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Optical Spectrum of a Galaxy Flux Recession velocity = 14387 km / s z = 0.0479 [O III] H H

Optical Spectrum of a Galaxy

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Optical Spectrum of a Galaxy. H a. Recession velocity = 14387 km / s z = 0.0479. Flux. H b. [O III]. Vesto Slipher. Redshifted Spectra. Edwin Hubble. The Original Hubble Law. Modern-Day Hubble Law. Today our best value for the Hubble constant is 70 +/- 5 km / s / Mpc. - PowerPoint PPT Presentation

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Page 1: Optical Spectrum of a Galaxy

Optical Spectrum of a GalaxyF

lux

Recession velocity = 14387 km / sz = 0.0479

[O III]

H

H

Page 2: Optical Spectrum of a Galaxy

Vesto SlipherVesto Slipher

Page 3: Optical Spectrum of a Galaxy

Redshifted SpectraRedshifted Spectra

Page 4: Optical Spectrum of a Galaxy

Edwin HubbleEdwin Hubble

Page 5: Optical Spectrum of a Galaxy

The Original Hubble LawThe Original Hubble Law

Page 6: Optical Spectrum of a Galaxy

Modern-Day Hubble LawModern-Day Hubble LawToday our best valuefor the Hubble constantis 70 +/- 5 km / s / Mpc.

Page 7: Optical Spectrum of a Galaxy

Balloon AnalogyBalloon Analogy

Page 8: Optical Spectrum of a Galaxy

Raisin-Bread AnalogyRaisin-Bread Analogy

Page 9: Optical Spectrum of a Galaxy

Measuring the Ages of the OldestMeasuring the Ages of the OldestObjects in the UniverseObjects in the Universe

Color-Magnitude Diagram for a Globular Cluster

The age of the Universe is thought to be 13.7 Gyr.

The oldest globular clusters are about 12.6 Gyr old.

So things seem consistent!