stars galaxies and the universe
DESCRIPTION
Stars Galaxies and the Universe. Introduction : The Big Picture. Hierarchy of structures:. Nuclei (particles) Atoms Stars/Planets Galaxies Universe. Atoms: Nuclei: protons neutrons Electrons. p.418a. Solar magnetic surface storm. Earth. Scale of the Solar System. - PowerPoint PPT PresentationTRANSCRIPT
Stars Galaxies and the Universe
Introduction : The Big Picture
Hierarchy of structures:• Nuclei (particles)• Atoms• Stars/Planets• Galaxies• Universe
Atoms:Nuclei:
protonsneutronsElectrons
p.418a
Solar magnetic surface storm
Earth
Scale of the Solar System
• Earth-moon system…..• The sun as an orange….• The nearest star• The galaxy !
Our Galaxy : The Milky Way
Milky way galaxy is a complex system• 1011 stars (& planets?)
Each with life cycle: birth/life/death• Material between the stars
Tenuous gas: clouds; diffuse
New star-formation region
Two young star clusters
Slow death of low mass star
Our Galaxy
Solar systemGalaxy Center
Earth = 100 nm = virusSun = 10 μm = cellEarth orbit = ¼ cm = pin headSolar system = 20 cm = saucerNearest star = 250 m = lawn
Naked eyestars
EagleNebula
Jewel BoxCluster
CrabNebula
The Population of Galaxies
Galaxies are a diverse population• Different sizes & shapes & motions
different histories?• They tend to form groups
pairs clusters; some collide and merge
Interactinggalaxies
Galaxies to the horizon
The Universe is filled with galaxies• 1011 galaxies visible• More distant ones appear younger
look-back time due to finite light speed
Our galaxy is here
3 billion light years
(~20% to “the edge”)
SDSS : ⅓ million galaxies
Hubble Deep Field~1500 galaxies
Sky area ~2.5×2.5 arcmin≡ pinhead @ arms-length
A 1689Rich galaxy cluster
2 Gly distantGravitational lens
The Visible Universe
HDF
SDSS &2dFGRS
“Nearby”galaxies
13.7 Gly 0
MW galaxy = 20 m = class roomMW galaxy = 20 m = class roomLocal group = 600 m = central groundsVirgo cluster = 15 km = WalmartComa cluster = 100 km = Culpeper
Our Galaxy
Keck/VLT+ Cluster Lens