Supermassive Jets and Asteroid 2026 TP6

On 2026-10-11, the Earth’s magnetosphere endured a significant period of unrest. The Kp index climbed to a peak of 6.7, classified as a G2 geomagnetic storm, before stabilising to a quiet level of 3 by the end of the day. This disturbance was driven by solar wind speeds reaching 677 km/s, coupled with a southward-pointing interplanetary magnetic field (Bz) of 10.4 nT. While these conditions often trigger vibrant displays, the aurora power dissipated to 0 GW as the storm lost its momentum. Satellite data from NOAA SWPC confirmed that the solar disc remained relatively subdued, producing only a minor C-class flare.

Conditions in the near-Earth environment shifted rapidly throughout the day, as evidenced by a Dst index of -46 nT. Monitoring stations recorded this moderate disruption alongside the usual passage of asteroids. Notably, 2026 TP6 made its closest approach today; precise tracking from NASA CNEOS confirmed it posed no threat to our planet.

Observers looking ahead to the night sky may have noticed the early signs of the Orionids meteor shower. Although the shower does not reach its maximum intensity until 2026-10-22, it remained active within its window of 2 October to 7 November. With its radiant point centred in the constellation Orion, this annual display—born from the debris of 1P/Halley—is expected to produce a zenithal hourly rate of 20 meteors.

Those interested in historical context can compare these readings to significant storms found in the archive. For further technical data, the glossary provides a breakdown of magnetic measurements, while our imagery section catalogues the day’s specific solar signatures. As we move out of this unsettled window, the local forecast suggests a return to geomagnetic calm. For any unexplained phenomena observed during the peak hours, reports remain open in the UAP database.