
NASA Science
How was the Saturn system imaged so clearly? Astrophotographer Tom Williams captured such exquisite details due to one night of exceptional atmospheric conditions above the United Kingdom. This means more than a cloudless sky. Pockets of air at different temperatures and densities move around and bend light as it travels through Earth’s atmosphere, distorting astronomy images. This is called “seeing.” Less atmospheric turbulence means clearer images. The astrophotographer reduced the impact of seeing with the lucky imaging technique: thousands of short-exposure images are taken very quickly with a high-speed camera and the clearest images are added up. Which object in this smörgåsbord interests you? Perhaps Titan or the icy stripes of Enceladus? Maybe the gaps and spokes in Saturn’s rings? Saturn's opposition, when Earth passes in between the planet and the Sun, occurred on October 4th. Due to the planet's proximity and full illumination from the Sun, now is a great time of year to observe it!Tomorrow's picture: bumpy
Station Ephemeris
Near-Earth Object (NEO) Radar Ledger
Ephemeris calculations and close-approach telemetry for near-Earth asteroids detected within 10 lunar distances, compiled from NASA's Center for Near Earth Object Studies (CNEOS).
| DESIGNATION / NAME | APPROACH EPOCH (UTC) | MISS DISTANCE (LD / KM) | RELATIVE VELOCITY | ESTIMATED DIAMETER | HAZARD CLASSIFICATION |
|---|---|---|---|---|---|
| (513312 (2007 DM41)) | 2026-Oct-08 14:27 | 64.81 LD ~24,922,544 km | 12.14 km/s | 103m – 230m | POTENTIALLY HAZARDOUS (PHA) |
| ((2007 TH3)) | 2026-Oct-08 07:39 | 131.11 LD ~50,420,385 km | 14.68 km/s | 31m – 68m | BENIGN FLYBY |
| ((2009 UU1)) | 2026-Oct-08 08:47 | 116.52 LD ~44,809,138 km | 18.91 km/s | 31m – 68m | BENIGN FLYBY |
| ((2015 TS238)) | 2026-Oct-08 17:12 | 4.72 LD ~1,813,910 km | 15.81 km/s | 22m – 49m | BENIGN FLYBY |
| ((2018 HO1)) | 2026-Oct-08 13:33 | 148.15 LD ~56,973,735 km | 8.47 km/s | 23m – 52m | BENIGN FLYBY |