The spacecraft would circumnavigate Venus every four to six days, with solar panels charging every two to three days on the side of planet illuminated by the sun. Credit: CRASH Lab, University at Buffalo.
Venus is colloquially referred to as “Earth’s Twin”, owing to the similarities it has with our planet. Not surprisingly though, there is a great deal that scientists don’t know about Venus. Between the hot and hellish landscape, extremely thick atmosphere, and clouds of sulfuric rain, it is virtually impossible to explore the planet’s atmosphere and surface. What’s more, Venus’ slow rotation makes the study of its “dark side” all the more difficult.
However, these challenges have spawned a number of innovative concepts for exploration. One of these comes from the University of Buffalo’s Crashworthiness for Aerospace Structures and Hybrids (CRASH) Laboratory, where researchers are designing a unique concept known as the Bio-inspired Ray for Extreme Environments and Zonal Explorations (BREEZE).
Neptune's moons Naiad and Thalassa are locked in a lunar dance. Image Credit: NASA/JPL
Like a long-married couple accustomed to each other’s kitchen habits, two of Neptune’s moons are masters at sharing space without colliding. And though both situations may appear odd to an observer, there’s a certain dance-like quality to them both.
Rev. Nick Miles, of the Pamunkey Tribe, opens the 2014 MU69/Arrokoth naming ceremony at NASA Headquarters with a traditional Algonquian song. Credits: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute
On July 14th, 2015, the New Horizons made the first-ever flyby of Pluto. As if that wasn’t enough, the mission made history again with the flyby of the Kuiper Belt Object (KBO) 2014 MU69 on December 31st, 2018. This constituted the farthest encounter from Earth with a celestial object, which the team had nicknamed Ultima Thule – a mythical northern island beyond the borders of the known world in Medieval literature.
Unfortunately, this name has generated some controversy due to the fact that it is also the name white supremacists use to refer to a mythical homeland. So with the consent of the tribal elders and representatives of the Powhatan nations, the New Horizons’ team recommended a new name for the KBO. Henceforth, it will be known as “Arrokoth“, the word for “sky” in the Powhatan/Algonquian language.
These images show some of the exoplanet host stars with companion stars (B, C) that were found during the project. The images are RGB composite images taken with the Panoramic Survey Telescope and Rapid Response System (PanSTARRS) in the y- (960 nm), i- (760 nm), and g-band (480 nm). The image in the middle shows a hierarchical triple star system.
Image: Mugrauer, PanSTARRS
Right now, we know of about 4,000 confirmed exoplanets, mostly thanks to the Kepler mission. TESS, the Transiting Exoplanet Survey Satellite, will likely raise that 4000 by a lot. But what about the stars that all of these planets orbit?
A new study from the Astrophysical Institute and University Observatory of the University of Jena identified over 200 exoplanets that exist in multiple star systems. The study is part of the effort to understand how host stars shape the formation and evolution of planets.
Artist's impression of the Hayabusa2 taking samples from the surface of the asteroid Ryugu. Credit: Akihiro Ikeshita/JAXA
Japan’s Hayabusa 2 spacecraft is on its way home. The asteroid-visiting, sample-return mission departed asteroid Ryugu (162173 Ryugu) on Wednesday, beginning its year-long journey back to Earth. And it’s carrying some precious cargo.
Apollo 12's launch in 1969, moments before the rocket was struck by lightning. Credit: NASA
The 50th anniversary of Apollo 11 was a huge celebration, and Apollo 13 may be an equally big commotion. Apollo 12 is tough sell in the middle. Even the Virginia Air & Space Center, which houses the Apollo 12 capsule, uses photographs of Apollo 11 to advertise. Ouch.
This unique mission and its important contribution to science was no less an accomplishment than its famous predecessor or tragic follower, and it pains many to see them become the “lost” journey between two better-known missions, with no movie to dramatize the details of their voyage.
An atmospheric drama has been playing out on Mars lately. Up until now, the main actor has been methane, and its unusual, spiking behaviour. But now Oxygen is taking the stage, and performing some theatrics of its own.
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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