Swarm of laser-sail spacecraft leaving the solar system. Credit: Adrian Mann
In the past decade, thousands of planets have been discovered beyond our Solar System. This has had the effect of renewing interest in space exploration, which includes the possibility of sending spacecraft to explore exoplanets. Given the challenges involved, a number of advanced concepts are currently being explored, like the time-honored concept of a light sail (as exemplified by Breakthrough Starshot and similar proposals).
However, in more recent years, scientists have proposed a potentially more-effective concept known as the electric sail, where a sail composed of wire mesh generates electrical charges to deflect solar wind particles, thus generating momentum. In a recent study, two Harvard scientists compared and contrasted these methods to determine which would be more advantageous for different types of missions.
Jezero Crater on Mars. Lighter colors represent higher elevations. The Mars 2020 rover will investigate the "bathtub ring" of carbonates around the edge of the crater for microscopic fossils. The dark oval is the landing ellipse. Image NASA/MRO
Back in November 2018, NASA announced that the Mars 2020 rover would land in the Jezero Crater. Jezero Crater is a geologically diverse area, with an alluvial fan of sediment deposited by an incoming river. That sediment may contain preserved ancient organic molecules, and the deposit is clearly visible in satellite images of the Crater.
But the crater holds something else that has scientists intrigued, something that doesn’t show up so clearly in visible light images: a “bathtub ring” of carbonates, which scientists think could hold fossils.
This week we welcome Dr. Rory Barnes to the Weekly Space Hangout. Rory is an assistant professor in the Department of Astronomy and Astrobiology Program at the University of Washington. He is also a member of NASA’s Virtual Planetary Lab as well as the University of Washington’s Big Data program. He studies the habitability of exoplanets with astrophysical, geophysical, and atmospheric computer models.
In August 2019, Rory released VPLanet, an open source, virtual planet simulator that links physical processes together and enables phenomena from one region of a planetary system to be tracked throughout its entire system. Eventually, it is hoped that this will help determine if an exoplanet is capable of supporting life.
VPLanet currently includes two modules which model the internal and magnetic evolution of terrestrial planets’ characteristics. However, being open source and designed for easy growth, researchers are able to write additional physical modules which can be easily integrated with VPLanet in essentially a “plug and play” manner.
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Do you wonder how astronomers find all those exoplanets orbiting stars in distant solar systems?
Mostly they use the transit method. When a planet travels in between its star and an observer, the light from the star dims. That’s called a transit. If astronomers watch a planet transit its star a few times, they can confirm its orbital period. They can also start to understand other things about the planet, like its mass and density.
The planet Mercury just transited the Sun, giving us all an up close look at transits.
Welcome to the 637th Carnival of Space! The Carnival is a community of space science and astronomy writers and bloggers, who submit their best work each week for your benefit. We have a fantastic roundup today so now, on to this week’s worth of stories!
Two Taurid meteors from the November 2015 shower, on November 10, taken from home as part of testing the Nikon D810a and 14-24mm Nikon lens. Green airglow lights the sky, as well as horizon glows from distant lights on this very frosty and humid night for a late fall evening. This is a stack of two exposures, one for each meteor, each 60 seconds at f/2.8 and at 14mm and at ISO 800, both tracked on the AP Mach One mount. Image credit and copyright: Alan Dyer
For the northern hemisphere observers, November is fireball season. This month, keep an eye out for two sure-fire annual meteor showers, and—just maybe—a wild card outburst from the obscure Alpha Monocerotids worth watching out for.
In May of 2019, Elon Musk began delivering on his promise to create a constellation of satellites (named Starlink) that would offer broadband internet access. It all started with the launch of the first sixty Starlink satellites and was followed by Musk sending the inaugural tweet using the service this past October. Earlier today, another batch of Starlink satellites was sent into space as part of a live-streamed launch event.
The mission, known as Starlink-1, saw the launch of another 60 satellites from Space Launch Complex 40 at Cape Canaveral Air Force Station, Florida, atop a Falcon 9rocket. Unlike previous launches, this mission involved the latest version of Starlink (Starlink 1.0), which feature a number of upgrades and refinements over the previous version (Starlink 0.9) and made this mission the heaviest Starlink launch to date.
Since the mid-20th century, scientists have had a pretty good idea of how the Universe came to be. Cosmic expansion and the discovery of the Cosmic Microwave Background (CMB) lent credibility to the Big Bang Theory, and the accelerating rate of expansion led to theories about Dark Energy. Still, there is much about the early Universe that scientists still don’t know, which requires that they rely on simulations on cosmic evolution.
This has traditionally posed a bit of a problem since the limitations of computing meant that simulation could either be large scale or detailed, but not both. However, a team of scientists from Germany and the United States recently completed the most detailed large-scale simulation to date. Known as TNG50, this state-of-the-art simulation will allow researchers to study how the cosmos evolved in both detail and a large scale.
On April 18th, 2018, NASA’s Transitting Exoplanet Survey Satellite (TESS) took to space for the first time. By August, it began capturing the light curves of distant stars for signs of planetary transits, effectively picking up where the Kepler Space Telescope left off. Now, just a few months away from the end of its primary mission, NASA has put a year’s worth of images of the southern sky together to create the beautiful mosaic you see here.
Beads of rainwater on a poplar leaf act like lenses, focusing light and enlarging the leaf's network of veins. Credit: Bob King
There is no doubt that climate change is a very serious (and worsening) problem. According to a recent report by the Intergovernmental Panel on Climate Change (IPCC), even if all the industrialized nations of the world became carbon neutral overnight, the problem would continue to get worse. In short, it’s not enough to stop pumping megatons of CO2 into the atmosphere; we also have to start removing what we’ve already put there.
This is where the technique known as carbon capture (or carbon removal) comes into play. Taking their cue from nature, an international team of researchers from the University of Waterloo, Ontario, have created an “artificial leaf” that mimics the carbon-scrubbing abilities of the real thing. But rather than turning atmospheric CO2 into a source of fuel for itself, the leaf converts it into a useful alternative fuel.
