Lifeboat Foundation

Scientists have discovered far more water ice deposits near the Moon’s south pole than previously hypothesized, which could help astronauts on future crewed missions to the lunar surface.

How much water ice could be present within the permanently shadowed regions (PSRs) near the Moon’s south pole? This is what a recent study published in The Planetary Science Journal hopes to address as a team of researchers investigated how water ice deposits could exist hundreds of miles beyond the PSRs located near the south pole, as opposed to close proximity to the south pole as previous studies have hypothesized. This study holds the potential to enable future crewed missions to locate water ice deposits, which could assist in water usage, oxygen generation from electrolysis, fuel, and energy.

For the study, the researchers used NASA’s Lunar Reconnaissance Orbiter (LRO) to obtain data on hydrogen concentration within several PSR craters near the lunar south pole, along with potential sources of the hydrogen concentrations. The reason PSRs are targets for water ice is due to their extreme depths where sunlight doesn’t reach, resulting in temperatures well below-freezing and the accumulation of water ice over millions, if not billions, of years. The team found that hydrogen concentrations existed in craters several hundred miles from the direct south pole and with temperatures below 75 Kelvin (−198.15 degrees Celsius/-324.67 degrees Fahrenheit). Additionally, the team also concluded that the likely sources of the hydrogen concentrations were from a variety of sources, including solar radiation, comets, and meteorites.

Continue reading “Widespread Water Ice Deposits Discovered on the Moon” »

Ian Pamerleau: “We used multiple observations made with Dawn data as motivation for finding an ice-rich crust that resisted crater relaxation on Ceres. Different surface features (e.g., pits, domes and landslides, etc.) suggest the near subsurface of Ceres contains a lot of ice.”

Was the dwarf planet Ceres once an ocean world like Europa and Enceladus? If so, how did it become the cratered and icy world we see today? This is what a recent study published in Nature Astronomy hopes to address as a team of researchers from Purdue University and NASA’s Jet Propulsion Laboratory (JPL) investigated the formation and evolution of the internal geological processes of Ceres and how this could help scientists better understand ocean worlds throughout the solar system.

“We think that there’s lots of water-ice near Ceres surface, and that it gets gradually less icy as you go deeper and deeper,” said Dr. Mike Sori, who is an assistant professor in the Department of Earth, Atmospheric, and Planetary Sciences at Purdue University and a co-author on the study. “People used to think that if Ceres was very icy, the craters would deform quickly over time, like glaciers flowing on Earth, or like gooey flowing honey. However, we’ve shown through our simulations that ice can be much stronger in conditions on Ceres than previously predicted if you mix in just a little bit of solid rock.”

Continue reading “How Ceres Challenges Our Understanding of Icy Bodies” »

https://earthobservatory.nasa.gov/images/153422/sprites-camera-action.

An astronaut on the International Space Station captured a red sprite over North America, a rare atmospheric phenomenon associated with powerful lightning.

Continue reading “Astronauts Reveal Dazzling Red Sprites: Stunning Phenomena Captured From Space Station [Video]” »

An international team of astronomers has performed radio observations of a star-forming galaxy known as NGC 4217. The observational campaign detected a large radio bubble in the galaxy’s halo. The finding was reported in a paper published September 23 on the pre-print server arXiv.

The U.S. National Science Foundation (NSF) Daniel K. Inouye Solar Telescope, the world’s most powerful solar telescope, designed, built, and operated by the NSF National Solar Observatory (NSO), achieved a major breakthrough in solar physics by directly mapping the strength of the magnetic field in the solar corona, the outer part of the solar atmosphere that can be seen during a total eclipse. This breakthrough promises to enhance our understanding of space weather and its impact on Earth’s technology-dependent society.

The corona: the launch pad of space weather.

The Sun’s magnetic field generates regions in the Sun’s atmosphere, often rooted by sunspots, that store vast amounts of energy that fuel explosive solar storms and drive space weather. The corona, the Sun’s outer atmosphere, is a superheated realm where these magnetic mysteries unfold. Mapping coronal magnetic fields is essential to understanding and predicting space weather — and to protect our technology in Earth and space.

Solar storms, characterized by sudden explosions of particles, energy, and magnetic fields from the Sun, can create disruptions in Earth’s magnetosphere. As told to NDTV, Dr. Annapurni Subramanian, Director of the Indian Institute of Astrophysics, stated, “The (solar) flare which occurred a few days ago is similar in terms of strength to the one which occurred in May.” These flares are known to produce geomagnetic storms that can result in radio blackouts and power outages on Earth.

Recent NDTV reports highlight a series of powerful solar flares emitted by the Sun, including an X7.1 flare on October 1 and an even stronger X9.0 flare on October 3. NASA captured these flares using its Solar Dynamics Observatory, emphasizing their potential to disrupt communication systems. NOAA classified the X9.0 flare as an R3-strength flare, indicating a “strong” potential for radio blackouts.

The team spotted the record-breaking triple star system because of strobing starlight caused by the stars crossing in front of each other, as seen from our position on Earth.

The team turned to machine learning to analyze vast amounts of data from TESS to spot a pattern indicating these eclipses. They then called upon the aid of citizen scientists to further filter this data to spot interesting signals.

“We’re mainly looking for signatures of compact multi-star systems, unusual pulsating stars in binary systems, and weird objects,” Rappaport said. “It’s exciting to identify a system like this because they’re rarely found, but they may be more common than current tallies suggest.”

Researchers at the University of Hawaiʻi have revealed that our galaxy, part of the Laniākea supercluster, might actually reside within a significantly larger cosmic structure, potentially centered around the massive Shapley concentration.

This discovery, emerging from the study of 56,000 galaxies, suggests that our cosmic neighborhood could be 10 times larger than previously estimated, challenging existing models of the universe’s structure.

An international research team guided by astronomers at the University of Hawaiʻi Institute for Astronomy is challenging our understanding of the universe with groundbreaking findings that suggest our cosmic neighborhood may be far larger than previously thought. The Cosmicflows team has been studying the trajectories of 56,000 galaxies, revealing a potential shift in the scale of our galactic basin of attraction.

The Parker Solar Probe has matched its own speed and distance records in a recent close encounter with the Sun and is preparing for an even closer approach aided by a Venus flyby.

On September 30, NASAs Parker Solar Probe completed its 21st close approach to the Sun, equaling its own distance record by coming within about 4.51 million miles (7.26 million kilometers) of the solar surface.

The close approach (known as perihelion) occurred at 5:15 UTC — or 12:15 a.m. EDT — with Parker Solar Probe moving 394,700 miles per hour (635,300 kilometers per hour) around the Sun, again matching its own record. The spacecraft checked in on October 3 with mission operators at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland — where the spacecraft was also designed and built — with a beacon tone indicating it was in good health and all systems were operating normally.