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Science and Technology Facilities Council


The search for ET just got easier

Astronomers at the Science and Technology Facilities Council's William Herschel Telescope have confirmed an effective way to search the atmospheres of planets for signs of life. This method uses transmission spectra, which can reveal vital information about a planet's atmosphere, providing clues about potential biological processes.

Swift Satellite records early phase of gamma ray burst

UK astronomers using NASA Swift Satellite captured an ultraviolet spectrum of a gamma ray burst just 251 seconds after its onset, marking the earliest ever recorded. This breakthrough allows for calculations of distance and brightness within hundreds of seconds and provides new insights into GRB causes and host galaxies.

SourceScience and Technology Facilities Council·JournalMonthly Notices of the Royal Astronomical Society·DateMar 2, 2009

Death of a star

For the first time a star has been observed as it goes supernova – a mind-bogglingly powerful explosion that briefly outshines an entire galaxy. UK scientists used NASA's Swift satellite and a combination of orbiting and ground-based observatories to catch the event in real-time.

Millennium simulation

The Millennium Simulation uses sophisticated modeling techniques to recreate evolutionary histories for 20 million galaxies and supermassive black holes. The simulation demonstrates that a few massive black holes can form early enough to account for rare quasars, and provides a new tool for understanding the nature of dark energy.

Whimpers from the Sun?

A new study reveals that Coronal Mass Ejections (CMEs) can originate from tiny magnetic regions on the Sun, challenging current theories. The research used data from NASA/ESA's SOHO spacecraft and found that these mini-CMEs were energetic enough to reach Earth, causing aurora and disrupting satellite communications.

Jupiter: A cloudy mirror for the Sun?

Astronomers using the European Space Agency's XMM-Newton telescope discovered that Jupiter's x-ray glow is due to x-rays from the Sun being reflected back off the planet's atmosphere. The discovery synchronises Jupiter's day-to-day disk x-rays with the Sun's emissions, providing new insights into solar activity.

SourceScience and Technology Facilities Council·JournalGeophysical Research Letters·DateMar 7, 2005

Dusting for clues: Gemini discovers evidence for recent planet-forming collisions around nearby star

Astronomers using the Gemini South telescope in Chile have observed new details in the dusty disk surrounding Beta Pictoris, showing a large collision between planetary-sized bodies may have occurred as recently as the past few decades. The mid-infrared observations provide evidence for energetic encounters during planetary formation.