Ingenuity is three for three on Mars.
Ingenuity aced its third-ever Martian flight early this morning (April 25), adding to its already impressive resume.
Ingenuity is three for three on Mars.
Ingenuity aced its third-ever Martian flight early this morning (April 25), adding to its already impressive resume.
A power-beaming experiment is scheduled to launch in 2024.
Space-based solar power won’t be just a sci-fi dream forever, if things go according to the U.S. Air Force’s plans.
Hebrew University Researcher Introduces New Approach to Three-Body Problem, Predicts its Outcome Statistics.
The “three-body problem,” the term coined for predicting the motion of three gravitating bodies in space, is essential for understanding a variety of astrophysical processes as well as a large class of mechanical problems, and has occupied some of the world’s best physicists, astronomers and mathematicians for over three centuries. Their attempts have led to the discovery of several important fields of science; yet its solution remained a mystery.
At the end of the 17th century, Sir Isaac Newton succeeded in explaining the motion of the planets around the sun through a law of universal gravitation. He also sought to explain the motion of the moon. Since both the earth and the sun determine the motion of the moon, Newton became interested in the problem of predicting the motion of three bodies moving in space under the influence of their mutual gravitational attraction (see illustration to the right), a problem that later became known as “the three-body problem.”
Circa 2013
Fusion-based nuclear propulsion has the potential to enable fast interplanetary transportation. Due to the great distances between the planets of our solar system and the harmful radiation environment of interplanetary space, high specific impulse (Isp) propulsion in vehicles with high payload mass fractions must be developed to provide practical and safe vehicles for human space flight missions.
The Z-Pinch dense plasma focus method is a Magneto-Inertial Fusion (MIF) approach that may potentially lead to a small, low cost fusion reactor/engine assembly [1]. Recent advancements in experimental and theoretical understanding of this concept suggest favorable scaling of fusion power output yield [2]. The magnetic field resulting from the large current compresses the plasma to fusion conditions, and this process can be pulsed over short timescales (10−6 s). This type of plasma formation is widely used in the field of Nuclear Weapons Effects testing in the defense industry, as well as in fusion energy research. A Z-Pinch propulsion concept was designed for a vehicle based on a previous fusion vehicle study called “Human Outer Planet Exploration” (HOPE), which used Magnetized Target Fusion (MTF) [3] propulsion.
Perseverance has performed a test of its MOXIE instrument to convert carbon dioxide into oxygen for the first time on Mars.
Great new episode with author and astronomer Linda Schweizer who talks about her new book “Cosmic Odyssey” which covers the history and science of Caltech’s Palomar Observatory.
Astronomer and author Linda Schweizer talks about her comprehensive new history of Palomar Observatory — “Cosmic Odyssey: How Intrepid Astronomers At Palomar Observatory Changed Our View of the Universe” from MIT Press. We focus on Palomar’s early 20th century construction and history. Schweizer is an expert on every aspect of the observatory; its history, and its many astronomical discoveries.
In celebration of the 31st anniversary of the launching of NASA’s Hubble Space Telescope, astronomers aimed the renowned observatory at a brilliant “celebrity star,” one of the brightest stars seen in our galaxy, surrounded by a glowing halo of gas and dust. Credit: NASA, ESA, STScI
The mighty blue giant AG Carinae is not your normal star. One of the brightest stars in our Milky Way galaxy, AG Carinae is sizzling hot, shining with the brilliance of 1 million suns. You would need super sunscreen if you lived in the star’s vicinity. The star is up to 70 times heftier than our Sun and burning fuel at a ferocious rate.
Its opulence means that the mammoth star is living life in the fast lane. Pouring out so much energy takes a toll on the stellar behemoth. It is prone to convulsive fits, expanding in size like a hot air balloon and shedding its outer layers of material into space. One or more giant eruptions 10000 years ago created the beautiful, expanding shell of dust and gas seen here. Stars like this one are rare: less than 50 reside in our local group of neighboring galaxies.
NASA’s Ingenuity Mars helicopter ‘went big’ with its second flight, reaching new milestones with a higher altitude, flying to the side and grabbing another black-and-white photo of its shadow on the ground below.
The US space agency said it climbed up to 16ft above the surface, hovered, tilted slightly and then moved sideways 7ft. When in position it hovered again to take a series of colour photos before landing.
Writing on Twitter, NASA JPL said: Go big or go home! The Mars Helicopter successfully completed its 2nd flight,’ adding that it ‘reached new milestones of a higher altitude, a longer hover, and lateral flying.’
We are made of stardust, the saying goes, and a pair of studies including University of Michigan research finds that may be more true than we previously thought.
The first study, led by U-M researcher Jie (Jackie) Li and published in Science Advances, finds that most of the carbon on Earth was likely delivered from the interstellar medium, the material that exists in space between stars in a galaxy. This likely happened well after the protoplanetary disk, the cloud of dust and gas that circled our young sun and contained the building blocks of the planets, formed and warmed up.
Carbon was also likely sequestered into solids within one million years of the sun’s birth — which means that carbon, the backbone of life on earth, survived an interstellar journey to our planet.
We’ve known for a while that Earth is under a constant rain of space dust, and that it’s copious. Given its microscopic size, however, it’s been very hard to obtain an accurate estimate of the quantity.
Such micrometeorites are no bigger than a fraction of a millimeter, shed like space dander from passing comets and asteroids.
After two decades of collecting the stuff in Antarctica, an international team of scientists now has a number: around 5200 tons of micrometeorites smaller than 700 micrometers (0.7 millimeters), every year.