Ample evidence of ancient rivers, streams and lakes make it clear that Mars was at some point warm enough for liquid water to flow on its surface. While that may conjure up images of a tropical Martian paradise, new research published in Nature Geoscience throws a bit of cold water on that notion.
New research by a team of European physicists could explain why the universe did not collapse immediately after the Big Bang. Studies of the Higgs particle have suggested that the production of Higgs particles during the accelerating expansion of the very early universe (inflation) should have led to instability and collapse.
While astronomers have observed the protoplanetary disk evolution throughout our galaxy, the mechanism by which planetary disks evolve at such a rapid rate has eluded scientists for decades. Now researchers have provided the first experimental evidence that our solar system’s protoplanetary disk was shaped by an intense magnetic field that drove a massive amount of gas into the sun within just a few million years.
Peering deep into time with one of the world’s newest, most sophisticated telescopes, astronomers have found a galaxy—AzTEC-3—that gives birth annually to 500 times the number of suns as the Milky Way galaxy, according to a new Cornell Univ.-led study published in the Astrophysical Journal.
When the double asteroid Patroclus-Menoetius passed directly in front of a star on the night of Oct. 20, 2014, a team of volunteer astronomers across the U.S. was waiting. Observing the event, known as an occultation, from multiple sites where each observer recorded the precise time the star was obscured, yielded the first accurate determination of the two objects’ size and shape.
Scientists at the Univ. of Arizona have discovered what might be the closest thing to "baby photos" of our solar system. A young star called HD 95086 is found to have two dust belts, analogous to the asteroid and Kuiper belts in the solar system, surrounded by a large dust halo that only young planetary systems have.
Two NASA and one European spacecraft, including NASA’s MAVEN mission led by the Univ. of Colorado Boulder, have gathered new information about the basic properties of a wayward comet that buzzed by Mars October 19, 2014, directly detecting its effects on the Martian atmosphere. Data from observations revealed that debris from the comet caused an intense meteor shower and added a new layer of ions, or charged particles, to the ionosphere.
The physics community has spent decades searching for and finding no evidence that dark matter is made of tiny exotic particles. Case Western Reserve Univ. theoretical physicists suggest researchers consider looking for candidates more in the ordinary realm and, well, more massive. Dark matter is unseen matter, that, combined with normal matter, could create the gravity that, among other things, prevents spinning galaxies from flying apart.
Results from experiments at the Relativistic Heavy Ion Collider, a particle collider located at the Brookhaven National Laboratory, reveal new insights about how quarks and gluons, the subatomic building blocks of protons, contribute to the proton’s intrinsic angular momentum, a property more commonly known as “spin.”
When NASA’s Dawn spacecraft visited the asteroid Vesta in 2011, it showed that deep grooves that circle the asteroid’s equator like a cosmic belt were probably caused by a massive impact on Vesta’s south pole. Now, using a super high-speed cannon at NASA’s Ames Research Center, Brown Univ. researchers have shed new light on the violent chain of events deep in Vesta’s interior that formed those surface grooves.
A disappearing act was the last thing Rice Univ. physicist Randy Hulet expected to see in his ultracold atomic experiments, but that is what he and his students produced by colliding pairs of Bose Einstein condensates (BECs) that were prepared in special states called solitons. Hulet’s team documented the strange phenomenon in a new study published online in Nature Physics.
Astronomers have caught their first glimpse of the invisible magnetic fields that sculpt solar systems. Looking at a bright, nearby baby star and the dust swirling in its cradle, astronomers from the Univ. of Illinois and six collaborating institutions were able to make out the shape of the magnetic field surrounding the star.
Scientists have identified an unexpected high-altitude methane ice cloud on Saturn's moon Titan that is similar to exotic clouds found far above Earth's poles. Now, eight years after spotting this mysterious bit of atmospheric fluff, NASA's Cassini spacecraft, researchers have determined that it contains methane ice, which produces a much denser cloud than the ethane ice previously identified there.
After 116 days of being subjected to extremely frigid temperatures like that in space, the heart of the James Webb Space Telescope, the Integrated Science Instrument Module and its sensitive instruments, emerged unscathed from the thermal vacuum chamber at NASA’s Goddard Space Flight Center. Operating a telescope powerful enough to reveal the first galaxies forming 13.5 billion years ago requires incredibly cold temperatures: about -387 F.
Massive black holes spewing out radio frequency-emitting particles at near-light speed can block formation of new stars in aging galaxies, a study has found. The research provides crucial new evidence that it is these jets of radio frequency feedback streaming from mature galaxies’ central black holes that prevent hot free gas from cooling and collapsing into baby stars.
Using extremely faint light from galaxies 10.8-billion light-years away, scientists have created one of the most complete, 3-D maps of a slice of the adolescent universe. The map shows a web of hydrogen gas that varies from low to high density at a time when the universe was made of a fraction of the dark matter we see today.
Why is the sun's million-degree corona, or outermost atmosphere, so much hotter than the sun's surface? This question has baffled astronomers for decades. A team led by the Harvard-Smithsonian Center for Astrophysics is presenting new clues to the mystery of coronal heating using observations from the recently launched Interface Region Imaging Spectrograph (IRIS).
The findings of NASA’s planet-hunting Kepler spacecraft suggest that the most common exoplanets are those that are just a bit larger than Earth but smaller than Neptune. These so-called super-Earths, which do not exist in our own solar system, have attracted the attention of astronomers, who have been trying to determine the composition of the closest of these planets. However, an unexpected barrier is blocking their progress.
The European Space Agency has confirmed the time and place it will attempt to land the first spacecraft on a comet. The unmanned probe Rosetta will release a 100-kg (220-lb) lander on Nov. 12 in a maneuver that will take about seven hours.
NASA’s MAVEN spacecraft has provided scientists their first look at a storm of energetic solar particles at Mars and produced unprecedented ultraviolet images of the tenuous oxygen, hydrogen and carbon coronas surrounding the Red Planet. In addition, the new observations allowed scientists to make a comprehensive map of highly variable ozone in the Martian atmosphere underlying the coronas.
Astronomers Chih-Hao Li and David Phillips of the Harvard-Smithsonian Center for Astrophysics want to rediscover Venus. They plan to “find” the second planet again using a powerful new optical device installed on the Italian National Telescope that will measure Venus' precise gravitational pull on the sun. If they succeed, their first-of-its-kind demonstration will be later used for finding Earth-like exoplanets orbiting distant stars.
In 2012, the Mars One project, led by a Dutch nonprofit, announced plans to establish the first human colony on the Red Planet by 2025. The mission would initially send four astronauts on a one-way trip to Mars, where they would spend the rest of their lives building the first permanent human settlement.
By focusing on large, star-forming galaxies in the universe, researchers at Johns Hopkins Univ. were able to measure its radiation leaks in an effort to better understand how the universe evolved as the first stars were formed. The team reports in a paper published online in Science that an indicator used for studying star-forming galaxies that leak radiation, is an effective measurement tool for other scientists to use.
Astronomers have detected a pulsating dead star that appears to be burning with the energy of 10 million suns, making it the brightest pulsar ever detected. The pulsar—a rotating, magnetized neutron star—was found in the galaxy Messier 82 (M82), a relatively close galactic neighbor that’s 12 million light-years from Earth.
Certain primordial stars—those between 55,000 and 56,000 times the mass of our sun, or solar masses—may have died unusually. In death, these objects—among the universe’s first-generation of stars—would have exploded as supernovae and burned completely, leaving no remnant black hole behind.