The article “Revolutionizing Our Knowledge: The Rubin Observatory’s Groundbreaking Discoveries in the Solar System” reveals that millions of new solar system objects will be detected by the NSF-DOE Vera C. Rubin Observatory, set to revolutionize our knowledge of the solar system’s small bodies – asteroids, comets, and other minor planets.

A team of astronomers from across the globe, led by Queen’s University Belfast, created Sorcha, an innovative new open-source software used to predict what discoveries are likely to be made. Sorcha is the first end-to-end simulator that ingests Rubin’s planned observing schedule, applying assumptions on how Rubin Observatory sees and detects astronomical sources in its images with the best model of what the solar system and its small body reservoirs look like today.

The team’s simulations show that Rubin will map:

* 127,000 near-Earth objects – asteroids and comets whose orbits cross or approach Earth. This will cut the risk of undetected asteroid impact of catastrophic proportions by at least two times.
* Over 5 million main-belt asteroids, up from about 1.4 million, with precise color and rotation data on roughly one in three asteroids within the survey’s first years.
* 109,000 Jupiter Trojans, bodies sharing Jupiter’s orbit at stable “Lagrange” points – more than seven times the number cataloged today.
* 37,000 trans-Neptunian objects, residents of the distant Kuiper Belt – nearly 10 times the current census.
* Approximately 1,500-2,000 Centaurs, bodies on short-lived giant planet-crossing orbits in the middle solar system.

The Rubin Observatory’s Legacy Survey of Space and Time (LSST) is a once-in-a-generation opportunity to fill in the missing pieces of our solar system. With this data, we’ll be able to update the textbooks of solar system formation and vastly improve our ability to spot – and potentially deflect – the asteroids that could threaten Earth.

The Sorcha code is open-source and freely available with the simulated catalogs, animations at https://sorcha.space. By making these resources available, the Sorcha team has enabled researchers worldwide to refine their tools and be ready for the flood of LSST data that Rubin will generate, advancing the understanding of the small bodies that illuminate the solar system like never before.

The James Webb Space Telescope (JWST) has provided new clues about how the ultra-hot exoplanet WASP-121b was formed and where it might have originated in the disc of gas and dust around its star. The detection of multiple key molecules, including water vapour, carbon monoxide, silicon monoxide, and methane, has allowed a team of astronomers to compile an inventory of the carbon, oxygen, and silicon in the atmosphere of WASP-121b.

The ultra-hot giant planet orbits its host star at a distance only about twice the star’s diameter, completing one orbit in approximately 30.5 hours. The planet exhibits two distinct hemispheres: one that always faces the host star, with temperatures locally exceeding 3000 degrees Celsius, and an eternal nightside where temperatures drop to 1500 degrees.

The team led by astronomers Thomas Evans-Soma and Cyril Gapp was able to compile an inventory of the carbon, oxygen, and silicon in the atmosphere of WASP-121b. The detection of these molecules suggests that the planet’s atmosphere is rich in gases that are stable at high temperatures.

However, the team’s observations also revealed a surprise: the abundance of methane on the nightside of the exoplanet was much higher than expected. To explain this result, the team proposes that methane gas must be rapidly replenished on the nightside to maintain its high abundance. A plausible mechanism for doing this involves strong vertical currents lifting methane gas from lower atmospheric layers.

The JWST’s Near-Infrared Spectrograph (NIRSpec) was used to observe WASP-121b throughout its complete orbit around its host star. As the planet rotates on its axis, the heat radiation received from its surface varies, exposing different portions of its irradiated atmosphere to the telescope. This allowed the team to characterize the conditions and chemical composition of the planet’s dayside and nightside.

The astronomers also captured observations as the planet transited in front of its star. During this phase, some starlight filters through the planet’s atmospheric limb, leaving spectral fingerprints that reveal its chemical makeup. The emerging transmission spectrum confirmed the detections of silicon monoxide, carbon monoxide, and water that were made with the emission data.

The MPIA scientists involved in this study included Thomas M. Evans-Soma (also at the University of Newcastle, Australia), Cyril Gapp (also at Heidelberg University), Eva-Maria Ahrer, Duncan A. Christie, Djemma Ruseva (also at the University of St Andrews, UK), and Laura Kreidberg.

Other researchers included David K. Sing (Johns Hopkins University, Baltimore, USA), Joanna K. Barstow (The Open University, Milton Keynes, UK), Anjali A. A. Piette (University of Birmingham, UK and Carnegie Institution for Science, Washington, USA), Jake Taylor (University of Oxford, UK), Joshua D. Lothringer (Space Telescope Science Institute, Baltimore, USA and Utah Valley University, Orem, USA), and Jayesh M. Goyal (National Institute of Science Education and Research (NISER), Odisha, India).

The JWST’s role in the discovery was crucial, as it allowed the team to observe WASP-121b throughout its complete orbit around its host star, capturing a wealth of information about the exoplanet’s atmosphere and composition.

In conclusion, the study provides new insights into the formation and evolution of ultra-hot exoplanets like WASP-121b. The detection of methane on the nightside of the exoplanet challenges current dynamical models of exoplanetary atmospheres, suggesting that these models will need to be adapted to reproduce the strong vertical mixing observed in this study.

The world of black holes has long been divided into three categories: stellar-mass black holes (about five to 50 times the mass of the sun), supermassive black holes (millions to billions of times the mass of the sun), and intermediate-mass black holes with masses somewhere in between. While we know that intermediate-mass black holes should exist, little is known about their origins or characteristics – they are considered the rare “missing links” in black hole evolution.

However, four new studies have shed new light on this mystery. The research was led by a team in the lab of Assistant Professor Karan Jani, who also serves as the founding director of the Vanderbilt Lunar Labs Initiative. The work was funded by the National Science Foundation and the Vanderbilt Office of the Vice Provost for Research and Innovation.

The primary paper, “Properties of ‘Lite’ Intermediate-Mass Black Hole Candidates in LIGO-Virgo’s Third Observing Run,” was published in Astrophysical Journal Letters and led by Lunar Labs postdoctoral fellow Anjali Yelikar and astrophysics Ph.D. candidate Krystal Ruiz-Rocha. The team reanalyzed data from the Nobel-Prize winning Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors in the U.S. and the Virgo detector in Italy.

The researchers found that these waves corresponded to mergers of black holes greater than 100 to 300 times the mass of the sun, making them the heaviest gravitational-wave events recorded in astronomy. “Black holes are the ultimate cosmic fossils,” Jani said. “The masses of black holes reported in this new analysis have remained highly speculative in astronomy. This new population of black holes opens an unprecedented window into the very first stars that lit up our universe.”

Earth-based detectors like LIGO capture only a split second of the final collision of these “lightweight” intermediate-mass black holes, making it challenging to determine how the universe creates them. To tackle this, Jani’s lab turned to the upcoming European Space Agency and NASA’s Laser Interferometer Space Antenna (LISA) mission, launching in the late 2030s.

In two additional studies published in Astrophysical Journal, “A Sea of Black Holes: Characterizing the LISA Signature for Stellar-origin Black Hole Binaries,” led by Ruiz-Rocha, and “A Tale of Two Black Holes: Multiband Gravitational-wave Measurement of Recoil Kicks,” led by former summer research intern Shobhit Ranjan, the team showed LISA can track these black holes years before they merge, shedding light on their origin, evolution, and fate.

Detecting gravitational waves from black hole collisions requires extreme precision – like trying to hear a pin drop during a hurricane. In a fourth study also published in Astrophysical Journal, “No Glitch in the Matrix: Robust Reconstruction of Gravitational Wave Signals under Noise Artifacts,” the team showcased how artificial intelligence models guarantee that signals from these black holes remain uncorrupted from environmental and detector noise in the data. The paper was led by postdoctoral fellow Chayan Chatterjee and expands upon Jani’s AI for New Messengers Program, a collaboration with the Data Science Institute.

“We hope this research strengthens the case for intermediate-mass black holes as the most exciting source across the network of gravitational-wave detectors from Earth to space,” Ruiz-Rocha said. “Each new detection brings us closer to understanding the origin of these black holes and why they fall into this mysterious mass range.”

Moving forward, Yelikar said the team will explore how intermediate-mass black holes could be observed using detectors on the moon.

“Access to lower gravitational-wave frequencies from the lunar surface could allow us to identify the environments these black holes live in – something Earth-based detectors simply can’t resolve,” she said.

In addition to continuing this research, Jani will also be working with the National Academies of Sciences, Engineering, and Medicine on a NASA-sponsored study to identify high-value lunar destinations for human exploration to address decadal-level science objectives. As part of his participation in this study, Jani will be contributing to the Panel on Heliophysics, Physics, and Physical Science, to identify and articulate the science objectives related to solar physics, space weather, astronomy, and fundamental physics that would be most enabled by human explorers on the moon.

“This is an exciting moment in history – not just to study black holes, but to bring scientific frontiers together with the new opportunity of training the next generation of students whose discoveries will be shaped by, and made from, the moon,” Jani said.