The Spectroscope: New Meanings in Light

Slides:



Advertisements
Similar presentations
Excited Elements.
Advertisements

Spectroscopy Study Guide
Fingerprints in Sunlight Understanding Spectroscopy
1 Fingerprints in Sunlight Understanding Spectroscopy Stanford University Solar Center.
Spectroscopy: and finding out the elements of deep space objects.
WHAT IS OUR SUN MADE OF? 94 % Hydrogen – the most abundant gas in the universe and 6 % Helium All the other elements make up just 0.13% (with oxygen, carbon,
Chapter 24 Studying the Sun
When heated to high temps, gases give off light. If this light is passed through a slit, then through a prism or diffraction grating, the following patterns.
< BackNext >PreviewMain Section 1 Stars Chapter 15 Bellringer List ways that stars differ from one another. How is the sun like other stars? How is it.
Earth Science 24.1 The Sun: Study of Light
FYNvpI. Topic 3: The Spectrocope: New Meanings in Light Science 9 - Space.
Stars and Galaxies 28.1 A Closer Look at Light Chapter 28.
WHAT ARE STARS? Huge, hot balls of gas that are trillions of kilometers away from the Earth.
Science 9: Unit E: Space Exploration Topic 3: Spectroscopy and the Doppler Shift.
Rainbows from Space. Astronomer’s Tools Telescopes Telescopes –On Earth or in Earth orbit Cameras Cameras Prisms (spectroscope) Prisms (spectroscope)
Lecture II Light spectra. The Birth of the Quantum Max Planck –The energy contained in radiation is related to the frequency of the radiation by the relationship.
Spectroscopy and Astronomy Erin Wood, M.S., M.S. Neil Marks, B.A.
Atoms & Light (Spectroscopy). Blackbody Radiation A. Blackbody = a hot solid, hot liquid, or hot high density gas that emits light over a range of frequencies.
Spectroscopy The study of the interaction between matter and light.
Quantum Theory, Part I The Atom Day 4 Prism n White light is made up of all the colors of the visible spectrum. –Passing it through a prism separates.
Spectral Analysis Gleaming Information From The Stars.
Tools of Modern Astronomy
 Fusion – process of 2 nuclei that combine to make one (a new element ) and emitting large amounts of energy.  The sun is a giant ball of hydrogen.
Gustav Kirchoff, Robert Bunsen
2.4 Studying the Sun. Electromagnetic Radiation  The visible light we see is only a fraction of energy coming from various objects  Most of what we.
Different Types of Spectrums. Types of Spectrums Continuous Spectrum Emission Spectrum Absorption Spectrum All colors of the spectrum Are shown (some.
Space Explorations Science 9. THE SPECTROSCOPE: NEW MEANINGS IN LIGHT Topic 3.
4. Complex Knowledge: demonstrations of learning that go aboveand above and beyond what was explicitly taught. 3. Knowledge: meeting the learning goals.
The Spectroscope.
Questions: What is a continuous spectrum?
Studying the Sun Notes H- Study of Light Chapter 24
Bohr’s Model of the Atom
Spectroscopy Lecture.
Most of what is known about stars comes from spectral studies.
Prepare your scantron: Setup:
Fingerprints in Sunlight
Electromagnetic Spectrum
Atomic Spectra Lab 1.
 Spectroscopy continued 
When heated to high temps,
24.1 – The Study of Light.
LINE SPECTRA New methods of splitting white light into its constituent wavelengths in thew 19th century (the diffraction grating) revealed that the spectrum.
I’m coming around to grade this.
Solar Spectrum wavelength in Å Joseph von Fraunhofer, 1814.
Chapter 4.
Spectra.
ELECTROMAGNETIC SPECTRUM
Prepare your scantron:
Electromagnetic Radiation
Unit III Part 1: Weathering and Erosion
Nature of light and atomic spectrum
 Spectroscopy continued 
Optical Telescopes, Radio Telescopes and Other Technologies Advance Our Understanding of Space Unit E: Topic Three.
ATOMIC SPECTRA.
Fingerprints in Sunlight
5.4 Learning from Light Our goals for learning
Light and The Electromagnetic Spectrum
The Spectroscope: New Meanings in Light
Spectroscopy.
Prepare your scantron:
Continuous, Emission, and Absorption
5.4 Learning from Light Our goals for learning
Spectra Lab.
Understand the electromagnetic spectrum and how it is organized.
Key Areas covered The bohr model of the atom
Color Color is light's version of pitch i.e. its how the eye perceives the frequency of the electromagnetic radiation between 4.3 x 1014 Hz and 6.7 x 1014.
Electromagnetic Spectrum
Ch Stars Chapter 19, Section 1 Part 1.
Aim: How to identify elements based on their atomic spectra
A Closer Look at Visible Light
Presentation transcript:

The Spectroscope: New Meanings in Light Topic 3 – Space and Exploration

Spectral Lines Isaac Newton passed a beam of light through a prism and produced a spectrum of colors. White light, is made up of ALL colors

Spectroscope A spectroscope is a device that has a narrow slit and a prism. It takes light and passes it through this very narrow slit and through the prism This creates much finer detail.

Experiment Joseph von Fraunhofer used a spectroscope to look at the sun. He noticed HUNDREDS of dark lines in the sun’s spectrum (solar spectrum) These dark lines are called spectral lines

Spectroscopy Spectroscopy is the Science of color Vapors of different elements give off different colors through a spectroscope when heated Mercury, when heated, is blue Sodium, when heated, is yellow

Gustav Kirchoff and Robert Bunsen heated all sorts of chemicals and looked at the vapors through a spectroscope They realized ….. NOT ALL THE COLORS OF THE RAINBOW ARE PRESENT!

Each element has its own FINGERPRINT No two elements are exactly the same It is like a human’s fingerprint. The colors that show up are unique to a certain light source.

Three Types of Spectra 1. Emission or bright line spectrum If you heat a gas at low pressure (vacuum), it produces a spectrum that is only a set of bright lines of certain colors on a black background.

2. Continuous Spectrum If you heat a solid, liquid or gas at high pressure, the resulting spectra contain ALL THE COLORS blending into one another. Like a rainbow in the sky.

3. Absorption or Dark Line Spectrum When white light is passed through a cooler gas, the spectrum is a continuous spectrum with dark gaps between colors The gas that the light passes through absorbs or removes some of the colors in the spectrum

THE COMBINATION This is Hydrogen…. Who can explain this?

Diffraction Gratings Spectroscopes usually use prisms to split the light into a spectrum. To get the best detail in a spectrum, a diffraction grating can be used instead of a prism.

This happens because the waves bend around corners and diffract (bend) When light is passed through VERY small openings, a spectrum is produced. This happens because the waves bend around corners and diffract (bend) A device with thousands of closely spaced slits is called a diffraction grating Examples of where diffraction gratings are used: CD’s Holographic trading cards

different sources of light produce different types of these spectra. Also, you know that Kirchoff and Bunsen discovered that each element (when heated in a vacuum) produces a unique pattern of spectral lines.

Solar Spectrum A light that passes through a gas will have spectral lines (dark) where the gas has absorbed the light. The solar spectrum had HUNDREDS of dark lines which means the light had to have passed through several gases in the sun’s atmosphere before reaching Earth

Spectral Analysis By looking at each of these dark lines in the solar spectrum, we can determine which elements are present in the Sun’s atmosphere. COOL!!

Example Hydrogen Helium Sodium Star 1 Star 2