We found our first potentially hazardous asteroid, 2022 SF289, using the HelioLinC3D code that will power
@VRubinObs
's LSST survey!! Written by
@uwdirac
's Ari Heinze, the new code can identify asteroids with half the observations as needed before. . 🧵 👇
@VRubinObs
@uwdirac
The solar system is home to millions of rocky bodies ranging from small asteroids a few feet in diameter, to dwarf planets the size of our moon. These objects remain from an era over four billion years ago, when the planets formed.
@VRubinObs
@uwdirac
Most of them are distant, but a number orbit close to the Earth. These are known as Near-Earth Objects (NEOs). The closest of these - whose trajectories takes them within ~5 million miles of the Earth's orbit - warrant special attention.
@VRubinObs
@uwdirac
The large, very nearby, objects are known as "Potentially Hazardous Asteroids" (PHAs). They're systematically searched for and monitored to ensure they won’t collide with the Earth. Such an impact would make for a /really/ bad day (or a millennium)...
@VRubinObs
@uwdirac
@NASA
@atlas_ifa
@UHIfA
To find asteroids, ATLAS takes images of parts of the sky at least four times every night. A discovery is made when they notice a point of light moving unambiguously in a straight line over the image series.
@VRubinObs
@uwdirac
@NASA
@atlas_ifa
@UHIfA
@NSF
@doescience
To be even more efficient, it will visit spots on the sky just twice each night rather than the four times needed by present telescopes. But with this novel observing cadence, we need a new type of discovery algorithm to reliably spot space rocks.