The formation of a young protostar following the collapse of a previously inert dust cloud
We had a great turnout for March’s Urban Astronomy session last week at the Sea Cadet’s Hall in Inverness. The indoor presentation massively benefited from our new giant screen, expertly erected by Robbie (pictured below). Here’s a selection of slides from my presentation on naked eye observing and the life of giant stars.
Robbie putting the final touches to our new giant screen for indoor astronomy presentations and virtual sky guiding
Topics covered:
– Naked eye and binocular observing
– Satellites: Iridium Flares and ISS
– Colour, temperature and mass of stars
– The Hertzsprung-Russell diagram
– Protostar formation from dark nebulae
– Main sequence burning and final fate of stars
– White dwarfs, supernovae, neutron stars and black holes.
As ever there were some superb questions during and after the talk. Stay tuned for upcoming events as myself and Caroline roll out the program.
In the simplest terms stars behave like black body radiators with colour linked to their surface temperatures.
The brightest stars in the night sky can be close – like Sirius – or giant stars very far away (eg. Betelgeuse, Rigel, Deneb).
The HR diagram. An elegant and reliable tool for describing the evolution of stars from main sequence burning into their final stages of life
