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Live sky
Observer context
Calculated from the Sun's position for 34.93°S 138.60°E.
Sunset is the moment the Sun's centre drops below the horizon. Astronomical darkness (Sun 18° below) is when faint nebulae and the Milky Way become visible from a dark site. Moon illumination is the fraction of the disc lit, not how bright the sky will be — a 30% moon still washes out faint targets.
International Space Station
Geometric passes above 10° elevation. A pass is only visible if the station is in sunlight while your sky is dark.
News & discoveries
Space weather
Planetary K-index
A 3-hourly planetary average of geomagnetic disturbance.
Kp is a 0–9 scale of geomagnetic disturbance, computed every three hours from magnetometer stations worldwide. Below 4 is quiet. At 5 the storm reaches G1: high-latitude aurora and minor power-grid effects. At 7 or above it is a severe storm. Aurora chasing is a lie detector — Kp forecasts change, and the site always shows the observed value, not a prediction.
The solar wind carries a magnetic field. When its north–south component (Bz) turns negative, it couples with Earth's magnetic field and energy pours in. A fast wind with positive Bz usually does nothing dramatic; a slower wind with strongly negative Bz can light up the aurora. That is why both are plotted.
Imagery
The wider universe
Nancy Grace Roman Space Telescope
Commissioning Roman is in space and being switched on, one instrument at a time.
Launched 30 August 2026. NASA reports Roman is completing commissioning; the first science images are still ahead of us.
When those images arrive, this section becomes the place to see them at full resolution — a mirror the size of Hubble's, with roughly a hundred times the sky in every exposure.
Official mission page ↗ Roman blog ↗
Roman's own science images do not exist yet. Nothing on this page is presented as Roman imagery.
Discussion
Provenance