#PlanetaryScience

The Perpetually Curious!theperpetuallycurious8
2026-03-12

🌍 Gravity is the quiet sculptor of worlds, shaping orbits and the weight beneath our feet. How might a 70 kg mass feel under the pull of different planets?

✍️ Explore the full story: TPC8.short.gy/Flm5GzXR

🌌 From apples to exoplanets, gravity quietly links every step we take to the wider cosmos.

SETI Institutesetiinstitute
2026-03-11

: The Italian Space Agency’s LICIACube traveled alongside NASA’s DART to capture the spacecraft’s collision with Dimorphos. In this LICIACube image, taken moments after impact on Sept. 26, 2022, rocky debris can be seen fanning out from the smaller asteroid below its larger binary partner, Didymos.

Credit: ASI/NASA

Low resolution image of the asteroid Didymos and its moonlet Dimorphos. The moonlet is shown just after the impact of the DART spacecraft, causing streams of dust and debris to eject from the small body in all directions.
Scientific Worldscientificworld
2026-03-10

Researchers may have uncovered a brand-new mineral on Mars, a discovery that could reshape planetary science and inspire future missions.

scientificworldinfo.com/2026/0

SETI Institutesetiinstitute
2026-03-10

: The Moon appears red during a total lunar eclipse over New Orleans, home of NASA’s Michoud Assembly Facility, on March 3, 2026. This “blood moon” occurs during a total lunar eclipse, as Earth lines up between the Moon and the Sun. When this happens, the only light that reaches the Moon’s surface is from the edges of Earth’s atmosphere. Credit: NASA/Michael DeMocker

Photograph of the moon during the 2026 total lunar eclipse, where the red appears red. Stars are also visible in the background.
2026-03-10

Io, lune de Jupiter, encaisse des marées gravitationnelles extrêmes. Résultat : le monde le plus volcanique du système solaire.
radiofrance.fr/franceculture/p

Fabrizio MusacchioFabMusacchio
2026-03-09

🛰️ New paper by Knowles et al.: Using the , the authors observed rapid variability in the auroral footprints of ’s in Jupiter’s .

IR observations show that the footprints of moons like can change on short timescales, highlighting the dynamic interaction between Jupiter’s and its satellites. The moon–magnetosphere coupling driving Jupiter’s is more variable than previously assumed.

📄doi.org/10.1029/2025GL118553

Figure 1: JWST/NIRSpec IFU observations of the auroral footprints of Io and Europa, indicated by yellow and purple arrows, respectively. (a) Integrated 
radiance with planetocentric latitude at 550 km above the 1-bar level (dotted) and System III (West) longitude (solid). (b) Total 
 emission with dotted gray lines for magnetic dip angle (degrees). (c) Integrated  fundamental emissions with total magnetic field strength in Gauss (blue dotted) and (d) integrated  hotband emissions with dash-dotted contours of the magnetic footprints of Io (5.9 ), Europa (9.4 ) and main auroral oval (25.0 ). UTC mid-points are given above.Figure 2:
 temperature and column density spectral retrievals. (a) 
 temperature, (b) uncertainty of the retrieved temperature, (c) 
 column density, and (d) its uncertainty.
SETI Institutesetiinstitute
2026-03-09

: JWST successfully observed the extremely faint near-Earth asteroid 2024 YR4 (circled in green) on 18 February 2026 with its Near-Infrared Camera (NIRCam). By analyzing the asteroid’s position relative to background stars whose locations are very well known, astronomers were able to rule out any chance that the asteroid could impact Earth’s Moon on 22 December 2032. Credit: NASA, ESA, CSA, STScI, M. Micheli (ESA NEOCC)

Pixelated image with four darker pixels circled in green, representing asteroid 2024 YR4 as seen by JWST in infrared.
Fabrizio MusacchioFabMusacchio
2026-03-06

🛰️ New paper by Němec et al.: After analyzing ~10 years of wave data, the authors report a -like electromagnetic signal in the . Its frequency dispersion matches theoretical propagation through ’ ionosphere and crustal magnetic fields, suggesting that electrical discharges may occur in the Martian .

🌍 doi.org/10.1126/sciadv.aeb4898

Fig. 1. Schematic showing the formation of a whistler.
A short electromagnetic pulse generated by an electric discharge (orange circle) spreads over time due to dispersion in the ionospheric plasma, where higher-frequency signals propagate faster than lower-frequency signals. These waves propagate to spacecraft altitudes (orange square) at locations where the magnetic field lines (black curves) are nearly vertical.Fig. 2. Frequency-time spectrogram of electromagnetic waves measured by MAVEN.
Wave intensity is color-coded according to the scale on the right. A dispersed whistler is observed in the second half of the time interval at frequencies up to about 110 Hz. The black dashed line shows a theoretical spectral shape for an impulsive source in the Martian atmosphere, calculated from a model with realistic magnetic field and plasma density profiles.
SETI Institutesetiinstitute
2026-03-06

: Martian 'Spiderwebs' Up Close

From orbit, parts of Mars look like sprawling spiderwebs etched across the hillsides. These patterns may record a time when groundwater flowed through large fractures in the rock, leaving minerals behind. Over time, those minerals hardened into ridges while the surrounding rock—lacking that reinforcement—was slowly worn away by wind.

Five panel close-up stitched view of a rock formation on the surface of Mars, as seen by the Curiosity rover. The formation is a light, sand color and is covered in pea-sized nodules.
adsdailyadsdaily
2026-03-04

📄 JWST Thermal Emission of the Terrestrial Exoplanet GJ 1132b

Quicklook:
Xue, Qiao et al. (2024) · The Astrophysical Journal
Reads: 166 · Citations: 49
DOI: 10.3847/2041-8213/ad72e9

🔗 ui.adsabs.harvard.edu/abs/2024

Scientific Frontlinesflorg
2026-03-03

Analysis of ancient zircon grains indicates that early Earth experienced rapid oxidation shortly after its formation and confirms that plate tectonics were active much earlier than previously recognized.

sflorg.com/2026/03/es03032602.

2026-03-03

Icy or Rocky Giants?

On the outskirts of our solar system, two enigmatic giants loom: Uranus and Neptune. In terms of mass and size, both resemble many of the exoplanets discovered in recent years. Within our own solar system, these planets are known as “icy giants,” but a new study suggests that moniker may be wrong.

Pinning down the interior composition of a planet is tough on limited measurements. In the case of these outer planets, our main data is gravitational, recorded from visiting spacecraft. That information cannot tell us directly what the composition of a planet is, but it gives constraints for what materials could produce such a gravitational field.

In their simulation, researchers began with random interior configurations for Uranus and Neptune, then had the model iterate through configurations to simultaneously match the gravitational measurements while satisfying the thermodynamic and physical constraints of a stable planet. By repeating the process several times, the researchers created a catalog of potential interiors for Uranus and Neptune. And while some were water-rich–consistent with the “icy giant” title–others were remarkably rocky.

The team suggests that we may need to retire that moniker and consider the possibility that these worlds are more like our own than we thought. To find out which is true, we will need more spacecraft to visit our frigid neighbors, to provide new gravitational measurements and other observations. (Image credit: NASA/ESA/A. Simon/M. Wong/A. Hsu; research credit: R. Morf and L. Helled; via Physics World)

#fluidDynamics #geophysics #Neptune #numericalSimulation #physics #planetaryScience #science
Hubble images of Uranus (left) and Neptune (right).
SETI Institutesetiinstitute
2026-03-02

: Korea’s Kompsat-2 satellite captured this image over the sand seas of the Namib Desert on 7 January 2012. The blue-and-white area is the dry riverbed of the Tsauchab. Black dots of vegetation are concentrated close to the river’s main route, while salt deposits appear bright white. Running through the river valley, a road connects Sossusvlei to the Sesriem settlement. Credit: KARI/ESA

Satellite photo of the Namib Desert. The top two-thirds are covered in red, undulated sand dunes, leading down to a dry river bed, seen in bands of blue and white. Along the river bed, black dots of vegetation curl around the pointed tips of dunes.
Scientific Frontlinesflorg
2026-03-01

Welcome to this week's installment of the Scientific Frontline publication’s "What Is" series. In this comprehensive research report, the focus turns toward the most intricate, dynamic, and fragile phenomenon known to modern science: the biosphere. Earth remains, according to all current astronomical observations, a solitary oasis of vitality in an otherwise sterile cosmic void.

sflorg.com/2026/03/wi03012601.

SETI Institutesetiinstitute
2026-02-28

Dr. Kimberly Bott received her PhD from the University of New South Wales, working on exoplanet polarimetry (observation and computational modeling). Subsequently, she held postdoc positions at the Virtual Planetary Laboratory and UC Riverside.

Currently, Dr. Bott is investigating the observability of terrestrial exoplanets in polarized light with contemporary and near-future telescopes and how the method might be used to map those worlds.

Text: #notjustaliens. Kimberly Bott, Planetary Science. Background: Starry night sky. Inset: Photo of Kimberly Bott.Text: Dr. Kimberly Bott received her PhD from the University of New South Wales working on exoplanet polarimetry (observation and computational modeling). Subsequently, she held postdoc positions at the Virtual Planetary Laboratory and UC Riverside. Background: Starry night sky with graphics of a star and exoplanets in front of it.Text: Currently, Dr. Bott is investigating the observability of terrestrial exoplanets in polarized light with contemporary and near-future telescopes and how the method might be used to map those worlds. Background: Starry night sky with graphics of a star and exoplanets.
SETI Institute logo. Graphics: (top) Black hole. (bottom) radio telescope dishes at the Allen Telescope Array. Background: Starry night sky.
ReDATA, University of Arizonaredata
2026-02-27

🔴Do you know that the seasonal streaks on ’ Martian slopes often result from dust storms, not water? 🌪️Research by Alfred S. McEwen, Ethan Schaefer, Colin M. Dundas, Sarah S Sutton, Leslie K Tamppari, and Matthew Chojnacki found that many new streaks appeared after the massive 2018 dust storm. Learn more from their dataset & article at doi.org/10.25422/azu.data.1338 & doi.org/10.1029/2020JE006575. Image: McEwen et al. (2021). CC BY-NC-ND 4.0.

Gullies on south-southwest-facing slopes with candidate RSL in west-facing slope facets, plus dust devil tracks. ESP_057951_1400 acquired December 7, 2018, MY34, Ls 302º, post-PEDE. All images in this paper are map projected with north up and illumination from the left (west). Full-resolution and uncropped versions of these and other images shown in this paper are available at https://uahirise.org. RSL, recurring slope lineae; PEDE, planet-encircling dust event.
SETI Institutesetiinstitute
2026-02-27

: With Mars on the opposite side of the Sun at dawn, only six planets were visible in this year's planetary parade, unlike last year, when all seven were in view. The timing of this shot was critical for the fainter planets, and astrophotographer Josh Dury cross-referenced planispheres to confirm their location. Credit: Josh Dury

Photograph of the night sky seen over the sculpture of a planisphere. At top left is Jupiter. The Moon is seen near the middle. Just below the moon is Uranus. Near the horizon are Neptune, Saturn, Mercury and Venus. All planets are marked with white circles and labeled.
Wilhelmusvvilhelmus
2026-02-27

Wonderful re-introduction to the Uranian planetary system by with all the latest updates. 🪐

If 18th century astronomers had named this : after the Roman god of the sky instead of the Greek one, then would be wearing an "Occupy Caelus" T-shirt instead of an "Occupy Mars" T-shirt. 🤷

youtu.be/wKcMvR2C0oA

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