Lifeboat Foundation

In a study published in The Astrophysical Journal, Prof. Zhou Xia from the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences and collaborators have, for the first time, derived the dispersion relation for photons with nonzero mass propagating in plasma, and established a stringent upper limit for the photon mass at 9.52 × 10–46 kg (5.34 × 10–10 eV c-2) using data collected by ultra-wideband (UWB) receivers from pulsar timing and fast radio bursts (FRBs).

A study analyzing the properties of polarized light from 128 non-repeating FRBs reveals mysterious cosmic explosions originate in far-away galaxies like our own Milky Way.

New research from the University of Toronto utilizing data from the Canadian Hydrogen Intensity Mapping Experiment reveals that the majority of Fast Radio Bursts (FRBs) likely originate from environments similar to our Milky Way, with modest densities and magnetic fields. This finding contrasts with earlier studies which suggested that repeating FRBs come from highly magnetized areas.

Fast Radio Burst Research Advancements

Astronomers are expecting a “new star” to appear in the night sky anytime between now and September in a celestial event that has been years in the making, according to NASA.

“It’s a once-in-a-lifetime event that will create a lot of new astronomers out there, giving young people a cosmic event they can observe for themselves, ask their own questions, and collect their own data,” said Dr. Rebekah Hounsell, an assistant research scientist specializing in nova events at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, in a statement. “It’ll fuel the next generation of scientists.”

The expected brightening event, known as a nova, will occur in the Milky Way’s Corona Borealis, or Northern Crown constellation, which is located between the Boötes and Hercules constellations.

Dr. Adomas Valantinas: “What we’re seeing may be a remnant of an ancient climate cycle on modern Mars, where you had precipitation and maybe even snowfall on these volcanoes in the past.”

How unique is the climate of Mars compared to Earth? This is what a recent study published in Nature Geoscience hopes to address as a team of international researchers investigated how frost could form on the summits of volcanoes that comprise the Tharsis volcanic province on Mars. This study holds the potential to help researchers better understand the present-day water cycle on the Red Planet and could have implications for harnessing some of it for future human exploration, as well.

For the study, the researchers used more than 30,000 images from the European Space Agency’s Trace Gas orbiter and the European Space Agency’s Mars Express orbiter to analyze morning frost on the summits of Olympus Mons (Mars’ tallest volcano and the tallest planetary mountain in the solar system), Arsia and Ascraeus Montes, and Ceraunius Tholus. Additionally, the researchers used climate model simulations to ascertain if water could condense and form at these summits, as well.

Continue reading “First Detection of Frost on Mars’ Equatorial Volcanoes” »

Mars isn’t protected.

Why is the warm gas-giant exoplanet WASP-107 b so puffy? Two independent teams of researchers have an answer.

Data collected using NASA’s James Webb Space Telescope, combined with prior observations from NASA’s Hubble Space Telescope, show surprisingly little methane (CH4) in the planet’s atmosphere, indicating that the interior of WASP-107 b must be significantly hotter and the core much more massive than previously estimated.

The unexpectedly high temperature is thought to be a result of tidal heating caused by the planet’s slightly non-circular orbit, and can explain how WASP-107 b can be so inflated without resorting to extreme theories of how it formed.

NASA will roll the fully assembled core stage for the agency’s SLS (Space Launch System) rocket that will launch the first crewed Artemis mission out of NASA’s Michoud Assembly Facility in New Orleans in mid-July. The 212-foot-tall stage will be loaded on the agency’s Pegasus barge for delivery to Kennedy Space Center in Florida.

Media will have the opportunity to capture images and video, hear remarks from agency and industry leadership, and speak to subject matter experts with NASA and its Artemis industry partners as crews move the rocket stage to the Pegasus barge.

NASA will provide additional information on specific timing later, along with interview opportunities. This event is open to U.S. and international media. International media must apply by June 14. U.S. media must apply by July 3. The agency’s media credentialing policy is available online.

It may seem like the sun is stationary while the planets in its orbit are moving, but the sun is actually orbiting around the Milky Way galaxy at an impressive rate of about 220 kilometers per second—almost half a million miles per hour. As fast as that may seem, when a faint red star was discovered crossing the sky at a noticeably quick pace, scientists took notice.

“Many primary atmospheres of those planets will probably be dominated by hydrocarbon compounds and not so much by oxygen-rich gases such as water and carbon dioxide,” said Dr. Thomas Henning.

Can rocky planets form around stars smaller than our Sun, also called low-mass stars? This is what a recent study published in Science hopes to address as a team of international researchers investigated the chemical properties of an exoplanetary system orbiting the star, ISO-Chal 147, which is located approximately 600 light-years from Earth and whose star has a mass of 11 percent of our Sun with age estimates between 1 to 2 million years old. For context, our Sun is approximately 4.5 billion years old. This study holds the potential to help astronomers better understand the formation and evolution of young exoplanetary systems and their potential to host rocky planets.

For the study, the researchers used the Mid-Infrared Instrument (MIRI) on the NASA’s James Webb Space Telescope (JWST) to identify carbon-bearing molecules at temperatures of approximately 30 degrees Celsius (86 degrees Fahrenheit) within the protoplanetary disk forming around the young star. However, the team also found these molecules did not possess compounds containing oxygen, meaning the system might not have water or carbon dioxide, which are typically found in systems surrounding stars like our Sun.

Continue reading “Implications for Rocky Planet Formation Around Low-Mass Stars” »