sensitive instruments and the ability to share and combine data from observatories worldwide. In particular, the science of very-long baseline interferometry (VLBI) is opening entirely new realms of possibility.

According to a recent study by researchers from Australia and Singapore, a new quantum technique could enhance optical VLBI. It’s known as Stimulated Raman Adiabatic Passage (STIRAP), which – in combination with pre-distributed entanglement – allows quantum information to be transferred without losses. When imprinted into a quantum error correction code, this technique could allow for VLBI observations into previously inaccessible wavelengths. Once integrated with next-generation instruments, this technique could allow for more detailed studies of black holes, exoplanets, the Solar System, and the surfaces of distant stars.

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Starliner Launches Successfully, but Two of its Thrusters Failed

An uncrewed Boeing CST-100 Starliner approaches the International Space Station above the south Pacific on May 20, 2022. Credit: NASA

Last week, Boeing’s next-generation CST-100 Starliner took off from Space Launch Complex 41 at Cape Canaveral, reached orbit, and docked with the International Space Station (ISS). Designated Orbital Flight Test-2 (OFT-2), this uncrewed test flight successfully validated the reusable space capsule for NASA’s Commercial Crew Program (CCP). This program, a public-private partnership between NASA and commercial launch providers (SpaceX and Boeing), aims to provide safe, reliable, and cost-effective payload and crew transportation to the ISS from American soil.

The mission came with its share of hiccups, which consisted of two of the spacecraft’s thrusters shutting off prematurely during orbital maneuvers. Nevertheless, this successful test flight was a welcome relief after three years of delays, checks, and corrective actions that followed the first failed attempt (OFT-1). After six days of being docked with the ISS, the spacecraft is scheduled to undock tomorrow autonomously (Wednesday, May 25th) and land at the White Sands Space Harbor at the U.S. Army’s White Sands Missile Range (WSMR) in New Mexico.

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The Closeby Habitable Exoplanet Survey (CHES) Could Detect Exoplanets Within a few Dozen Light-Years of Earth Using Astrometry

Artist's concept of Earth-like exoplanets, which (according to new research) need to strike the careful balance between water and landmass. Credit: NASA

As of this article’s writing, NASA has indicated that 5,030 extrasolar planets have been confirmed in 3,772 systems, with another 8,974 candidates awaiting confirmation. With next-generation instruments like the James Webb Space Telescope (JWST) coming online, the number and diversity of confirmed exoplanets are expected to grow exponentially. In particular, astronomers anticipate that the number of known terrestrial planets and Super-Earths will drastically increase.

In the coming years, the opportunities for exoplanet studies will increase considerably as thousands more are discovered using various methods. In a recent study, a team led by the Chinese Academy of Sciences (CAS) described a new space-telescope concept known as the Closeby Habitable Exoplanet Survey (CHES). This proposed observatory will search for Earth-like planets in the habitable zones (HZs) of Sun-like stars within approximately 33 light-years (10 parsecs) using a method known as micro-arcsecond relative astrometry.

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Dust Storms on Mars Happen When the Planet Can’t Release its Heat Fast Enough

June 2018 Mars dust storm taken from NASA's Curiosity Rover standing inside Gale Crater looking out to the crater rim. Credits: NASA

Mars is well-known for its seasonal dust storms, which can sometimes grow to encompass the entire planet. In June 2018, the dust storms became so severe that they obscured most of the planet’s surface, causing NASA to lose contact with Opportunity, which eventually proved fatal to the record-breaking rover. Understanding these storms and what causes them is critical to ensuring that solar-powered robotic missions continue to operate and future crewed missions can remain safe.

Specifically, scientists are looking for seasonal changes (i.e., changes in absorbed solar energy and temperature increases) that trigger dust storms and cause them to combine and grow. In a recent study conducted by researchers from the University of Houston, they could result from seasonal energy imbalances in the amount of solar energy absorbed and released by the planet. These findings could lead to a new understanding of the Red Planet’s climate and atmosphere.

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China has a new Human Lunar Space Program, With Plans for Landers, Orbiters, Rovers, and a Lunar Base

The China National Space Agency (CNSA) has advanced considerably since the turn of the century, boasting new launch vehicles, robotic missions to the Moon and Mars, and a modular space station in orbit (Tiangong). According to various sources, they plan to advance even further in the coming years and decades. Given the tight-lipped nature of the Chinese government and its agencies, much of what we periodically hear is based on snippets of information, gossip, and speculation.

However, in a recent interview with the state-owned CCTV new network, chief designer Huang Zhen confirmed that China’s space agency has established the Crewed Lunar Program Office. This program will consist of additional robotic missions to explore the Moon, followed by crewed missions and the creation of a base camp. Zhen also confirmed that he and his team at the China Association for Science and Technology (CAST) are currently developing the key technologies that will make this happen.

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Merging Supermassive Black Holes Gives us a New Way to Measure the Universe

The study of black holes has advanced immensely in the past few years. In 2015, the first gravitational waves were observed by scientists at the Laser Interferometer Gravitational-Wave Observatory (LIGO). This finding confirmed what Einstein predicted a century before with General Relativity and offered new insight into black hole mergers. In 2019, scientists with the Event Horizon Telescope (EHT) Collaboration shared the first image of a supermassive black hole (SMBH), which resides at the center of the M87 galaxy.

Earlier this month, the EHT announced that they had also acquired the first image of Sagittarius A*, the black hole at the center of the Milky Way Galaxy. And just in time for Black Hole Week (May 2nd to May 6th), a pair of researchers from Columbia University announced a new and potentially easier way to study black holes. In particular, their method could enable the study of black holes smaller than M87* in galaxies more distant than the M87 galaxy.

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Engineers Design an Electrical Microgrid for a Lunar Base

Moon base
Illustration of NASA astronauts on the lunar South Pole. Mission ideas we see today have at least some heritage from the early days of the Space Age. Credit: NASA

For seventy years, Albuquerque-based Sandia National Laboratories has been developing electrical microgrids that increase community resilience and ensure energy security. Applications include the Smart Power Infrastructure Demonstration for Energy Reliability and Security (SPIDERS), designed to support military bases abroad, and independent power systems for hospitals and regions where electrical grids are at risk of being compromised by natural disasters (like hurricanes, flooding, and earthquakes).

In the coming years, Artemis Program, NASA will be sending astronauts back to the Moon for the first time since the Apollo Era and establish a “sustained program of lunar exploration.” To ensure that astronauts have the necessary power to maintain their habitats and support operations on the surface, NASA has partnered with Sandia to develop microgrids for the Moon! This technology could also support future endeavors, like mining, fuel processing, and other activities on the Moon.

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A CubeSat is Flying to the Moon to Make Sure Lunar Gateway’s Orbit is Actually Stable

Artist rendition of the CAPSTONE mission. Credit: Advanced Space.

Before this decade is over, NASA will send astronauts to the Moon for the first time since the Apollo Era. As part of the Artemis Program, NASA also plans to establish the infrastructure that will allow for a “sustained program of lunar exploration.” A key part of this is the Lunar Gateway, an orbiting space station that will facilitate regular trips to and from the lunar surface. In addition to being a docking point for ships going to and from Earth, the station will also allow for long-duration missions to Mars.

The Gateway will have what is known in orbital mechanics as a “near rectilinear halo orbit” (NRHO), meaning it will orbit the Moon from pole to pole. To test the long-term stability of this orbit, NASA will be sending the Cislunar Autonomous Positioning System Technology Operations and Navigation Experiment (CAPSTONE) to the Moon by the end of May. This nine-month CubeSat mission will be the first spacecraft to test this orbit and demonstrate its benefits for the Gateway.

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