Fast radio bursts (FRBs) represent the most intense radio explosions in the universe. Since the first discovery in 2007, FRBs have garnered significant attention, culminating in the 2023 Shaw Prize in Astronomy. With yet unknown origin, these extreme cosmic bursts are among the most enigmatic phenomena in astronomy as well as physics.
“The problems arising when interpreting the data from WASP-39b are well known from many other exoplanets — regardless whether they are observed with Kepler, TESS, James Webb, or the future PLATO spacecraft,” said Dr. Nadiia Kostogryz.
While there is currently a myriad of techniques used to both discover exoplanets and calculate their physical characteristics, could other methods be developed to overcome specific data errors? This is what a recent study published in Nature Astronomy hopes to address as an international team of researchers investigated how a star’s magnetic field can be used to ascertain additional data for an exoplanet, which is traditionally done using conventional exoplanet detection methods, specifically the transit detection method. This study holds the potential to help astronomers establish new methods for discovering and characterizing exoplanets throughout the cosmos.
For the transit method, an exoplanet passes in front of its parent star, causing its starlight to slightly decrease and has been instrumental in discovering and characterizing thousands of exoplanets. However, astronomers have also discovered that a star’s limb darkening, which is the observed edge of the star, causes errors in transit light curves for exoplanets, despite using state-of-the-art atmospheric models to predict observations.
For the study, the researchers focused on WASP-39b, which is a gas giant located approximately 700 light-years from Earth and has been studied in great detail using a myriad of space telescopes, and most recently with NASA’s James Webb Space Telescope (JWST). However, astronomers have discovered inconsistencies between models and observations, which this study hopes to overcome.
How much of Venus’s atmosphere is being stripped by the Sun, and what can this tell us about how the planet lost its water long ago? This is what a recent study published in Nature Astronomy hopes to address as a team of international researchers examined data obtained from a 2021 Venus flyby by the BepiColombo spacecraft, which is a joint mission between the European Space Agency (ESA) and Japan Aerospace and Exploration Agency (JAXA) currently en route to Mercury. This study holds the potential to help researchers better understand the formation and evolution of planetary atmospheres, both within our solar system and beyond.
“Characterizing the loss of heavy ions and understanding the escape mechanisms at Venus is crucial to understand how the planet’s atmosphere has evolved and how it has lost all its water,” said Dr. Dominique Delcourt, who is a CNRS researcher at the Plasma Physics Laboratory (LPP) and the Principal Investigator of the Mass Spectrum Analyzer (MSA) instrument onboard BepiColombo, and a co-author on the study.
During its journey to Mercury, BepiColombo needs to conduct several gravity assists to slow down enough to enter Mercury’s orbit, with one such gravity assist occurring at Venus on August 10, 2021. During this flyby, BepiColombo passed through Venus’s magnetosheath, which is Venus’s version of a weak magnetic field that is produced by charged particles from the Sun interacting with Venus’s upper atmosphere. Over the course of 90 minutes, BepiColombo and its powerful instruments successfully measured data on how much atmospheric loss Venus is currently experiencing, which could help researchers better understand the formation and evolution of Venus’s atmosphere, and specifically how the planet lost its water long ago.
A team of international astronomers have discovered 49 new gas-rich galaxies using the MeerKAT radio telescope in South Africa from observations that were not even three hours long and were made possible by IDIA (Inter-University Institute of Data Intensive Astronomy).
The International Space Station shares an out-of-this-world view of the celestial event. ABC News’ Gio Benitez reports.
On April 9, 1959, reporters and news media crammed into the ballroom of the Dolley Madison House in Washington—the location of NASA Headquarters at that time—to learn the names of the first American astronauts who came to be known as the Mercury 7. Public Information Director Walter Bonney kicked off the announcement by pointing to the seven men sitting on stage. “These are our astronaut volunteers,” he announced. “Take your pictures as you will, gentlemen.” One of those men on the dais, Deke Slayton, a test pilot from Edwards Air Force Base, recalled the pandemonium he witnessed. “I’ve never seen anything like it, before or since.” He described the event as, “a frenzy of light bulbs and questions…it was some kind of roar.” His colleague, Wally Schirra, a test pilot from Naval Air Station Patuxent River, called the media’s interest scary because he soon came to realize that their, “private lives were in jeopardy.”
Groundbreaking observations by the James Webb Space Telescope of an early galaxy merger indicate faster and more efficient star formation than previously understood, revealing complex stellar populations and challenging current cosmological theories. Galaxies and stars developed faster after t.
A multidisciplinary team is teaching dog-like robots to navigate the moon’s craters and other challenging planetary surfaces.
As part of the research funded by NASA, researchers from various universities and NASA Johnson Space Center tested a quadruped named Spirit at Palmer Glacier on Oregon’s Mount Hood.
During five days of testing in the summer of 2023, Spirit traversed various terrains, ambling over, across, and over around shifting earth, mushy snow, and stones with his spindly metal legs.
Kyushu University researchers have shed new light into a critical question on how baby stars develop. Using the ALMA radio telescope in Chile, the team found that in its infancy, the protostellar disk that surrounds a baby star discharges plumes of dust, gas, and electromagnetic energy.
These “sneezes,” as the researchers describe them, release the magnetic flux within the protostellar disk, and may be a vital part of star formation. Their findings were published in The Astrophysical Journal.
Stars, including our sun, all develop from what are called stellar nurseries, large concentrations of gas and dust that eventually condense to form a stellar core, a baby star. During this process, gas and dust form a ring around the baby star called the protostellar disk.
Posted in nuclear energy, physics, space, sustainability | 1 Comment on The proton engine Einstein predicted, created for the first time: challenges the laws of the universe and makes cars sustainable
Do you know what they’ve discovered? This is the proton engine that Einstein predicted decades ago and that, for the first time, they’ve managed to materialize. The best part? It challenges even the laws of physics and the universe, and it’s going to decarbonize transportation.
Nuclear fusion has long been a sought-after but elusive goal for science. It involves joining atomic nuclei to release energy, the same process that occurs in the Sun and other stars. In fact, it’s a process similar to what we saw two weeks ago with the plasma engine.
Unlike nuclear fission used in current nuclear power plants—which, remember, we are highly critical of due to its lack of being an eco-friendly or renewable option—fusion offers the promise of a virtually inexhaustible and clean energy source.
