The James Webb is Measuring Distant Galaxies 5-10 Times Better Than any Other Telescope

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

On December 25th, 2021, after many years of waiting, the James Webb Space Telescope (JWST) finally launched to space. In the sixth-month period that followed, this next-generation observatory unfurled its Sunshield, deployed its primary and secondary mirrors, aligned its mirror segments, and flew to its current position at the Earth-Sun Lagrange 2 (L2) Point. On July 12th, 2022, the first images were released and presented the most-detailed views of the Universe. Shortly thereafter, NASA released an image of the most distant galaxy ever observed (which existed just 300 million years after the Big Bang).

According to a new study by an international team of scientists, the JWST will allow astronomers to obtain accurate mass measurements of early galaxies. Using data from James Webb’s Near-Infrared Camera (NIRCam), which was provided through the GLASS-JWST-Early Release Science (GLASS-ERT) program, the team obtained mass estimates from some of the distant galaxies that were many times more accurate than previous measurements. Their findings illustrate how Webb will revolutionize our understanding of how the earliest galaxies in the Universe grew and evolved.

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A Black Hole can Tear a Neutron Star Apart in Less Than 2 Seconds

Numerical simulation of a black hole-neutron star merger. Credit and ©: K. Hayashi (Kyoto University)

Almost seven years ago (September 14th, 2015), researchers at the Laser Interferometer Gravitational-wave Observatory (LIGO) detected gravitational waves (GWs) for the first time. Their results were shared with the world six months later and earned the discovery team the Noble Prize in Physics the following year. Since then, a total of 90 signals have been observed that were created by binary systems of two black holes, two neutron stars, or one of each. This latter scenario presents some very interesting opportunities for astronomers.

If a merger involves a black hole and neutron star, the event will produce GWs and a serious light display! Using data collected from the three black hole-neutron star mergers we’ve detected so far, a team of astrophysicists from Japan and Germany was able to model the complete process of the collision of a black hole with a neutron star, which included everything from the final orbits of the binary to the merger and post-merger phase. Their results could help inform future surveys that are sensitive enough to study mergers and GW events in much greater detail.

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Before we Develop Self-Replicating Machines to Explore the Universe, we Should Figure out how to Turn Them off Again

An early NASA concept of an interstellar space probe. Credit: NASA/Johns Hopkins University Applied Physics Laboratory

In 1948/49, famed computer scientist, engineer, and physicist John von Neumann introduced the world to his revolutionary idea for a species of self-replicating robots (aka. “Universal Assemblers”). In time, researchers involved in the Search for Extraterrestrial Intelligence (SETI) adopted this idea, stating that self-replicating probes would be an effective way to explore the cosmos and that an advanced species may be doing this already. Among SETI researchers, “Von Neumann probes” (as they’ve come to be known) are considered a viable indication of technologically advanced species (technosignature).

Given the rate of progress with robotics, it’s likely just a matter of time before humanity can deploy Von Neumann probes, and the range of applications is endless. But what about the safety implications? In a recent study by Carleton University Professor Alex Ellery explores the potential harm that Von Neumann Probes could have. In particular, Ellery considers the prospect of runaway population growth (aka. the “grey goo problem”) and how a series of biologically-inspired controls that impose a cap on their replication cycles would prevent that.

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Nancy Grace Roman Will be Launching on a Falcon Heavy Rocket

Artist's impression of the Nancy Grace Roman Space Telescope, named after NASA’s first Chief of Astronomy. When launched later this decade, the telescope should make a significant contribution to the study of FFPs. Credits: NASA

In 2026, the Nancy Grace Roman Space Telescope (RST) – aka. the “Mother of Hubble” – will take to space and begin addressing some of the deepest mysteries of the Universe. This will include capturing the deepest field images of the cosmos, refining measurements of the Hubble Constant (aka. Hubble’s Law), and determining the role of Dark Matter and Dark Energy in the evolution of the cosmos. Alongside its next-generation partner, the James Webb Space Telescope (JWST), the RST will acquire infrared images with over 200 times the surveying power of its predecessor with the same rich level of detail.

On Tuesday, July 19th, NASA announced that it had awarded SpaceX with a Launch Services (NLS) II contract to provide the rocket that will deploy the RST mission to space. As specified in the NLS II, the launch will take place in October 2026 (May 2027, at the latest) and consist of a Falcon Heavy rocket transporting the RST from Launch Complex 39A at NASA’s Kennedy Space Center to orbit. This indefinite-delivery/indefinite-quantity contract is valued at approximately $255 million and covers the launch and other mission-related costs.

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NASA Wants Your Help Designing a Starshade to Observe Exoplanets

Artist's concept of the prototype starshade, a giant structure designed to block the glare of stars so that future space telescopes can take pictures of planets. Credit: NASA/JPL
Artist's concept of the prototype starshade, a giant structure designed to block the glare of stars so that future space telescopes can take pictures of planets. Credit: NASA/JPL

The field of exoplanet study has come a long way in recent decades. To date, 5,063 exoplanets have been confirmed in 3,794 systems beyond our own, with another 8,819 candidates awaiting confirmation. In the coming years, tens of thousands of more planets are expected to be found, thanks to next-generation observatories. The ultimate goal in this search is to find planets that are “Earth-like,” meaning they have a good chance of supporting life. This is no easy task, as rocky planets located within their parent star’s habitable zones (HZs) tend to orbit closely, making them harder to see.

To make this process easier, NASA is designing a hybrid observatory consisting of a “Starshade” that will block out a star’s light so that a ground-based telescope can directly image planets orbiting it. The concept is known as the Hybrid Observatory for Earth-like Exoplanets (HOEE), and NASA is looking for public input to make it a reality. To that end, they have launched the Ultralight Starshade Structural Design Challenge, where participants are asked to develop a design for a lightweight starshade structure that could be used as part of the HOEE concept.

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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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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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A New Method for Making Graphene has an Awesome Application: A Space Elevator!

Credit: Lux Virtual/Galactic Harbor

The Space Elevator is one of those ideas that seems to have an endless supply of lives. Originally proposed about a century ago, this concept calls for a tether of supermaterial that connects a station in orbit to Earth’s surface. Our planet’s rotation would keep this tether taut, and a system of “climbers” would transport people and payloads to and from space. The engineering challenges and costs associated with such a structure have always been enormous. But every generation or so, new research comes along that causes engineers and space agencies to reevaluate the concept.

The single-greatest challenge has always been the tether since no known material has ever been strong enough to handle the stresses involved. But as it turns out, this issue may finally be resolved! According to scientists with the International Space Elevator Consortium (ISEC), a cost-effective manufacturing process could produce graphene ribbons that are strong enough to fashion a tether! Their latest findings are detailed in a paper they will present at the upcoming 2022 International Astronomical Congress in Paris.

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Dmitry Rogozin is no Longer the Head of Roscosmos

Russian Deputy Prime Minister Dmitry Rogozin. Credit: RIA Novosti

According to a recent report by Euronews, the controversial head of Roscosmos (Dmitri Rogozin) has been dismissed from his position. For those associated with space exploration and the global space industry, Rogozin is something of a household name. Since 2018, he has led Russia’s space program and established a reputation for inflammatory statements and anti-Western bluster, especially where Russia’s invasion of Ukraine, U.S., and European sanctions are concerned. His dismissal was part of a reshuffle ordered on Friday, July 15th, by Russian President Vladimir Putin.

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To get Artificial Gravity on the Moon, you'd Need a Giant Rotating Lunar Base

Credit: Kajima Construction

Living and working in space for extended periods of time presents a number of challenges. These include radiation, as locations beyond Earth’s protective magnetosphere are exposed to greater levels of solar and cosmic rays. There’s also the need for self-sufficiency since Lunar or Martian bases are too far to rely on regular resupply missions like the International Space Station (ISS). Last, there’s the issue of low gravity, which is especially pressing for long-term missions and habitats beyond Earth. If humanity’s future truly lies in space, we must devise solutions to this issue in advance.

A popular idea is to create rotating habitats in space that simulate artificial gravity, like the Pinwheel Station or the O’Neill Cylinder. Another proposal by a team of Japanese researchers calls for something bolder: a rotating habitat on the Moon! On July 5th, representatives from Kyoto University and the Kajima Corporation (one of the oldest and largest construction companies in Japan) announced that they would be partnering to conduct a study on this concept and how it could make humanity’s plans for living on the Moon and Mars a reality!

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