40th Rocket Lab Electron Mission, “We Love The Nightlife”, Launches From New Zealand with Reused Engine

Rocket Lab’s 40th Electron mission, “We Love The Nightlife”, lifted-off from New Zealand’s Mahia Peninsula on August 24th at 11:45 am NZST (August 23rd at 7:45pm EST). (Credit: Rocket Lab)

Private space company, Rocket Lab, launched its 40th Electron mission on their lauded Electron rocket, dubbed “We Love The Nightlife”, on August 24th at 11:45am New Zealand Standard Time (August 23rd at 7:45pm EST), which also marks the 7th launch of 2023, all successful. The purpose of the mission was to deliver the next-generation Acadia satellite for Capella Space to a circular orbit above the Earth at 640 km (400 miles), which was executed flawlessly. Acadia is part of Capella’s synthetic aperture radar (SAR) constellation and is the first of four Acadia satellites that Rocket is currently contracted to launch for Capella.

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Dr. Tracy Becker Honored with 2023 Carl Sagan Medal for Science Communication

2023 Carl Sagan Medal recipient, Dr. Tracy Becker, who is a group leader in the Southwest Research Institute’s Space Science Division. Dr. Becker is a planetary scientist whose research interests include remote observations of space phenomena such as the asteroid system shown here. (Credit: Southwest Research Institute)

This year’s prestigious Carl Sagan Medal, also known as the “Sagan Medal” and named after the late astronomer, Dr. Carl Sagan, has been awarded to Dr. Tracy Becker, who is a planetary scientist in the Space Science Division of the Southwest Research Institute (SwRI) in San Antonio, Texas. The Sagan Medal recipient is chosen by the Division for Planetary Sciences of the American Astronomical Society (AAS) and is meant to acknowledge planetary scientists who are not only active in science communication with the general public but have taken enormous strides in helping the general public better understand, and get excited for, the field of planetary science.

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Watch an Actual Exoplanet Orbit its Star for 17 Years

Artist rendition of exoplanet, Beta Pictoris b, whose partial orbit was recently featured in a time-lapsed video. (Credit: ESO L. Calçada/N. Risinger)

Searching for exoplanets is incredibly difficult given their literal astronomical distances from Earth, which is why a myriad of methods have been created to find them. These include transit, redial velocity, astrometry, gravitational microlensing, and direct imaging. It is this last method that was used to recently create a time-lapse video that compresses a mind-blowing 17 years of the partial orbit of exoplanet, Beta Pictoris b, into 10 seconds. The data to create the video was collected between 2003 and 2020, it encompasses approximately 75 percent of the total orbit, and marks the longest time-lapse video of an exoplanet ever produced.

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This Jupiter-Sized Exoplanet is Unusual for Several Reasons

Artist illustration of a warm Jupiter gas-giant exoplanet (right) orbiting its parent star, along with several smaller exoplanets. (Credit: Detlev Van Ravenswaay/Science Photo Library)

In a recent study published in the Monthly Notices of the Royal Astronomical Society, a team of international researchers examined exoplanet TOI-4860 b, which is located approximately 80 parsecs (261 light-years) from Earth and has an orbital period of approximately 1.52 days around a low-mass star, or a star smaller than our Sun. Exoplanets orbiting so close to their parent stars aren’t uncommon and commonly known as “hot Jupiters”.

However, TOI-4860 b is unique due its relative size compared to its parent star, along with its lower surface temperatures compared to “hot Jupiters” and possessing large amounts of heavy elements. These attributes are why researchers are classifying TOI-4680 b as a “warm Jupiter”, and could challenge traditional planetary systems formation models while offering new insights into such processes, as well.

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Interpreting Dune Patterns: Insights from Earth and Mars

Examples of active dune fields within Nili Patera on Mars. Dunes like these were examined for this study in hopes of giving scientists better insights into how their interactions are influenced by a planet’s climate. (Credit: NASA/JPL-Caltech/Univ. of Arizona)

A recent study published in the journal Geology attempts to interpret the patterns of dunes, which are sand mounds frequently formed by aeolian (wind) processes and range in size from small ripples observed on beaches to massive structures observed in the desert. Specifically, the researchers focused on patterns of dune crestlines, which are the top of the dunes. Different dune crestline patterns might appear as mundane features, but their formations are often the result of a myriad of influences, including climate change, surface processes, and atmospheric phenomena.

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China’s Chang’e-7 Will Deploy a Hopper that Jumps into a Crater in Search of Water Ice

Artist rendition of potential future facilities on the lunar surface. (Credit: CFP)

Researchers from the Chinese Academy of Sciences and the Chinese National Space Administration recently published a study in the journal Space: Science & Technology outlining how the upcoming Chang’e-7 mission, due to launch in 2026, will use a combination of orbital observations and in-situ analyses to help identify the location, amount, and dispersion of water-ice in the permanently-shadowed regions (PSRs) of the Moon, specifically at the lunar south pole.

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Jupiter’s Moons Get the JWST Treatment

Spectroscopic map of Ganymede (left) obtained from JWST’s Near-Infrared Spectrograph (NIRSpec) instrument displaying light absorption in the polar regions distinctive of the molecule hydrogen peroxide. A JWST NIRSpec infrared image of Io (right) displaying volcanic eruptions at Kanehekili Fluctus (center) and Loki Patera (right) with temperatures up to 1200 Kelvin (926.85 degrees Celsius/1700 degrees Fahrenheit). Circles indicate the surfaces of both moons. (Credit: Ganymede: Cornell/Dr. Samantha Trumbo; Io: UC Berkeley/Dr. Imke de Pater)

A pair of studies published in JGR: Planets and Science Advances discuss new findings from NASA’s James Webb Space Telescope (JWST) regarding Jupiter’s first and third Galilean Moons, Io and Ganymede, and more specifically, how the massive Jupiter is influencing activity on these two small worlds. For Io, whose mass is about 21 percent larger than Earth’s Moon, the researchers made the first discovery of sulfur monoxide (SO) gas on the volcanically active moon. For Ganymede, which is the largest moon in the solar system and boasts twice the mass of the Earth’s Moon, the researchers made the first discovery of hydrogen peroxide, which exists in Ganymede’s polar regions.

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NASA is Working on Technology to 3D Print Circuits in Space

Image of a 3D-printed circuit on display during the Goddard Field Day event that launched on the Suborbital Technology Experiment Carrier-9 (SubTEC-9) technology test flight from NASA's Wallops Flight Facility in April 2023. (Credit: NASA/Karl B. Hille)

A collaboration of engineers from NASA and academia recently tested hybrid printed electronic circuits near the edge of space, also known as the Kármán line. The space-readiness test was demonstrated on the Suborbital Technology Experiment Carrier-9, or (SubTEC-9), sounding rocket mission, which was launched from NASA’s Wallops Flight Facility on April 25 and reached an altitude of approximately 174 kilometers (108 miles), which lasted only a few minutes before the rocket descended to the ground via parachute.

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Have We Seen the First Glimpse of Supermassive Dark Stars?

Three dark star candidates, JADES-GS-z13-0 (top), JADES-GS-z12-0 (middle), and JADES-GS-z11-0 (bottom) were originally identified as galaxies by the JWST Advanced Deep Extragalactic Survey (JADES) team. Recently, a team of researchers have hypothesized these candidates could be “dark stars,” which are theoretical objects far more massive and brighter than our sun, and allegedly powered by demolishing particles of dark matter. (Credit: NASA/European Space Agency)

A recent study published in the Proceedings of the National Academy of Sciences (PNAS) examines what are known as dark stars, which are estimated to be much larger than our Sun, are hypothesized to have existed in the early universe, and are allegedly powered by the demolition of dark matter particles. This study was conducted using spectroscopic analysis from NASA’s James Webb Space Telescope (JWST), and more specifically, the JWST Advanced Deep Extragalactic Survey (JADES), and holds the potential to help astronomers better understand dark stars and the purpose of dark matter, the latter of which continues to be an enigma for the scientific community, as well as how it could have contributed to the early universe.

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There Could be Trillions of Rogue Planets Wandering the Milky Way

Artist's rendition of an ice-encrusted, Earth-mass rogue planet free-floating through space. (Credit: NASA’s Goddard Space Flight Center)

A pair of new studies set to be published in The Astronomical Journal examine new discoveries in the field of rogue planets, which are free-floating exoplanets that drift through space unbound by the gravitational tug of a star. They can form within their own solar system and get ejected, or they can form independently, as well. The first study examines only the second discovery of an Earth-mass rogue planet—the first being discovered in September 2020—while the second study examines the potential number of rogue planets that could exist in our Milky Way Galaxy.

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