Japanese Researchers Show how Microgravity Affects Astronauts’ Muscles and Nerves

Canadian astronaut Robert Thirsk using the exercise bike on the ISS. Exercise is one way of combatting muscle atrophy in space. Image Credit: NASA

It’s well-known that spending long periods in microgravity can adversely affect astronaut health and physiology. According to decades of research performed aboard the International Space Station (ISS), like NASA’s much-popularized Twins Study, these effects include the loss of muscle mass and bone density, as well as changes to cardiovascular health, eyesight, organ function, and gene expression. There’s even the possibility that astronauts will experience mood swings and psychological problems while in space or during recovery here on Earth.

According to a recent study by a team of Japanese researchers, one of the lesser-studied effects is how long periods spent in microgravity can damage the skeletal muscles that are important to maintaining our posture. This group of muscles – located mostly in our limbs, back, and neck – are rightly known as our “anti-gravity” muscles because they are load-bearing and allow us to stand upright and move against the force of gravity. This research and the countermeasures they propose could have significant implications for astronauts returning from long-term stays in space.

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Gravitational Wave Telescopes Could Detect Clumps of Dark Matter Drifting Through the Solar System

This image shows the galaxy MCS J0416.1–2403, one of six clusters targeted by the Hubble Frontier Fields programme. The blue in this image is a mass map created by using new Hubble observations combined with the magnifying power of a process known as gravitational lensing. In red is the hot gas detected by NASA’s Chandra X-Ray Observatory and shows the location of the gas, dust and stars in the cluster. The matter shown in blue that is separate from the red areas detected by Chandra consists of what is known as dark matter, and which can only be detected directly by gravitational lensing.Credit: ESA/Hubble, NASA, HST Frontier Fields. Acknowledgement: Mathilde Jauzac (Durham University, UK) and Jean-Paul Kneib (École Polytechnique Fédérale de Lausanne, Switzerland).

Attempts to directly detect dark matter have come up empty. A team of physicists have proposed a brand new method: if dark matter exists in clumps that occasionally pass through the solar system, we may be able to detect their slight influence with ultra-sensitive gravitational waves detectors.

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Here’s M74 Like You’ve Never Seen it Before, Thanks to Judy Schmidt and JWST

The JWST recently imaged NGC628, also knows an M74. Well-known astronomy image processor Judy Schmidt reworked the image to show more detail. Image Credit: NASA/ESA/CSA/STSCI/JUDY SCHMIDT CC BY 2.0

The JWST is grabbing headlines and eyeballs as its mission gains momentum. The telescope recently imaged M74 (NGC 628) with its Mid-Infrared Instrument (MIRI.) Judy Schmidt, a well-known amateur astronomy image processor, has worked on the image to bring out more detail.

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An Ambitious Plan to Find Earth 2.0

When it comes to astronomy, the more instruments watching the sky, the better. Which is why it has been so frustrating that the world’s rising superpower – China – has long lacked focus on space-science missions. In recent years, with some notable exceptions, China’s space agency has focused on lunar exploration and human spaceflight, as well as some remote monitoring capabilities, leaving the technical know-how of arguably the world’s second more capable country on the sidelines when it comes to collecting space science data. Now, a team led by Jian Ge of the Shanghai Astronomical Observatory has suggested the most ambitious Chinese-led space science mission to date. And it plans to search for one of the holy grails of current astronomy research – an exoplanet like Earth.

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A Dormant Black Hole has Been Discovered Just Outside the Milky Way

home of the dormant black hole

What happens when a massive star dies? Conventional wisdom (and observational evidence) say that it can collapse to form a “stellar-mass” black hole. Astronomers detect black holes by the X-ray emissions they emit.

But, what if the black hole isn’t giving off high levels of X-ray emissions? Then, it could be a very rare object indeed: a dormant black hole. Not many of these have been seen. So, it’s exciting to know that a team of astronomers has found one. It’s called VFTS 243. They detected it in Very Large Telescope observations of stars in the Tarantula Nebula, in the neighboring Large Magellanic Cloud.

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You can see Where JWST Took a Direct hit From a Micrometeorite on one of its Mirrors

Artist conception of the James Webb Space Telescope. Credit: NASA GSFC/CIL/Adriana Manrique Gutierrez

The world is still reeling from the release of the James Webb Space Telescope‘s (JWST) first images. These provided a comprehensive overview of the kind of science operations that Webb will conduct over its 20-year mission. They included the most sensitive and detailed look at some iconic astronomical objects, spectra from an exoplanet atmosphere, and a deep field view of some of the most distant galaxies in the Universe. Since their release, we’ve also been treated to glimpses of objects in the Solar System captured by Webb‘s infrared instruments.

Meanwhile, the JWST collaboration released a full report titled titled “Characterization of JWST science performance from commissioning,” in which they examined everything Webb has accomplished so far and what they anticipate throughout the mission. This paper recently appeared online and covers everything from the telescope’s navigation and pointing to the performance of its many instruments. An interesting tidbit, which was not previously released, is how Webb suffered a series of micrometeoroid impacts, one of which caused “uncorrectable change” in one mirror segment.

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Uh Oh, NASA is Reviewing Psyche and May Terminate the Mission

NASA's mission to asteroid 16 Psyche has been delayed. Now a review panel is examining the delay. Credit: Maxar/ASU/P. Rubin/NASA/JPL-Caltech

NASA is reviewing its mission to visit the asteroid 16 Psyche. The Administration has convened a 15-member review board to examine the mission and its failure to meet the scheduled 2022 launch. The review began on July 19, and the board will present their findings to NASA and JPL in late September.

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Earth has Clouds of Water. Hot Exoplanets Have Clouds of Sand

Artist's impression of a lava world. The exoplanet K2-141b is so close to its host star that it likely has magma oceans and surface temperatures over 3000 degrees. It's possible water is mixed in with the magma. c. ESO
Artist's impression of a lava world. The exoplanet K2-141b is so close to its host star that it likely has magma oceans and surface temperatures over 3000 degrees. It's possible water is mixed in with the magma. c. ESO

A team of astronomers studied brown dwarfs to figure out how hot exoplanets form clouds of sand. They found that sand clouds can only exist in a narrow range of temperatures.

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We Finally Know Where the Highest Energy Cosmic Rays are Coming From: Blazars

blazar

Way out there in space is a class of objects called blazars. Think of them as extreme particle accelerators, able to marshall energies a million times stronger than the Large Hadron Collider in Switzerland. It turns out they’re the culprits in one of the great astrophysical mysteries: what creates and propels neutrinos across the universe at blazingly fast speeds? It turns out that the answer’s been there all along: blazars pump out neutrinos and cosmic rays. That’s the conclusion a group of astronomers led by Dr. Sara Buson of Universität Wurzburg in Germany came to as they studied data from a very unique facility here on Earth: the IceCube Neutrino Observatory in Antarctica.

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The Gravitational Constant is Tricky to pin Down Accurately. Here’s a new way to Measure it

The central parts of our Galaxy, the Milky Way, as observed in the near-infrared with the NACO instrument on ESO's Very Large Telescope. The position of Sgr A*,with a mass 4 million times that of the Sun, is marked by the orange cross. The star S2 made a close pass to the region of the black hole in 2018. Courtesy ESO.
The central parts of our Galaxy, the Milky Way, as observed in the near-infrared with the NACO instrument on ESO's Very Large Telescope. The position of Sgr A*,with a mass 4 million times that of the Sun, is marked by the orange cross. The star S2 made a close pass to the region of the black hole in 2018. Courtesy ESO.

A team of physicists have used a pair of vibrating rods to measure the gravitational constant to incredibly fine precision. While the new technique has relatively high uncertainty, they hope that future improvements will provide a new pathway to nailing down this elusive constant.

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