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Our Start to Our End: Methane Skies & Black Holes

The event takes place on one level with the side of the Taproom opened for step-free access. Toilets are not accessible.
Mon 19 May Doors 7:00 pm
Event 7:30 pm to 9:30 pm
Left Handed Giant Taproom, Unit 3 Wadehurst Industrial Park,
Bristol BS2 0JE
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Standard £5.00
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Science going

Tickets remaining: 35

A double billed evening of astrophysics and planetary science! We start with a Tour of Titan from Joshua Ford, from the methane rich atmosphere to an underground ocean, we find a world similar to our own before life began. Following that we move far away to explore black holes with Fergus Baker, with cutting edge simulations to trace the paths taken by light, he’ll illuminate what’s happening around these stellar corpses.

A Tour of Titan: The Most Interesting Place in The Solar System

Joshua Ford ( PhD Researcher in Planetary Science, University of Bristol)
Titan, Saturn’s largest moon, is a world both alien and familiar. Beneath its thick orange haze lies a dynamic atmosphere, vast methane lakes and a subsurface ocean. Using ground and space-based telescopes, scientists have uncovered how Titan’s hazes shape its climate and whether key organic molecules, similar to prebiotic Earth, hint at conditions for life. In this talk, we’ll explore Titan’s mysteries, from its methane rain to its cryovolcanism, and why this moon pushes the limits of planetary chemistry! Grab a pint and learn why Titan is the most interesting thing in our solar system.
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Light Echoes From Black Holes

Fergus Baker (PhD student at the University of Bristol)
The lifetime of a star can end in a number of spectacular ways, and what remains after a star has imploded can take on a life of its own. Black holes, once a theoretical curiosity, are now understood to be ubiquitous and fundamental to the evolution of the Universe, ranging in mass from a few to a billion times the mass of the Sun. Those we observe with telescopes seem to be intensely restless, but as they are too far away to resolve as images, our best way to understand them today is by trying to simulate the system and gleam understanding from their changing spectra.
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