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Astronomy Picture of th e Day
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Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Dec 21, 2015

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Page 1: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Astronomy Picture of the Day

Page 2: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Possible First Pic of Extrasolar Planet

http://news.yahoo.com/s/space/20080915/sc_space/possiblefirstphotoofplanetaroundsunlikestar

Page 3: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Question

The color of visible light is determined by its ____.

A)brightness B) amplitude C)speed D)wavelength

Page 4: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Question

If the wavelength of light increases, while the speed remains constant, the frequency must ____.

A)increase also B) decrease C)remain unchanged

Page 5: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Question

If the wavelength of light increases, while the speed remains constant, the frequency must ____.

A)increase also B) decrease C)remain unchanged

c = f

Page 6: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Question

The bending of light that occurs when moving between media of different densities is called ___.

A)reflection B) refraction C)diffraction D)distortion

Page 7: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Question

The bending of light that occurs when moving between media of different densities is called ___.

A)reflection B) refraction C)diffraction D)distortion

“The change of direction of light as it passes from one medium to another is associated with a change in velocity and wavelength. The energy of the light is unchanged as it passes from one media to another. When visible light in air enters a medium such as glass, the velocity of light decreases to 75% of its velocity in air and in other materials the decrease can be even more substantial.”

Page 8: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

fc =

1 nm = 10 -9 m , 1 Angstrom = 10 -10 m

The Electromagnetic Spectrum

Page 9: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Spectroscopy and Atoms

How do you make a spectrum?

Page 10: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

When you bend light, bending angle depends on wavelength, or color.

Refraction of light

(Prism demo)

Page 11: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

What does the spectrum of an astronomical object's radiation look like?

Many objects (e.g. stars) have roughly a "Black-body" spectrum:

Brightness

Frequency

also known as the Planck spectrum or Planck curve.

Page 12: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Questions

How is temperature related to the amount of energy radiated?

How is temperature related to the color of the object?

(Blackbody Demo)

Page 13: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

"cold" dust

"hot" stars

"cool" star

Sun

frequency increases, wavelength decreases

The wavelength of peak emission tells us the temperature of the object!

Page 14: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Types of Spectra

1. "Continuous" spectrum- a luminous solid or liquid, or a sufficiently dense

gas, emits light of all wavelengths and produces

a continuous spectrum

2. "Emission" spectrum- a low-density, hot gas emits light whose

spectrum consists of a series of bright emission lines that are characteristic of the composition of the gas.

1. "Absorption” Spectrum- a cool, thin gas absorbs certain wavelengths

from a continuous spectrum, leaving dark absorption lines in their place, superimposed on the continuous spectrum.

Page 15: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Pattern of lines is a fingerprint of the element

Page 16: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

For a given element, emission and absorption lines occur at the same wavelengths.

Helium discovered in Sun’s spectrum before being found on Earth!

Sodium emission and absorption spectra

Page 17: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

The Particle Nature of Light

Light interacts with matter as individual packets of energy, called photons.

cphoton energy is proportional to frequency:

E f (or E 1

example: ultraviolet photons are more harmful than visible photons.

Page 18: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

The Nature of Atoms

The Bohr model of the Hydrogen atom:

_

+

proton

electron

"ground state"

_

+

an "excited state"

Text Website Video Clips

Page 19: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

When an atom absorbs a photon, it moves to a higher energy state briefly

When it jumps back to lower energy state, it emits photon(s) in a random direction, conserving the total energy of the system!

(video clips)

Page 20: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Other elements

Helium Carbon

neutron proton

Each element has its own allowed energy levels yielding a unique spectral fingerprint.

Page 21: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Questions?

How Many Types of Spectra?

What Causes spectra?

Text Website Tutorial

Page 22: Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet .

Spectrum of the Sun

Absorption spectrum

What causes emission/absorption of light at specific wavelengths?