The measure of Cosmological distances
Asaf Pe’erSpace Telescope Science
Institute
How far is Jupiter??
Greece, c. 300BCWhat is the size of earth ?
I. Science at ancient times
Syene, EgiptFirst measurement of earth’s radius:
Eratosthenes of Cyrene (276BC- 196 BC)
Eratosthenes: Earth circumference =40000 km Earth radius = 6000 km
Measuring the size of the moon using lunar eclipse
Time to full eclipse~ moon radiusTotal eclipse time
~ earth radius
Moon radius ~ ¼ earth radius
Aristarchus of Samos, 310BC- 230BC
Distance to the moon ~380.000 km (240.000 mi)
Given moon radius, distance is simple geometry
Geocentric (=earth at the center) vs. Heliocentric (=sun at the center)
universeAristotle (384BC - 322BC) Aristarchus of Samos
(310BC - 230BC)
Why Geocentric ?1. "we see" 2. if the earth moves, where is the wind ?3. Gravity – everything is attracted to the center of the universe4. Parallax: stars don't move !
Parallax
Parsec = paralax-arcsecond =~ 3.3 l.y.
But some stars do move..
Retrograde motion of Mars
The universe according to Ptolemy
Ptolemy: 83-161 AD Circle - “Perfect” shape
Mars motion according to Ptolemy
Mars motion according to Heliocentric theory
Ptolemy model - consistent with observations!!!
Nicolaus Copernicus (1473 - 1543)
Advantages:1. Correct
2 .Simple
Disadvantage:1 .Less accurate than geocentric model
2. Copernicus was unknown
II. Rise of Heliocentric Cosmology
Tycho Brahe (1546 - 1601):Accurate measurements of planet orbits
Johannes Kepler (1571 - 1630):Planets move in ellipses (not circles) around the sun
Kepler’s laws of planetary motion helped Neuton to develop the theory of Gravity
Next breakthrough: the Telescope (1608)
Galileo Galilei (1564 - 1642):First astronomer to use a telescope
Moon has craters ! =(not perfect sphere)!
Jupiter has moons ! =(not everything rotates around earth)!
“Smoking gun”: Venus phases Cannot be explained by Geocentric model
Even the sun has spots ! =(sun is not perfect)!
Measuring the distance to the sun
Giovanni Cassini (1625 - 1712)
1672 -Cassini & Richer measure the distance to Mars
Using Kepler’s laws, Cassini deduce the distance to the sun:150.000.000 km = 1 Astronomical unit (1 A.U.)
William Herschel (1738 - 1822)
Herschel’s 20 foot reflector
III. Measuring distance to the stars
-Found new planet (Uranus)-Discover Infra-Red light-First map of the sky:
Idea: All the stars are the same. Therefore, bright stars are closer.
Herschel’s model of the milky way:
-Stars are ordered in space.
We are part of the Galaxy.
- But he could not scale the size of the galaxy
Friedrich Bessel (1784 - 1845)
1838 :First measurement of distance to a star
61 signi
Distance = 100,000,000,000,000 km =(11 light years)
Scaling the milky way: width = 10.000 l.y,.(today: 100.000 l.y ).Thickness = 1.000 l.y.
Charles Messier (1730 - 1817):deep sky catalogueof Nebulae
“The great debate”:Are nebulae part of the milky way galaxy
- or not?
M31
The great debate
John Goodricke (1764 - 1786):Discovery of variable stars & Cepheids
Mechanism: Envelope contains opaque He2+ - heated - pressure increases- expansion - radiation escape - cooling
Henrietta Leavitt (1868 - 1921):1908: Discovery of periodicity- Luminosity relation in Cepheids
25 Cepheids at the small Magellanic cloud All at same distance from us
1917 :Shapley & Hertzsprung measured the distance to a Cepheid - allow the use of Cepheids as “Standard candles”
1918 :Harlow Shapely measures the milky way
Size of the milky way: 100.000 l.y. ; Thickness = 1.000 l.y
Cepheids in Globular clusters
What about the nebulae?
Edwin Hubble (1889 - 1953):I. 1923 - Discovery of Cepheids in Andromeda galaxy
Distance to M31: 900.000 light years >> Milky
way!!
Spectroscopy: measuring the chemical elements in starsFraunhofer, Bunsen, Kirchhoff (1859)
IV. Measuring distance to the galaxies
Spectrum of the sun
1868 - Lockyer & Janssen discover a new element in the sun (He)1860’s - Huggins: stars contain the same elements as the earth.
1868 - William Huggins finds red shift of Sirius,determine its velocity: 45 km/s
Red Shift
1912 :Vesto Slipher measures red shift of galaxies
V ~ 300-1000 km/s
Strangley, most of the galaxies
are receding from us !
Edwin Hubble (1889 - 1953):II. 1929 - Discovery of distance - velocity relation in galaxies
Hubble’s law Velocity = Distance H0
H0 = Hubble’s constant = 70 (km/s) / Mpc
Mpc = Mega (Million)-parsec ;Parsec = paralax-arcsecond =~ 3.3 l.y.
Baade (1952) & Sandage (1954) corrected the value of H0
Back in time, all the matter was concentrated in a very small region
1915 :General Theory of relativity -- universe collapse (Gravity);
Cosmological constant 1922 :Alexander Friedman
Universe expands !
1927 :Georges Lemaitre
Albert Einstein (1879 - 1955)
V. The big bang theory and beyond
Further proofs for universe expansion & “Big bang”
Ralph Alpher (1921 - 2007):
1948 :Alpher, Bethe, Gamow - H, He production in big bang Alpher, Gamow & Herman - cosmic microwave background (CMB)
Universe: 90% H, 9% He
1964 :Penzias & Wilson discover the CMB
1991 -Fluctuations in the CMB (COBE satellite): “embryos” of galaxies
Mather & Smoot, 2006 Nobel prize
The future
1998 :A surprising twist
Astronomers led by Adam Riess (STScI), Saul Perlmutter (Berkeley)
-The universe accelerates!!!
The universe, 2008
Wmap