NASA JPL Archives

October 22, 2024October 22, 2024 by Matt Williams

New Research Reveals Provides Insight into Mysterious Features on Airless Worlds

Artist's rendition of the Dawn mission on approach to the protoplanet Ceres. Credit: NASA/JPL

Between 2011 and 2018, NASA’s Dawn mission conducted extended observations of Ceres and Vesta, the largest bodies in the Main Asteroid Belt. The mission’s purpose was to address questions about the formation of the Solar System since asteroids are leftover material from the process, which began roughly 4.5 billion years ago. Ceres and Vesta were chosen because Ceres is largely composed of ice, while Vesta is largely composed of rock. During the years it orbited these bodies, Dawn revealed several interesting features on their surfaces.

This included mysterious flow features similar to those observed on other airless bodies like Jupiter’s moon Europa. In a recent study, Michael J. Poston, a researcher from the Southwest Research Institute (SWRI), recently collaborated with a team at NASA’s Jet Propulsion Laboratory to attempt to explain the presence of these features. In the paper detailing their findings, they outlined how post-impact conditions could temporarily produce liquid brines that flow along the surface, creating curved gullies and depositing debris fans along the impact craters’ walls.

October 12, 2024October 14, 2024 by Matt Williams

A Possible Exomoon Could be Volcanic, like Jupiter’s Moon Io

New NASA-led research suggests a sodium cloud seen around the exoplanet WASP-49 b might be created by a volcanic moon, which is depicted in this artist’s concept. Jupiter’s fiery moon Io produces a similar cloud. Credit: NASA/JPL-Caltech

In 2012, astronomers detected a gas giant transiting in front of WASP-49A, a G-type star located about 635 light-years from Earth. The data obtained by the WASP survey indicated that this exoplanet (WASP-49 b) is a gas giant roughly the same size as Jupiter and 37% as massive. In 2017, WASP-49 b was found to have an extensive cloud of sodium, which was confounding to scientists. Further observations in 2019 using the Hubble Space Telescope detected the presence of other minerals, including magnesium and iron, which appeared to be magnetically bound to the gas giant.

WASP-49 b and its star are predominantly composed of hydrogen and helium, with only trace amounts of sodium – not enough to account for this cloud. In addition, there was no indication of how this sodium cloud was ejected into space. In our Solar System, gas emissions from Jupiter’s volcanic moon Io create a similar phenomenon. In a recent study, an international team led by scientists from NASA’s Jet Propulsion Laboratory found potential evidence of a rocky, volcanic moon orbiting WASP-49 b. While not yet confirmed, the presence of a volcanic exomoon around this gas giant could explain the presence of this sodium cloud.

November 4, 2023November 13, 2023 by Matt Williams

Civilizations Could Use Gravitational Lenses to Transmit Power From Star to Star

A new study shows how Solar Gravitational Lenses (SGLs) could be used to beam power from one system to another.. Credit: NASA/ESA

In 1916, famed theoretical physicist Albert Einstein put the finishing touches on his Theory of General Relativity, a geometric theory for how gravity alters the curvature of spacetime. The revolutionary theory remains foundational to our models of how the Universe formed and evolved. One of the many things GR predicted was what is known as gravitational lenses, where objects with massive gravitational fields will distort and magnify light coming from more distant objects. Astronomers have used lenses to conduct deep-field observations and see farther into space.

In recent years, scientists like Claudio Maccone and Slava Turyshev have explored how using our Sun as a Solar Gravity Lens (SGL) could have tremendous applications for astronomy and the Search for Extratterstiral Intelligence (SETI). Two notable examples include studying exoplanets in extreme detail or creating an interstellar communication network (a “galactic internet”). In a recent paper, Turyshev proposes how advanced civilizations could use stellar gravitational lenses to transmit power from star to star – a possibility that could have significant implications in our search for technosignatures.

June 30, 2023July 1, 2023 by Laurence Tognetti

Psyche Mission Passes Independent Review Board with Flying Colors

Image of NASA engineers preparing the Psyche spacecraft for launch within a clean room at the Astrotech Space Operations Facility located near the NASA Kennedy Space Center. Psyche is scheduled to launch in October 2023 on a SpaceX Falcon Heavy rocket from historic Launch Complex 39A at Kennedy. (Credit: NASA/Ben Smegelsky)

An independently appointed review board recently announced that NASA, their Jet Propulsion Laboratory (JPL), and the California Institute of Technology (Caltech) have exceeded expectations in taking steps to ensure the successful launch of the metal-rich-asteroid-hunting Psyche mission this October. This comes after Psyche’s initial launch date was delayed from August 2022 due to late delivery of the spacecraft’s flight software and testing equipment, which prevented engineers from performing the necessary checkouts prior to launch.

July 30, 2021July 30, 2021 by Matt Williams

InSight has Mapped out the Interior of Mars, Revealing the Sizes of its Crust, Mantle, and Core

NASA's SEIS instrument on the Martian surface. SEIS is protected by a dome. Image Credit: NASA/JPL-Caltech

In May of 2018, NASA’s Interior Exploration using Seismic Investigations, Geodesy, and Heat Transport (InSight) landed on the Martian surface. This mission is the first of its kind, as all previous orbiters, landers, and rovers focused on studying the surface and atmosphere of Mars. In contrast, InSight was tasked with characterizing Mars’ interior structure and measuring the core, mantle, and crust by reading its seismic activity (aka. “marsquakes”).

The purpose of this is to learn more about the geological evolution of Mars since it formed 4.5 billion years ago, which will also provide insight into the formation of Earth. According to three recently published papers, the data obtained by InSight has led to new analyses on the depth and composition of Mars’ crust, mantle and confirmed the theory that the planet’s inner core is molten.

July 28, 2021July 28, 2021 by David Dickinson

Balloon Mission May Also Work to Detect Quakes on Venus

An opportunity in 2019 lays the groundwork for balloon-borne detectors on Venus, working to unravel a key mystery.

The skies of Venus may become a busy place in the coming decade, using technology field-tested here on Earth.

A team out of NASA JPL-Caltech hypothesized that terrestrial earthquakes should also produce low-frequency infrasonic sound waves, which would be transmitted from the ground through the atmosphere as changes in barometric pressure. These sound waves, while difficult to detect, should be measurable via highly sensitive barometers carried aloft.

July 26, 2021July 26, 2021 by Matt Williams

Perseverance is About to Collect the First Sample on Mars That Could Eventually be Returned to Earth

Artist's impression of the Perseverance rover on Mars. Credit: NASA-JPL

On Feb. 18^th, 2021, NASA’s Perseverance rover landed within the Jezero Crater on Mars. Like its predecessor, Curiosity, a fellow member of NASA’s Mars Exploration Program (MEP), the goal of Perseverance is to seek out evidence of possible life on Mars (past and present). A key part of this mission will be the first sample return ever performed on Mars, where samples obtained by Perseverance will be placed in a cache for later retrieval and return to Earth.

For the past five months, mission controllers at NASA have been driving the rover further from where it landed (Octavia E. Butler Landing Site) and conducting test flights with the Ingenuity helicopter. NASA is now in the midst of making final preparations for Perseverance to collect its first sample of Martian rock. This historic first is expected to begin by the end of the month or by early August and will culminate with the return of the samples to Earth by 2031.

March 26, 2021March 26, 2021 by Matt Williams

Exploring the Moon’s Shadowed Regions Using Beamed Energy

Light Bender Artist Concept. Credits: Ronald Neale

In less than three years, astronauts will return to the Moon for the first time since the Apollo Era. As part of the Artemis Program, the purpose is not only to send crewed missions back to the lunar surface to explore and collect samples. This time around, there’s also the goal of establishing vital infrastructure (like the Lunar Gateway and a Base Camp) that will allow for “sustained lunar exploration.”

A key requirement for this ambitious plan is the provision of power, which can be difficult in regions like the South Pole-Aitken Basin – a cratered region that is permanently-shadowed. To address this, a researcher from the NASA Langley Research Center named Charles Taylor has proposed a novel concept known as “Light Bender.” Using telescope optics, this system would to capture and distribute sunlight on the Moon.