ASTR 1120 ASTR 1120 General Astronomy: General Astronomy: Stars & Galaxies Stars & Galaxies
EXT Tuesday 10/20:
earching for dist
stant world earching for dist stant world
GO DIRECTLY TO THE PLANETARIUM
earching for dist stant world stant world GO DIRECTLY TO THE - - PowerPoint PPT Presentation
ASTR 1120 ASTR 1120 General Astronomy: General Astronomy: Stars & Galaxies Stars & Galaxies ID IDTERM # #2 : ID IDTERM # #2 EXT ursday 10/15: EXT Tuesday 10/20: earching for dist earching for dist
GO DIRECTLY TO THE PLANETARIUM
– Gravity vs. electron degeneracy pressure
– Gravity vs. neutron degeneracy pressure
Even more massive stars (M>30-40 (M>30-40 M Msun
sun)
) black black holes holes
– Gravity wins
when Mcore > 3 Msun
[Image from “Spacetime and Gravity” by S. Carroll]
[Image by R. Jantzen]
can act like lens can act like lens can can redshift redshift light light
A B
[Image credit: R. Ellis & I. Smail with HST (NASA/STScI)]
Source behind the lens: EINSTEIN RING
[Image credit: L. King with HST (NASA/STScI)]
The arches are the result of gravitational lensing
[Image credit:
(NASA/STScI)]
– can fall in but never get out
– Event horizon is a “theoretical” point of no return
Gravity imposes curvature on space curvature on space – – light light’ ’s path through space will be s path through space will be “ “bent by gravity bent by gravity” ” – – within the event horizon, it cannot within the event horizon, it cannot climb out of the hole climb out of the hole
As matter approaches event horizon event horizon… … – – tidal forces are tremendous tidal forces are tremendous – – object would be
“spaghettified spaghettified” ”
Criteria:
system is too massive to be white dwarf or neutron star
– Mass > 3 MSun
normal star
Blue Blue supergiant supergiant Accretion disk Accretion disk
Short Long
High star rotation likely needed
[Image from http://www.laeff.esa.es/BOOTES/esp/grb/grb4.htm]