● NOAA SWPC & NASA OPEN DATA STREAM ACTIVE • TELEMETRY SYNCED
GEOMAGNETIC KpKp NaN — QUIET
SOLAR WIND SPEED418.4 km/s • Density: 5.8 p/cm³
X-RAY FLUX CLASSC1.4 • NORMAL BACKGROUND
UTC / IST DUAL SYNC • POLLING 5M
DEEP-SKY OBSERVATORY • DAILY ASTRONOMICAL PLATE
NASA Science
Credit: NASA/ESA/HubblePlate Date: 2026-10-08

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

ORBITAL FLIGHT TELEMETRY (ZARYA - 25544)

Station Ephemeris

LATITUDE / LONGITUDECALCULATING...
ORBITAL VELOCITYCALCULATING...
ALTITUDECALCULATING...
OVERPASS REGION...
● TRANSPONDER SIGNAL NOMINAL • REFRESHING 5S
CREW ROSTER IN SPACE
0 HUMANS IN ORBIT
Telemetry unavailable...
PLANETARY DEFENSE • ASTEROID CLOSE APPROACHES

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 / NAMEAPPROACH EPOCH (UTC)MISS DISTANCE (LD / KM)RELATIVE VELOCITYESTIMATED DIAMETERHAZARD CLASSIFICATION
(513312 (2007 DM41))2026-Oct-08 14:27
64.81 LD
~24,922,544 km
12.14 km/s103m – 230mPOTENTIALLY HAZARDOUS (PHA)
((2007 TH3))2026-Oct-08 07:39
131.11 LD
~50,420,385 km
14.68 km/s31m – 68mBENIGN FLYBY
((2009 UU1))2026-Oct-08 08:47
116.52 LD
~44,809,138 km
18.91 km/s31m – 68mBENIGN FLYBY
((2015 TS238))2026-Oct-08 17:12
4.72 LD
~1,813,910 km
15.81 km/s22m – 49mBENIGN FLYBY
((2018 HO1))2026-Oct-08 13:33
148.15 LD
~56,973,735 km
8.47 km/s23m – 52mBENIGN FLYBY
Data Methodology: Heliospheric telemetry syndicated via the National Oceanic and Atmospheric Administration Space Weather Prediction Center (NOAA SWPC). Near-Earth Asteroid orbits and orbital ephemerides derived from NASA Jet Propulsion Laboratory (JPL) Small-Body Database and CNEOS NeoWs. Orbital station telemetry calculated via NORAD Two-Line Element sets.
Endpoints: NOAA/SWPC-JSON • NASA/NeoWs-v1 • Revalidation: 300s
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