Lectures | Lecture page | Astro1 page |
High mass stars live for almost no time at all
(a few to a few 10's of millions of years)
- most prominent as red giants:
the most massive are the youngest
Two key ingredients to determining a stellar population:
... with the Sun at the center
planetary nebulae
spiral nebulae
They are galaxies like the Milky Way
- there are other types of extra-galactic ``nebulae'' that
represent different types of galaxies
- the Milky Way is roughly 30 kpc in size,
a round, centrally located bulge, primarily of old stars,
and a halo of exclusively made of old stars.
North Celestial Pole vs. North Galactic Pole . . .
. . . off by 60 degrees
RR Lyrae
- On the Horizontal Branch
- 102 as luminous as the Sun
- The Sun will be a RR Lyrae in about 5 billion years
- Period and luminosity uncorrelated (``horizontal'')
- But narrow range of luminosity (``horizontal'')
- Plentiful (there are many low-mass stars)
- Tomorrow's super novae - Type II
- 104 as luminous as the Sun
- pulsation period and luminosity strongly correlated
(b) there was no available method to infer distances to these 'nebulae'
(c) these 'nebulae' had appearances identical to confirmed Galactic nebulae
(d) there was no philosophical precedence for believing in external galaxies
(e) The size of the Milky Way was unknown
Lectures | Lecture page | Astro1 page |