Observatoryspace.joelcornish.com
--:-- Adelaide

Observatory

The sky, as it is
tonight.

Launches, space weather, telescope imagery and mission status — gathered from NASA, ESA, NOAA and The Space Devs, refreshed while you watch.

Launch centre

What leaves the ground next

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Live sky

Tonight, over Adelaide

Orbit propagated locally from CelesTrak elements

Observer context

    Calculated from the Sun's position for 34.93°S 138.60°E.

    What these mean

    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

    Where is it right now?

    Passes over Adelaide, next 24 hours

      Geometric passes above 10° elevation. A pass is only visible if the station is in sunlight while your sky is dark.

      News & discoveries

      What the sky is telling us

      Headlines and links only — the publishers keep the articles.

        Space weather

        The Sun's mood, measured

        NOAA SWPC · near-real-time

        Planetary K-index

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        A 3-hourly planetary average of geomagnetic disturbance.

        Geomagnetic activity (Kp)last ~7 days · 3-hourly
        Solar windspeed, last 8 hours · km/s
        Interplanetary magnetic field, BznT · negative means energy can enter Earth's field
        Solar X-ray fluxlast 6 hours · flare classes
        How to read the Kp index

        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.

        Why Bz matters more than speed

        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

        Light worth travelling for

        NASA Image & Video Library · archival

        The wider universe

        Machines that look outward

        Curated mission reference · live numbers where the source allows

        Nancy Grace Roman Space Telescope

        A wider eye on the dark universe

        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.

          Latest official updates

            Discussion

            Talk about it

            Provenance

            Where every number comes from