[PPT]PowerPoint Presentation - Risa Wechsler -...

32
Midterm Distribution 31 A’s, 37 B’s, 26 C’s, 21 D’s, 17 F’s

Transcript of [PPT]PowerPoint Presentation - Risa Wechsler -...

Page 1: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Midterm Distribution31 A’s, 37 B’s, 26 C’s, 21 D’s, 17 F’s

Page 2: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Common Mistakes

Do the algebra first! Units, Units, Units Does your answer make sense? Using ratios

Page 3: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Lecture 18:

Telescopes and

Observational Astronomy

Page 4: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

There are two kinds of telescopes

RefractingRefracting: a lens is used to focus the light from distant objects.

ReflectingReflecting: a primary mirror is used to gather and focus light.

Page 5: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

A Refracting Telescope

Page 6: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

A Reflecting Telescope

Page 7: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Alternative designs for reflecting telescopes

Page 8: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date
Page 9: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Charge Coupled Devices (CCD)

Page 10: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Fundamental Telescope Properties

Light collecting area (diameter of primary mirror or lens)

angular resolution (smallest angular distance that can be resolved clearly) limited by effects of Earth’s atmosphere

Page 11: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Angular Separation

= 360o . s /(2d) “small angle formula”

Page 12: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Angular Resolution

Page 13: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Diffraction

Page 14: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

The Diffraction Limitdiffraction limit = 2.5 x 105 x wavelength of light(arcsec) diameter of telescope

Find the diffraction limit of the 2.4 m Hubble Space Telescope for visible light (500 nm).

d.l. = 2.5 x 105 (500 x 10-9 m/2.4 m) = 0.05 arcsec

Page 15: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Where to put your telescope high and dry – to minimize the blurring

effects of the Earth’s atmosphere and emission/absorption from water vapor

away from light pollution with roads, electricity, and other support

systems nearby

Page 16: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

The Summit of Mauna Kea

Page 17: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

The Keck Telescopes

Page 18: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

The Magellan Telescopes

Page 19: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Basic Functions of Telescopes

Imaging/photometryaccurate measurement of light intensity filters can be used to separate into different

colors spectroscopy

light spread out using a diffraction grating time sequence

how an object’s brightness changes with time

Page 20: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date
Page 21: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

A Basic Spectrograph

Page 22: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Spectral Resolution

Page 23: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Telescopes across the spectrum

Page 24: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Hubble Space Telescope

Page 25: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Infra-red Telescopes

SOFIA

SIRTF

Page 26: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Radio Telescopes

Arecibo

Very Large Array (VLA)

Page 27: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Interferometry An array of smaller

telescopes can be used together

the light gathering power is equal to the sum of all the areas

the angular resolution is greatly improved

Page 28: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

X-ray Telescopes

grazing incidence mirror

Page 29: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Chandra X-ray Observatory

Page 30: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Compton Gamma-ray Observatory

Page 31: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Images of non-visible light

Page 32: [PPT]PowerPoint Presentation - Risa Wechsler - Homerisa.stanford.edu/satam/dl2/rachlec112/lecture18.ppt · Web viewTitle PowerPoint Presentation Last modified by laxmi Created Date

Radio

CO

FIR

NIR

vis.

X-ray

gammaray