A new study shows how changes in ocean circulation could reshape global rainfall patterns. A storm reaching California can begin with changes thousands of miles away in the Atlantic Ocean. Climate modeling suggests that as one of the planet’s major ocean circulation systems weakens, more moisture could be directed toward the West Coast while snowfall [...]
It's a shameful day for the Church of England, says Julian Mann, as its General Synod passes an anti-Israel motion pledging to "engage with" what the Chief Rabbi calls a "shocking" document containing "so much falsehood".
The post A Shameful Day for the Church of England appeared first on The Daily Sceptic.
The Japanese government wants to sharply increase the number of launches despite struggles with both current and new launch vehicles.
The post Japan seeks to ramp up launch activity appeared first on SpaceNews.
The School of Science has announced the winners of its 2025 Awards for Excellence in Teaching and Mentoring. This year, the Teaching Prizes were restructured to acknowledge early- and mid-career teaching excellence, in addition to an overall prize for teaching excellence that includes instructors and non-tenured instructors or lecturers.
Olivia Corradin, assistant professor of biology and a member of the Whitehead Institute for Biomedical Research, received an Award for Teaching Excellence. Corradin’s nominators emphasized that she is an exceptionally clear and engaging educator.
Julien Tailleur, associate professor of physics, received an Award for Excellence in Mentoring and Advising in recognition of his dedication to mentorship. Nominators describe Tailleur as an outstanding research supervisor and group leader who cultivates an open and respectful environment.
John Urschel, Class of 1956 Career Development Assistant Professor of Mathematics, received an Award for Teaching Excellence. Many students call Urschel the best instructor they have had and their favorite professor at MIT, noting that he cares greatly about his students’ success and shows them why linear algebra is “so cool.”
Recipients of the School of Science Awards for Excellence in Teaching and Mentoring were honored alongside School of Science Infinite Expansion and Mile Award winners at a celebratory luncheon.
The School of Science welcomes nominations for the teaching prize at the end of each semester. Nominations can be submitted to the School.
The post Three win School of Science Awards for Excellence in Teaching and Mentoring appeared first on MIT School of Science.
The British government is preparing to release a new space strategy that will provide a “whole-of-government” approach for space in the country.
The post U.K. government preparing to release new space strategy appeared first on SpaceNews.
Using the upgraded GRAVITY+ instrument on ESO’s Very Large Telescope Interferometer (VLTI), astronomers have measured the ratio of carbon isotopes in the atmosphere of the young exoplanet Beta Pictoris, offering new insights into how giant planets form.
The post Astronomers Probe Chemistry of Giant Exoplanet Beta Pictoris b appeared first on Sci.News: Breaking Science News.
The post Summer 2026 recommended reading from MIT appeared first on MIT School of Science.
When you think of an asteroid impact, you’re probably imagining something like the cataclysmic event that nearly wiped out the dinosaurs. In an astonishingly rare event, a rock the size of the island of Manhattan could come hurtling from deep space towards Earth and destroy the world.
On the contrary, asteroids are generally leftover debris from the primordial solar system that didn’t become part of a larger body, like a planet or moon, and they’re not particularly rare. Scientists estimate that there are about 1 billion asteroids and comets classified as near-Earth objects, or NEOs. NEOs are generally much smaller than the asteroid that killed the dinosaurs. They range from weakly held-together piles of rubble 200 meters (700 feet) across, to the minuscule 2024 BX1, approximately 44 centimeters (17 inches) across.
For several decades, astronomical surveys of the sky have looked for these asteroids. NASA’s Center for Near-Earth Object Studies (CNEOS) Fireball and Bolide Database has records of over 1,000 incidents of objects colliding with our planet since the mid-1990s. Among these is a set of 11 objects that scientists detected before they hit Earth, known as imminent impactors. Finding imminent impactors allows scientists unique opportunities to study the smallest building blocks of the solar system, enabling them to learn more about asteroid composition, structure, and history.
A team of scientists recently conducted a study on how the newly built Vera Rubin Observatory could detect more imminent impactors before they strike Earth. They examined the CNEOS Fireball and Bolide Database impact records spanning February 1, 1994, to January 1, 2026, for records of the asteroids’ coordinates, velocities, and the energy they released at the time of collision.
They found that 343 NEOs met this criterion, including 5 known imminent impactors. Using these recorded data, they reconstructed the objects’ pre-impact characteristics. The team predicted the asteroids’ orbital paths from the recorded coordinates and velocity. Assuming the objects were spherical, they estimated the size from velocity and impact energy. From this information about the asteroids’ state before impact, the team could then simulate whether the Rubin Observatory would have detected them.
When small asteroids hit Earth, they mostly burn up in the atmosphere, producing a bright flash that is relatively easy to spot compared to when they are in space. The Rubin Observatory can see objects up to 10 billion times dimmer than the brightest star in the night sky, Sirius. To predict if the Rubin Observatory can detect dim NEOs, the team used the solar system simulator SORCHA. SORCHA takes an observatory’s specifications and the physical properties of the NEOs and uses these to determine whether the observatory could detect them. It also estimates the measured sizes and speeds of the NEOs, and predicts when the observatory would have seen them.
At the Rubin Observatory, an imminent impactor is considered discovered if it’s observed at least 3 separate times over 15 days before hitting Earth. So this team applied this same criterion to their simulation. They found that of their 343 impactors, SORCHA estimated that the Rubin Observatory would have discovered 14 of them before impact.
They also found that SORCHA predicted 4 additional impactors that could have been observed at least once, potentially allowing scientists to search other telescope data for evidence of their existence in pre-collision images. Based on these results, the team estimated that the Rubin Observatory could find 4% of all objects longer than 1 meter (3 feet) before they hit Earth. This percentage of discovery translates to 1 to 2 imminent impactors detected every year, at least double their current discovery rate.
The ability to more consistently find imminent impactors would allow researchers to study the smallest pieces of the solar system in detail and to draw general conclusions about the properties of objects that could potentially collide with Earth. This would also allow scientists to more accurately calculate the orbits of imminent impactors, determine where more meteorites land to recover them, and keep tabs on the extremely rare but more hazardous large impactors for planetary defense initiatives. So, humanity can learn more about the ancient solar system, and hopefully avoid going the way of the dinosaurs while doing so!
The post How many asteroids can we detect before they hit Earth? appeared first on Sciworthy.
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