SIRTF NASA’s Space InfraRed Telescope Facility Alyssa A. Goodman Professor of Astronomy Harvard University.

Slides:



Advertisements
Similar presentations
Telescopes Section 1-4. Telescope l Tele – distant, far l Scope- see l Invented in the 16 th century l First used by Galileo Who found moons around Jupiter.
Advertisements

Oct. 18, Review: Telescopes – their primary purpose… Across the full EM spectrum (radio through very high energy gamma- rays) telescopes fundamentally.
Chapter 19: Between the Stars: Gas and Dust in Space.
Astronomy and the Electromagnetic Spectrum
A105 Stars and Galaxies Today’s APOD 8:30 PM on Thursday!
Astronomy 1010 Planetary Astronomy Fall_2014 Day-22.
X-Ray UltravioletVisibleInfraredRadio The Electromagnetic Spectrum and the Universe.
Spectral Lines Celestial Fingerprinting. Goals From light we learn about –Composition –Motion.
Hot Molecular Gas Orbiting Young Stars: Planet Forming Disks or Small Stellar Companions? A look at data taken at the 200” Mount Palomar Telescope, and.
Infrared Astronomy The image above is an aitoff projection of the sky centered on the center of the Milky Way Galaxy (in the constellation Sagittarius).
Honors Ch Pg Almost everything we know about the universe (space) comes by studying light from distant sources. Light from what?
7 Emission Astronomy: The Science of Seeing. 7 Goals What is light? What are the types of light? Where does the light we see come from? Understanding.
Chapter 3: Telescopes. Goals Describe basic types of optical telescopes Explain why bigger is better for telescopes Describe how the Earth’s atmosphere.
5 Spectral Lines Celestial Fingerprinting. 5 Goals From light we learn about –Composition –Motion.
Ionization, Resonance excitation, fluorescence, and lasers The ground state of an atom is the state where all electrons are in the lowest available energy.
The SOAR Telescope MSU’s Laboratory for Astronomical Discovery.
Light and Telescopes Chapter 5. Radio Interferometry The Very Large Array (VLA): 27 dishes are combined to simulate a large dish of 36 km in diameter.
Celestial Fingerprinting
In 1800 William Herschel discovered “invisible light” It’s energy with all the same characteristics as visible light, but is not sensed by the human eye.
Microwave: The Cosmic Microwave Background (CMB). Shortly after the Big Bang, the Universe cooled enough to allow atoms to form. After this point in time,
Telescopes and Astronomical Instruments The 2 main points of telescopes are 1)To make images with as much angular information as possible 2)To gather as.
Stellar Evolution: from star birth to star death and back again Prof. David Cohen Dept. of Physics and Astronomy.
Infrared Telescopes 1.
Modern Telescopes Lecture 12. Imaging Astronomy in 19c Photography in 19c revolutionize the astronomy Photography in 19c revolutionize the astronomy 
Outline This Presentation contains slides appropriate for all the sections of the activity. – White slides are included (but hidden from the Slideshow)
ELECTRO MAGNETIC SPECTRUM The electromagnetic spectrum extends from wavelengths of many meters to wavelengths of submicroscopic size. Visible light has.
Creating Light. Light as a Wave Light (or electromagnetic radiation), can be thought of as either a particle or a wave. As a wave, light has a wavelength,
Astronomy and the Electromagnetic Spectrum
Multiwavelength Astronomy What do different wavelength regimes allow astronomers to “see”?
 Named after Edwin Hubble, the astronomer who discovered the expansion of the universe. Launched in 1990 and contains a 2.4 m (95 in) mirror with which.
How do colors in a spectrum help us understand stars? Image from
Light. Review Question What is light? Review Question How can I create light with a cow magnet?
BROWN DWARFS Failed Stars of the Universe. Stars come in many shapes and sizes, but they all have one thing in common-they are massive enough to ignite.
Tools of Astronomy.
Telescopes. Images can be formed through reflection (mirror) or refraction (lens). Reflecting mirror Optical Telescopes.
Tools of Astronomy. Electromagnetic Radiation Light travels as an “Electromagnetic” Wave The light you see is called Visible Light Speed of light: 186,000.
Telescopes Portals of Discovery. Telescope A telescope is an instrument designed to aid the observation of remote objects by collecting some form of electromagnetic.
Space Telescopes and Astronomy Physics 113 Goderya Chapter(s): 6 Learning Outcomes:
Astronomy! Emily Cunningham Institut d’Astrophysique de Paris.
A105 Stars and Galaxies  Homework #4 due today  Telescopes  Read unit 30 for next week  News Quiz Tuesday  First Exam on Sept. 28 Today’s APODAPOD.
Using All of Our Tools What the Various Parts of the Spectrum Tell us About Space.
What Does the Infrared Have to Do With Space?
Emission Spectra.
Agenda International Year of Light Resources EM Spectrum Review NASA Astrophysics Observatories, techniques, images Visible Spectra, IR demo, UV beads.
What I did for Spring Break …. Bit of Administration …. ReadingReading –BSNV Chaps. 7 and 8 Particularly important discussion section -Particularly important.
Spitzer Space Telescope
Astronomy 1010 Planetary Astronomy Fall_2015 Day-23.
Instruments of Astronomy Space Observatories. NASA’s Four Great Observatories.
NIR, MIR, & FIR.  Near-infrared observations have been made from ground based observatories since the 1960's  Mid and far-infrared observations can.
Astronomy Picture of the Day APOD. March 2, 2015.
Star Formation The stuff between the stars Nebulae Giant molecular clouds Collapse of clouds Protostars Reading
Telescope Technology Types of Telescopes Hubble Telescope and NASA’s Great Observatories.
7 Spectral Lines Celestial Fingerprinting. 7 Goals From light we learn about –Composition –Motion.
Universe Galaxies & Stars Electromagnetic Spectrum
Telescopes.
Multiwavelength Images
Lesson 1 Observing the Universe
6.3 Telescopes and the Atmosphere
Ch.1, Sec.2 - Telescopes Optical Telescopes
The Universe and Electromagnetic Spectrum
Telescopes and the Electromagnetic Spectrum Section 3
IR Telescopes Need relatively large objectives for reasonable resolution at infrared wavelengths. Need cooling to reduce thermal background “noise”
The Study of Light Picture taken
Chapter 36—Optical Instruments
Radio Astronomy.
Bell Ringer Cell phones have become an important device in modern society. Which wavelength of the Electromagnetic Spectrum do you believe is responsible.
Telescopes 4/23/15 IN: What is a telescope? How is it used?
Astronomy from Space Working from the ground, astronomers must contend with the Earth's atmosphere. In addition to blurring the view due to seeing, the.
Unit 3 Practice Test Answer KEY
Astronomy Ch.1 Sec.3.
Presentation transcript:

SIRTF NASA’s Space InfraRed Telescope Facility Alyssa A. Goodman Professor of Astronomy Harvard University

It’s not always so cold in space… “Revenge is a dish best served cold, and it’s very cold in space.”-- Khan

Observatories for Any “Temperature”

Wavelength

NASA’s Great Observatories

What wavelengths are easy to observe from the ground?

The Electromagnetic Spectrum LOW TO HIGH ENERGY SIRTF

Infrared Life

The “Thermal” (or “Far”) Infrared Temperature, deg F

“Emission” from a Cold-blooded Lizard Optical Image Far-Infrared Image “Room Temperature”

Emission & Absorption Emitter Absorber “Emission” “Absorption”

Emission Emitter “Emission”

Absorption Absorber “Absorption”

Not all Wavelengths are Absorbed Equally “Dust Grain” “Dust Grain” Light is “Extinguished” & Does not Reach Us Light Goes Right by & Reaches Us

Near-Infrared Optical

SIRTF NASA’s Space InfraRed Telescope Facility “Great Observatory” for Near- and Far-Infrared Astronomy

Real Star Formation Today’s Tour: Optical and Infrared Views of Orion (Images prepared for upcoming “L-30 Press Briefing at NASA HQ, March 25, 2003)

Simulate d Star Formatio n

SIRTF “L-30” Press Conference Nebula Far- infrared Image Orion

Hubble Space Telescope Image Near- infrared Image

SIRTF NASA’s Space InfraRed Telescope Facility Alyssa A. Goodman Professor of Astronomy Harvard University

(Far-)Infrared Astronomy