In 2011, scientists confirmed a suspicion: There was a split in the local cosmos. Samples of the solar wind brought back to Earth by the Genesis mission definitively determined oxygen isotopes in the sun differ from those found on Earth, the moon and the other planets and satellites in the solar system.

Early in the solar system's history, material that would later coalesce into planets had been hit with a hefty dose of ultraviolet light, which can explain this difference. Where did it come from? Two theories emerged: Either the ultraviolet light came from our then-young sun, or it came from a large nearby star in the sun's stellar nursery.

Now, researchers from the lab of Ryan Ogliore, assistant professor of physics in Arts & Sciences at Washington University in St. Louis, have determined which was responsible for the split.

This is the main camera that ESA's Hera mission for planetary defense will be relying on to explore and maneuver around the Didymos asteroid system.

Hera—named after the Greek goddess of marriage—will be, along with NASA's Double Asteroid Redirect Test (DART) spacecraft, humankind's first probe to rendezvous with a binary asteroid system, a little understood class making up around 15% of all known asteroids.

The DART spacecraft—due for launch this November—will first perform a kinetic impact on the smaller of the two bodies. Hera will follow-up with a detailed post-impact survey to turn this grand-scale experiment into a well-understood and repeatable asteroid deflection technique.

Produced by Jena-Optronik in Germany, this lightweight camera is being supplied to OHB System AG, leading the Hera industrial consortium for ESA. The camera will be used both for spacecraft navigation and scientific study of the two asteroids' surfaces.

The camera is based on Jena-Optronik's existing ASTROhead design. ASTROhead has already been proven in space, aboard Northrop Grumman's Mission Extension Vehicle, MEV-1 in 2019, helping it perform a historic autonomous docking with a geostationary telecommunication satellite in order to extend the satellite's working lifetime.

When 'Oumuamua, the first interstellar object ever observed passing through the solar system, was discovered in 2017, it exhibited some unexpected properties that left astronomers scratching their heads. Its elongated shape, lack of a coma, and the fact that it changed its trajectory were all surprising, leading to several competing theories about its origin: was it a hydrogen iceberg exhibiting outgassing, or maybe an extraterrestrial solar sail (sorry folks, not likely) on a deep-space journey? We may never know the answer, because 'Oumuamua was moving too fast, and was observed too late, to get a good look.

It may be too late for 'Oumuamua, but we could be ready for the next strange interstellar visitor if we wanted to. A spacecraft could be designed and built to catch such an object at a moment's notice. The idea of an interstellar interceptor like this has been floated by various experts, and funding to study such a concept has even been granted through NASA's Innovative Advanced Concepts (NIAC) program. But how exactly would such an interceptor work?