NASA s SOFIA: Stratospheric Observatory for Infrared Astronomy" D. Backman! SOFIA Outreach / NASA Ames / SETI Institute!

Size: px
Start display at page:

Download "NASA s SOFIA: Stratospheric Observatory for Infrared Astronomy" D. Backman! SOFIA Outreach / NASA Ames / SETI Institute!"

Transcription

1 NASA s SOFIA: Stratospheric Observatory for Infrared Astronomy" D. Backman! SOFIA Outreach / NASA Ames / SETI Institute!

2 Outline:" Infrared light & infrared astronomy" SOFIA s engineering development" SOFIA in operation" SOFIA science highlights " Airborne Astronomy Ambassadors"

3 William Herschel" Discovery of Infrared Radiation !

4 Getting a more complete picture:! Constellation Orion left: view at visual wavelengths right: far-infrared view!

5 Representing invisible light is as much art as science.!

6 Special capabilities of an infrared observatory:" " Study objects cooler than normal stars," "e.g. stars & planets forming" " Study objects inside or behind interstellar dust clouds" " Study organic molecules in space"

7 View of troposphere / stratosphere boundary (tropopause) from above!

8 Mauna Kea observatories!

9 Evolution of NASA s Airborne Telescopes" LearJet! 10-inch! Kuiper! Airborne! Observatory! 36-inch! SOFIA! 100-inch! Aircraft flying above about 40,000 ft" can observe most of the infrared universe. Airborne infrared telescopes can be more versatile and much less expensive -- than space infrared telescopes. " "

10 SOFIA: An Engineering Marvel"

11 How does SOFIA work?" Airborne observatory has 3 critical parts:!! Boeing 747SP aircraft that must fly at 41,000+ ft!!for hour missions! 17 M-ton reflecting telescope that must be able to point precisely at targets in the universe! Interchangeable Science Instruments that must be able to make sensitive infrared measurements!

12 Component 1: The Aircraft"

13 NASA s Kuiper Airborne Observatory (KAO)" The KAO, a C-141 with a 0.9-meter (36-inch) telescope onboard, was based at NASA-Ames near San Jose and flew from 1975 to 1995,!

14 Studies of cavity acoustics: SOFIA 7%-scale model in NASA Ames 14-ft transonic wind tunnel

15 ^ 1977 >! < 2007!

16 SOFIA on its way to Waco, TX to get chopped:"

17 video of telescope door opening!

18 Component 2: The Telescope"

19 SOFIA Light Path Secondary mirror Spherical bearing CABIN! Infrared instrument Light tube IR light reflection Visible light reflection Visible- wavelength camera Primary mirror

20

21 Putting it together - L-3 Communications Integrated Systems, Waco, Texas!

22 Telescope cavity, with door open:"

23 Component 3: Science Instruments"

24 Four First-generation Instruments HIPO UV / visual / near-ir fast photometer (Lowell Observatory) FLITECAM near-ir camera w/ grism (UCLA) FORCAST mid-ir camera w/ grism (Cornell) GREAT far-ir spectrometer (MPIfR)

25 SOFIA Science Instrument footprints in spectral resolution versus wavelength!

26 SOFIA in operations"

27 SOFIA -- The Next Generation Airborne Observatory! 2.5-meter (100-inch) diameter telescope in a Boeing 747SP Based at NASA-Armstrong facility in southern Calif., with mission science center at NASA-Ames in northern Calif. 20% share with the German space agency DLR First science flight was in 2010 Goal: hr science flights per year, 20-yr lifetime 4-7 weeks per year in Southern Hemisphere deployments

28 SOFIA the observatory! Educator work stations" Pressure bulkhead" Open cavity! (door not shown)! Scientist work stations, telescope and instrument control, etc." Scientific instrument (1 of 6)" TELESCOPE"

29 " View aft past the Mission Directors console." " The telescope is beyond the blue bulkhead." " The science instrument & counterweight are seen at center-rear. "

30

31 Sample Flight Plan!

32 Pointing the telescope: Floating on spherical bearing; Orientation sensed by gyroscopes; Optical TV cameras view field near target!

33 SOFIA: A Scientific Marvel"

34 JUPITER"

35 W3A in Perseus" " Compact HII region &" massive protostar cluster" " [inset]" SOFIA/FORCAST" 7.7, 20, 32 µm" ~ 1.5 x 1.0 pc" " [background]" Spitzer/IRAC" 3.6, 4.5, 7.9 µm" " Note bubble at left, cleared by winds from young O stars in the cluster, resolved by SOFIA." " Salgado et al (Ap.J.)" " Hi-resolution deconvolution" by J. De Buizer"

36 Images of the Milky Way Galaxy s nucleus Ring of molecular clouds orbiting! central supermassive black hole.! [Only massive central star cluster is seen.]! SOFIA: mid-ir" Hubble: near-ir"

37 M82 - SN 2014J" " SOFIA/FLITECAM+grism" µm" " Co II 1.77 µm" FWHM ~ 12,000 km s -1" " Two epochs:" t o + 36 days" t o + 44 days" " Vacca et al (Ap.J.)" " Insets: [left] SOFIA/ FLITECAM J,H,K image of M82, arrow points to SN 2014J" [right] Optical light curves; epoch of first SOFIA observation indicated."

38 MARS" " SOFIA/EXES" H 2 0 & 7.2 µm" R ~ 85,000" " Disk-integrated spectrum compared with terrestrial atmosphere transmission" " Ratio of HDO to H 2 " confirms wetter Mars" in the past." " Encrenaz et al. 2015" (submitted to A&A)" "! Insets:" (left) EXES on SOFIA telescope! (right) Mars 7.2 µm continuum map!

39 Stellar Occultations" SOFIA is able to:!! Probe the sizes," structures (rings & moons), and " "atmospheres of solar system " "bodies by measuring how they " "occult background stars." " Can go anywhere on Earth to " reach the occultation shadow" "of a Solar System object." Toward Occulted Star Object Motion of Occulting Object Shadow of Occulting Object Earth

40 The rings of Uranus discovered via occultation observations by SOFIA s predecessor, the KAO. Star behind Uranus and rings Rings were discovered via occultations of a background star

41 2015 Pluto" occultation" shadow track"

42 video of SOFIA Pluto observations!

43 2015 occultation light curve!

44 Airborne Astronomy Ambassadors"

45 2011: First Airborne Astronomy Ambassador educators! Mary Blessing, Herndon, Va. " Cris DeWolf, Remus, Mich. with Dana Backman (SETI)" Pamela Harman (SETI) with Margaret Piper, Frankfort, Ill. " Kathleen Fredette, Palmdale, CA" Theresa Paulsen, Mellen, Wis. and Marita Beard, San Jose, Calif. " with Coral Clark (USRA)" Cecilia Scorza (DSI) with Wolfgang Vieser, Munich, Germany" Jörg Trebs, Berlin, Germany"

46 22 Educators Selected for the Cycle 4 AAA" Program (flights in 2016), Including:! Marie Thornsberry, Hughbanks Elementary, Rialto CA Wendi Rodriquez, The Heritage School, Phelan CA

47 JOBS IN THE SOFIA PROGRAM" (Many career paths lead here )! Scientists & mathematicians 40 Engineering incl. software & IT 70 Aircraft incl. pilots & mechanics 30 Business & accounting 40 Admin & admin assistants 25 Outreach 10 TOTAL 215!

48 !! For further information:! SOFIA Science Center home page & EPO main page! Spitzer Space Telescope s award-winning infrared tutorial! (includes instructions for home-made Herschel demo)!! To contact the presenter:! dbackman@sofia.usra.edu!!

CYCLE 1 SCIENCE STATUS AND HOW TO PROPOSE TIME ON SOFIA. Helen J. Hall¹, Erick T. Young¹, Hans Zinnecker²,³

CYCLE 1 SCIENCE STATUS AND HOW TO PROPOSE TIME ON SOFIA. Helen J. Hall¹, Erick T. Young¹, Hans Zinnecker²,³ CYCLE 1 SCIENCE STATUS AND HOW TO PROPOSE TIME ON SOFIA Helen J. Hall¹, Erick T. Young¹, Hans Zinnecker²,³ ¹SOFIA Science Center, Universities Space Research Association, NASA Ames Research Center MS 232-12,

More information

Early Science Results from SOFIA, the World s Largest Airborne Observatory

Early Science Results from SOFIA, the World s Largest Airborne Observatory Early Science Results from SOFIA, the World s Largest Airborne Observatory James M. De Buizer Universities Space Research Association Stratospheric Observatory For Infrared Astronomy ABSTRACT The Stratospheric

More information

SOFIA Stratospheric Observatory For Infrared Astronomy

SOFIA Stratospheric Observatory For Infrared Astronomy 1 SOFIA Stratospheric Observatory For Infrared Astronomy E.E. Becklin SOFIA Chief Scientist ISSTT 2008 April 28, 2008 2 Outline of Material Overview of SOFIA Progress to Date Science Schedule and Future

More information

The Stratospheric Observatory for Infrared Astronomy (SOFIA) and the Transient Universe

The Stratospheric Observatory for Infrared Astronomy (SOFIA) and the Transient Universe The Stratospheric Observatory for Infrared Astronomy (SOFIA) and the Transient Universe Dan Lester Department of Astronomy, University of Texas D. Lester Eventful Universe Symposium March 19, 2010 1 Airborne

More information

Observation of Exoplanets with the Stratospheric Observatory for Infrared Astronomy (SOFIA)

Observation of Exoplanets with the Stratospheric Observatory for Infrared Astronomy (SOFIA) Observation of Exoplanets with the Stratospheric Observatory for Infrared Astronomy (SOFIA) a, D. Angerhausen b, E. E. Becklin c, M. A. Greenhouse d, S. Horner e, A. Krabbe b, M. R. Swain f, and E. T.

More information

From Supernovae to Planets

From Supernovae to Planets From Supernovae to Planets Developed by the SOFIA Team Topic: Supernovae Concepts: Supernovae, Planet formation, Infrared observations Missions: Kepler Coordinated by: The NASA Astrophysics Forum An Instructor

More information

American-German Stratospheric Observatory for Infrared Astronomy (SOFIA) Science Mission Operations Briefing

American-German Stratospheric Observatory for Infrared Astronomy (SOFIA) Science Mission Operations Briefing American-German Stratospheric Observatory for Infrared Astronomy (SOFIA) Science Mission Operations Briefing Prof. Dr. Hans-Peter Röser and Helen Hall June 20, 2009 www.irs.uni-stuttgart.de 1 Agenda Who

More information

SOFIA: An Observatory for THz Science and Technology

SOFIA: An Observatory for THz Science and Technology SOFIA: An Observatory for THz Science and Technology Eric E. Becklin *a, Sean C. Casey a, and Xander Tielens b a Universities Space Research Association, NASA MS 211-3, Moffett Field, CA 94035-1000 b Code

More information

SOFIA Edwin Erickson NASA Ames Research Center

SOFIA Edwin Erickson NASA Ames Research Center Rationale Science Status Program SOFIA Stratospheric Obsevatory for Infrared Astronomy SOFIA Edwin Erickson NASA Ames Research Center Stratospheric Observatory for Infrared Astronomy The Dusty and Molecular

More information

Observing with SOFIA

Observing with SOFIA Observing with SOFIA Motivation for Infrared Astronomy The infrared is a key part of the spectrum. The emission arises from gas and dust not in stars and allows to study the colder universe. Stars Hollenbach

More information

Stratospheric Observatory for Infrared Astronomy

Stratospheric Observatory for Infrared Astronomy Stratospheric Observatory for Infrared Astronomy William T. Reach NASA Astrophysics Assets Workshop May 2015 SOFIA Overview Why Infrared Thermal radiation Absorbed sunlight is re-emitted at peak wavelength

More information

R. D. Gehrz a E. E. Becklin b, and Göran Sandell b

R. D. Gehrz a E. E. Becklin b, and Göran Sandell b Infrared Spectroscopic Studies with the Stratospheric Observatory for Infrared Astronomy (SOFIA) a E. E. Becklin b, and Göran Sandell b a University of Minnesota b Universities Space Research Association

More information

The Stratospheric Observatory for Infrared Astronomy (SOFIA)

The Stratospheric Observatory for Infrared Astronomy (SOFIA) The Stratospheric Observatory for Infrared Astronomy (SOFIA) a and E. E. Becklin b a University of Minnesota b Universities Space Research Association This talk is at: http://www.sofia.usra.edu/science/speakers/index.html

More information

SOFIA. Science Operations of an Airborne Observatory

SOFIA. Science Operations of an Airborne Observatory Science Operations of an Airborne Observatory Dr.-Ing. Thomas Keilig Deutsches Institut (DSI) University of Stuttgart keilig@dsi.uni-stuttgart.de, Pfaffenwaldring 29, 70569 Stuttgart, Germany 1 What is?

More information

NASA IRTF and Synergies with SOFIA

NASA IRTF and Synergies with SOFIA 1 NASA IRTF and Synergies with SOFIA Eric Becklin SOFIA/USRA Chief Scientific Advisor Professor Emeritus UCLA NASA IRTF: Future Directions Workshop Biosphere 2, Tucson AZ Feb. 14, 2018 2 Outline of Material

More information

SOFIA Science Metrics Update

SOFIA Science Metrics Update SOFIA Science Metrics Update Bill Reach SOFIA Deputy SMO Director WReach@usra.edu Astrophysics Advisory Committee NASA Headquarters July 2017 Kimberly Ennico Smith NASA SOFIA Project Scientist Kimberly.Ennico@nasa.gov

More information

Launching Astronomers into the Stratosphere

Launching Astronomers into the Stratosphere Launching Astronomers into the Stratosphere Dan Lester University of Texas DFL 2/19/2010 Next-Generation Suborbital Researchers Conference 1 Considering NGSR, note the path blazed by airborne platforms

More information

Telescopes and the Atmosphere

Telescopes and the Atmosphere Telescopes and the Atmosphere Our goals for learning How does Earth s atmosphere affect ground-based observations? Why do we put telescopes into space? How does Earth s atmosphere affect ground-based observations?

More information

SOFIA Science Highlights Cycle 4 Progress Cycle 5 Call for Proposals

SOFIA Science Highlights Cycle 4 Progress Cycle 5 Call for Proposals SOFIA Science Highlights Cycle 4 Progress Cycle 5 Call for Proposals Erick Young SOFIA Science Center Executive Summary Since Last SUG Completed Cycle 3 319 GI Time 122 GTO Time 5 DDT Horsehead Nebula

More information

Todays Topics 3/19/2018. Light and Telescope. PHYS 1403 Introduction to Astronomy. CCD Camera Makes Digital Images. Astronomical Detectors

Todays Topics 3/19/2018. Light and Telescope. PHYS 1403 Introduction to Astronomy. CCD Camera Makes Digital Images. Astronomical Detectors PHYS 1403 Introduction to Astronomy Light and Telescope Chapter 6 Todays Topics Astronomical Detectors Radio Telescopes Why we need space telescopes? Hubble Space Telescopes Future Space Telescopes Astronomy

More information

The Stratospheric Observatory for Infrared Astronomy (SOFIA)

The Stratospheric Observatory for Infrared Astronomy (SOFIA) The Stratospheric Observatory for Infrared Astronomy (SOFIA) R. D. Gehrz Lead, SOFIA Community Task Force Department of Astronomy, University of Minnesota This talk will be available at http://www.sofia.usra.edu/science/speakers/index.html

More information

Planetary Science with SOFIA. William T. Reach SOFIA Community Day University of Arizona May 2016

Planetary Science with SOFIA. William T. Reach SOFIA Community Day University of Arizona May 2016 Planetary Science with SOFIA William T. Reach SOFIA Community Day University of Arizona May 2016 Quick tour of possibilities Terrestrial Planets Mercury: not visible Venus: atmosphere composition, dynamics

More information

Light and Telescopes

Light and Telescopes Light and Telescopes The key thing to note is that light and matter interact. This can happen in four principal ways: 1) emission a hot object such as the filament in a light bulb emits visible light 2)

More information

Outline HST HST. HST& JWST CARMA and ALMA SOFIA Chandra Blackbodies. Doppler Effect. Homework #5 was due today.

Outline HST HST. HST& JWST CARMA and ALMA SOFIA Chandra Blackbodies. Doppler Effect. Homework #5 was due today. Outline Homework #5 was due today. Next homework is #6 due next Friday at 11:50 am. There will be another make-up nighttime observing session in November. Stay tuned. I will be teaching Paul s class on

More information

SOFIA Science Capabilities and Instrument Overview

SOFIA Science Capabilities and Instrument Overview SOFIA Science Capabilities and Instrument Overview Bernhard Schulz with lots of help from Andrew Helton, Bill Vacca, B-G Andersson, Raquel Destefano, Kimberly Ennico Smith, Bill Reach Atmospheric Transparency

More information

Educational Product Teachers Grades K-12 EG MSFC

Educational Product Teachers Grades K-12 EG MSFC Educational Product Teachers Grades K-12 NASA Spacelink Optics: An Educators Guide With Activities In Science and Mathematics is available in electronic format through NASA Spacelink one of the Agency

More information

Our View of the Milky Way. 23. The Milky Way Galaxy

Our View of the Milky Way. 23. The Milky Way Galaxy 23. The Milky Way Galaxy The Sun s location in the Milky Way galaxy Nonvisible Milky Way galaxy observations The Milky Way has spiral arms Dark matter in the Milky Way galaxy Density waves produce spiral

More information

What is Earth Science?

What is Earth Science? What is Earth Science? A.EARTH SCIENCE: the study of Earth and its history B. Earth science is divided into 4 main branches: 1. Geology: study of the lithosphere 2. Oceanography: study of oceans 3. Meteorology:

More information

The Stratospheric Observatory for Infrared Astronomy (SOFIA): Infrared Sensor Development and Science Capabilities

The Stratospheric Observatory for Infrared Astronomy (SOFIA): Infrared Sensor Development and Science Capabilities The Stratospheric Observatory for Infrared Astronomy (SOFIA): Infrared Sensor Development and Science Capabilities Joel E. Nelson Agilex Technologies, Inc. Martin J. Ruzek Universities Space Research Association

More information

Benefits of Infrared. The Spitzer Space Telescope. Instruments/Components of Spitzer. Cryostat. Infrared Telescope

Benefits of Infrared. The Spitzer Space Telescope. Instruments/Components of Spitzer. Cryostat. Infrared Telescope The Spitzer Space Telescope Benefits of Infrared IR can reveal objects that don't emit visible light IR provides different information than visible light IR is better than visible for viewing cold objects

More information

THE EMISSION AND DISTRIBUTION OF DUST OF THE TORUS OF NGC 1068

THE EMISSION AND DISTRIBUTION OF DUST OF THE TORUS OF NGC 1068 THE EMISSION AND DISTRIBUTION OF DUST OF THE TORUS OF NGC 1068 ENRIQUE LOPEZ RODRIGUEZ Instrument Scientist (HAWC+) Stratospheric Observatory For Infrared Astronomy (SOFIA) / NASA elopezrodriguez@nasa.gov

More information

A Science Vision for SOFIA

A Science Vision for SOFIA A Science Vision for SOFIA 3 March 2017 Harold W Yorke Director, SOFIA Science Mission Operations Setting the Stage (1/3) For NASA s space missions, Level 1 requirements are sacrosanct (NPR 7120.5E) Level

More information

AST4930: Star and Planet Formation. Syllabus. AST4930: Star and Planet Formation, Spring 2014

AST4930: Star and Planet Formation. Syllabus. AST4930: Star and Planet Formation, Spring 2014 AST4930: Star and Planet Formation Lecture 1: Overview Assoc. Prof. Jonathan C. Tan jt@astro.ufl.edu Bryant 302 Syllabus AST4930: Star and Planet Formation, Spring 2014 Assoc. Prof. Jonathan C. Tan (jt

More information

Chapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization

Chapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization Objectives Describe characteristics of the universe in terms of time, distance, and organization Identify the visible and nonvisible parts of the electromagnetic spectrum Compare refracting telescopes

More information

The skin of Orion. Molecular Astrophysics: The Herschel and ALMA era PRESS RELEASE

The skin of Orion. Molecular Astrophysics: The Herschel and ALMA era PRESS RELEASE Molecular Astrophysics: The Herschel and ALMA era PRESS RELEASE The skin of Orion 9- October- 2015 Imaging Orion in ionized carbon emission. Among the brightest emissions from the interstellar medium and

More information

The High Resolution Spectrometer for SOFIA

The High Resolution Spectrometer for SOFIA Slide 1 The High Resolution Spectrometer for SOFIA Gerónimo Villanueva Max Planck Institut für Aeronomie November 00 Index SOFIA Observatory Atmospheric transmission and sensitivity GREAT-CTS Project Scientific

More information

Stellar Life Cycle in Giant Galactic Nebula NGC edited by David L. Alles Western Washington University

Stellar Life Cycle in Giant Galactic Nebula NGC edited by David L. Alles Western Washington University Stellar Life Cycle in Giant Galactic Nebula NGC 3603 edited by David L. Alles Western Washington University e-mail: alles@biol.wwu.edu Introduction NGC 3603 is a giant HII region in the Carina spiral arm

More information

Notes: Reference: Merline, W. J. and S. B. Howell (1995). "A Realistic Model for Point-sources Imaged on Array Detectors: The Model and Initial

Notes: Reference: Merline, W. J. and S. B. Howell (1995). A Realistic Model for Point-sources Imaged on Array Detectors: The Model and Initial Notes: Notes: Notes: Reference: Merline, W. J. and S. B. Howell (1995). "A Realistic Model for Point-sources Imaged on Array Detectors: The Model and Initial Results." Experimental Astronomy 6: 163-210.

More information

HST Observations of Planetary Atmospheres

HST Observations of Planetary Atmospheres HST Observations of Planetary Atmospheres John T. Clarke Boston University Hubble Science Legacy 3 April 2002 Venus - Near-UV images reveal cloud motions and winds - UV spectra track SO 2 composition,

More information

Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical

Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical Trigonometry p. 9 The Earth p. 12 The Celestial Sphere p. 14 The

More information

Methane in Mars Atmosphere: Evidence for Life or Uncertain Detections?

Methane in Mars Atmosphere: Evidence for Life or Uncertain Detections? Design Reference Mission Case Study Stratospheric Observatory for Infrared Astronomy Science Steering Committee Methane in Mars Atmosphere: Evidence for Life or Uncertain Detections? Program contacts:

More information

Directed Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past?

Directed Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past? Skills Worksheet Directed Reading Section: Viewing the Universe 1. How did observations of the sky help farmers in the past? 2. How did observations of the sky help sailors in the past? 3. What is the

More information

arxiv: v1 [astro-ph.im] 3 May 2012

arxiv: v1 [astro-ph.im] 3 May 2012 Accepted by ApJL 2012 January 24 Preprint typeset using L A TEX style emulateapj v. 5/2/11 EARLY SCIENCE WITH SOFIA, THE STRATOSPHERIC OBSERVATORY FOR INFRARED ASTRONOMY arxiv:1205.0791v1 [astro-ph.im]

More information

Searching for Other Worlds

Searching for Other Worlds Searching for Other Worlds Lecture 32 1 In-Class Question What is the Greenhouse effect? a) Optical light from the Sun is reflected into space while infrared light passes through the atmosphere and heats

More information

Detectors for IR astronomy

Detectors for IR astronomy Detectors for IR astronomy Where does infrared begin? Wavelength sensi?vity of the human eye vs. wavelength Note: the eye has some (limited) sensi?vity to IR light at ~1000nm (=0.5x energy of photons the

More information

Great Observatories Galactic Center Region Image Unveiling Science Telecon. October 6, 2009

Great Observatories Galactic Center Region Image Unveiling Science Telecon. October 6, 2009 Great Observatories Galactic Center Region Image Unveiling Science Telecon October 6, 2009 1 Multiwavelength Observations Dr. Frank Summers 2 3 4 Support Web Site http://hubblesource.stsci.edu/events/iyafinale/support/

More information

The Stratospheric Observatory for Infrared Astronomy (SOFIA)

The Stratospheric Observatory for Infrared Astronomy (SOFIA) The Stratospheric Observatory for Infrared Astronomy (SOFIA) R. D. Gehrz Lead, SOFIA Community Task Force Department of Astronomy, University of Minnesota 1 University of Washington, Seattle, WA, February

More information

SOFIA: First Light to First Science

SOFIA: First Light to First Science SOFIA: First Light to First Science FORCAST Team members: Terry Herter (Principal Investigator), Joe Adams (Project Scientist), George Gull (Lead Engineer), Justin Schoenwald (Software Engineer), Chuck

More information

Transneptunian objects. Minor bodies in the outer Solar System. Transneptunian objects

Transneptunian objects. Minor bodies in the outer Solar System. Transneptunian objects Transneptunian objects Minor bodies in the outer Solar System Planets and Astrobiology (2016-2017) G. Vladilo Around 1980 it was proposed that the hypothetical disk of small bodies beyond Neptune (called

More information

Galactic Center. Exploring. the. A case study of how USRA answered a question posed by James Webb in 1966.

Galactic Center. Exploring. the. A case study of how USRA answered a question posed by James Webb in 1966. Exploring Volodymyr Goinyk/Shutterstock.com the Galactic Center A case study of how USRA answered a question posed by James Webb in 1966. (5) Should we change the orientation of some of our NASA Centers?

More information

The Interstellar Medium in Galaxies: SOFIA Science

The Interstellar Medium in Galaxies: SOFIA Science The Interstellar Medium in Galaxies: SOFIA Science Margaret Meixner (STScI) Xander Tielens (NASA/Ames/Leiden Univ.), Jesse Dotson (NASA/ARC), Bruce Draine (Princeton), Mark Wolfire (U. Maryland), Jackie

More information

AST 101 INTRODUCTION TO ASTRONOMY SPRING MIDTERM EXAM 2 TEST VERSION 1 ANSWERS

AST 101 INTRODUCTION TO ASTRONOMY SPRING MIDTERM EXAM 2 TEST VERSION 1 ANSWERS AST 101 INTRODUCTION TO ASTRONOMY SPRING 2008 - MIDTERM EXAM 2 TEST VERSION 1 ANSWERS Multiple Choice. In the blanks provided before each question write the letter for the phrase that best answers the

More information

Number of Stars: 100 billion (10 11 ) Mass : 5 x Solar masses. Size of Disk: 100,000 Light Years (30 kpc)

Number of Stars: 100 billion (10 11 ) Mass : 5 x Solar masses. Size of Disk: 100,000 Light Years (30 kpc) THE MILKY WAY GALAXY Type: Spiral galaxy composed of a highly flattened disk and a central elliptical bulge. The disk is about 100,000 light years (30kpc) in diameter. The term spiral arises from the external

More information

Astronomy 1504/15014 Section 20

Astronomy 1504/15014 Section 20 1 point each Astronomy 1504/15014 Section 20 Midterm 1 (Practice Exam) September 21, 2015 Exam Version A Choose the answer that best completes the question. Read each problem carefully and read through

More information

Beyond the Visible -- Exploring the Infrared Universe

Beyond the Visible -- Exploring the Infrared Universe Beyond the Visible -- Exploring the Infrared Universe Prof. T. Jarrett (UCT) Infrared Window Telescopes ISM -- Galaxies Infrared Window Near-infrared: 1 to 5 µm Mid-infrared: 5 to 50 µm

More information

Extrasolar Planets: Molecules and Disks

Extrasolar Planets: Molecules and Disks Extrasolar Planets: Molecules and Disks The basic question: Is our solar system typical of what we should affect around other stars (inhabited or not), or is it an unusual freak? One approach is to look

More information

Chapter 23 The Milky Way Galaxy Pearson Education, Inc.

Chapter 23 The Milky Way Galaxy Pearson Education, Inc. Chapter 23 The Milky Way Galaxy The Milky Way is our own galaxy viewed from the inside. It is a vast collection of more than 200 billion stars, planets, nebulae, clusters, dust and gas. Our own sun and

More information

Career Exploration: Science, Technology, Engineering, and Math (STEM)

Career Exploration: Science, Technology, Engineering, and Math (STEM) Career Exploration: Science, Technology, Engineering, and Math (STEM) What is the Career Exploration Lab? Six (6) 3D Printers Large wall mounted touchscreen monitor Accessible design software Located in

More information

The Milky Way Galaxy

The Milky Way Galaxy 1/5/011 The Milky Way Galaxy Distribution of Globular Clusters around a Point in Sagittarius About 00 globular clusters are distributed in random directions around the center of our galaxy. 1 1/5/011 Structure

More information

Clicker Question: Clicker Question: Clicker Question:

Clicker Question: Clicker Question: Clicker Question: Test results Last day to drop without a grade is Feb 29 Grades posted in cabinet and online F D C B A In which direction would the Earth move if the Sun s gravitational force were suddenly removed from

More information

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS) Page1 Earth s Formation Unit [Astronomy] Student Success Sheets (SSS) HS-ESSI-1; HS-ESS1-2; HS-ESS1-3; HS-ESSI-4 NGSS Civic Memorial High School - Earth Science A Concept # What we will be learning Mandatory

More information

Energy. mosquito lands on your arm = 1 erg. Firecracker = 5 x 10 9 ergs. 1 stick of dynamite = 2 x ergs. 1 ton of TNT = 4 x ergs

Energy. mosquito lands on your arm = 1 erg. Firecracker = 5 x 10 9 ergs. 1 stick of dynamite = 2 x ergs. 1 ton of TNT = 4 x ergs Energy mosquito lands on your arm = 1 erg Firecracker = 5 x 10 9 ergs 1 stick of dynamite = 2 x 10 13 ergs 1 ton of TNT = 4 x 10 16 ergs 1 atomic bomb = 1 x 10 21 ergs Magnitude 8 earthquake = 1 x 10 26

More information

Exoplanets Direct imaging. Direct method of exoplanet detection. Direct imaging: observational challenges

Exoplanets Direct imaging. Direct method of exoplanet detection. Direct imaging: observational challenges Black body flux (in units 10-26 W m -2 Hz -1 ) of some Solar System bodies as seen from 10 pc. A putative hot Jupiter is also shown. The planets have two peaks in their spectra. The short-wavelength peak

More information

Herschel and Planck: ESA s New Astronomy Missions an introduction. Martin Kessler Schloss Braunshardt 19/03/2009

Herschel and Planck: ESA s New Astronomy Missions an introduction. Martin Kessler Schloss Braunshardt 19/03/2009 Herschel and Planck: ESA s New Astronomy Missions an introduction Martin Kessler Schloss Braunshardt 19/03/2009 Missions in Operations Rosetta Hubble Integral Newton Mars Express SOHO Ulysses Cluster Venus

More information

Fundamental Astronomy

Fundamental Astronomy H. Karttunen P. Kroger H. Oja M.Poutanen K.J. Donner (Eds.) Fundamental Astronomy Fifth Edition With 449 Illustrations Including 34 Colour Plates and 75 Exercises with Solutions < J Springer VII 1. Introduction

More information

Gas 1: Molecular clouds

Gas 1: Molecular clouds Gas 1: Molecular clouds > 4000 known with masses ~ 10 3 to 10 5 M T ~ 10 to 25 K (cold!); number density n > 10 9 gas particles m 3 Emission bands in IR, mm, radio regions from molecules comprising H,

More information

Radio spectroscopy. Annoying question at a NSF Science and Technology Center Review

Radio spectroscopy. Annoying question at a NSF Science and Technology Center Review Radio spectroscopy A. Harris Image: part of an H-ATLAS field as seen in the Herschel-SPIRE 250/350/500 m bands H-ATLAS: Eales et al., PASP 2010 Annoying question at a NSF Science and Technology Center

More information

Properties of Thermal Radiation

Properties of Thermal Radiation Observing the Universe: Telescopes Astronomy 2020 Lecture 6 Prof. Tom Megeath Today s Lecture: 1. A little more on blackbodies 2. Light, vision, and basic optics 3. Telescopes Properties of Thermal Radiation

More information

Clicker Question: Clicker Question: What is the expected lifetime for a G2 star (one just like our Sun)?

Clicker Question: Clicker Question: What is the expected lifetime for a G2 star (one just like our Sun)? How Long do Stars Live (as Main Sequence Stars)? A star on Main Sequence has fusion of H to He in its core. How fast depends on mass of H available and rate of fusion. Mass of H in core depends on mass

More information

Planet-like Companion to a Brown Dwarf

Planet-like Companion to a Brown Dwarf National Aeronautics and Space Administration Planet-like Companion to a Brown Dwarf Taken from: Hubble 2010: Science Year in Review Produced by NASA Goddard Space Flight Center and the Space Telescope

More information

Light and Telescopes

Light and Telescopes Light and Telescopes Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day We find them smaller and fainter, in constantly increasing numbers, and we know that we

More information

Universe Now. 2. Astronomical observations

Universe Now. 2. Astronomical observations Universe Now 2. Astronomical observations 2. Introduction to observations Astronomical observations are made in all wavelengths of light. Absorption and emission can reveal different things on different

More information

Stars, Galaxies & the Universe Lecture Outline

Stars, Galaxies & the Universe Lecture Outline Stars, Galaxies & the Universe Lecture Outline A galaxy is a collection of 100 billion stars! Our Milky Way Galaxy (1)Components - HII regions, Dust Nebulae, Atomic Gas (2) Shape & Size (3) Rotation of

More information

Stellar Life Cycle in Giant Galactic Nebula NGC 3603

Stellar Life Cycle in Giant Galactic Nebula NGC 3603 Stellar Life Cycle in Giant Galactic Nebula NGC 3603 edited by David L. Alles Western Washington University e-mail: alles@biol.wwu.edu Last Updated 2009-11-20 Note: In PDF format most of the images in

More information

Galaxies: The Nature of Galaxies

Galaxies: The Nature of Galaxies Galaxies: The Nature of Galaxies The Milky Way The Milky Way is visible to the unaided eye at most place on Earth Galileo in 1610 used his telescope to resolve the faint band into numerous stars In the

More information

An x-ray image of teeth. Can you see the filling?

An x-ray image of teeth. Can you see the filling? X-Rays APA National Aeronautics and Space Administration, Science Mission Directorate. (2010). X-Rays. Retrieved December 12, 2012, from Mission:Science website: http://missionscience.nasa.gov /ems/11_xrays.html

More information

Foundations of Astrophysics

Foundations of Astrophysics Foundations of Astrophysics Barbara Ryden The Ohio State University Bradley M. Peterson The Ohio State University Preface xi 1 Early Astronomy 1 1.1 The Celestial Sphere 1 1.2 Coordinate Systems on a Sphere

More information

ASTR 2310: Chapter 6

ASTR 2310: Chapter 6 ASTR 231: Chapter 6 Astronomical Detection of Light The Telescope as a Camera Refraction and Reflection Telescopes Quality of Images Astronomical Instruments and Detectors Observations and Photon Counting

More information

Lecture 25 The Milky Way Galaxy November 29, 2017

Lecture 25 The Milky Way Galaxy November 29, 2017 Lecture 25 The Milky Way Galaxy November 29, 2017 1 2 Size of the Universe The Milky Way galaxy is very much larger than the solar system Powers of Ten interactive applet 3 Galaxies Large collections of

More information

Telescopes 3 Feb. Purpose

Telescopes 3 Feb. Purpose Telescopes 3 Feb Key parameters of telescopes Optical telescopes SOAR Telescope, MSU s window on the universe Radio telescopes Telescopes in space SOAR Telescope Cerro Pachon, Chile First Test is Thurs

More information

The Milky Way Galaxy Guiding Questions

The Milky Way Galaxy Guiding Questions The Milky Way Galaxy Guiding Questions 1. What is our Galaxy? How do astronomers know where we are located within it? 2. What is the shape and size of our Galaxy? 3. How do we know that our Galaxy has

More information

The Milky Way Galaxy

The Milky Way Galaxy The Milky Way Galaxy Guiding Questions 1. What is our Galaxy? How do astronomers know where we are located within it? 2. What is the shape and size of our Galaxy? 3. How do we know that our Galaxy has

More information

Astro 1010 Planetary Astronomy Sample Questions for Exam 3

Astro 1010 Planetary Astronomy Sample Questions for Exam 3 Astro 1010 Planetary Astronomy Sample Questions for Exam 3 Chapter 6 1. Which of the following statements is false? a) Refraction is the bending of light when it passes from one medium to another. b) Mirrors

More information

Light and Telescopes

Light and Telescopes Light and Telescopes Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day We find them smaller and fainter, in constantly increasing numbers, and we know that we

More information

Astro 1: Introductory Astronomy

Astro 1: Introductory Astronomy Astro 1: Introductory Astronomy David Cohen Class 16: Thursday, March 20 Spring 2014 large cloud of interstellar gas and dust - giving birth to millions of stars Hubble Space Telescope: Carina Nebula

More information

Lecture Outlines. Chapter 23. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 23. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 23 Astronomy Today 8th Edition Chaisson/McMillan Chapter 23 The Milky Way Galaxy Units of Chapter 23 23.1 Our Parent Galaxy 23.2 Measuring the Milky Way Discovery 23-1 Early Computers

More information

A Tale of Star and Planet Formation. Lynne Hillenbrand Caltech

A Tale of Star and Planet Formation. Lynne Hillenbrand Caltech A Tale of Star and Planet Formation Lynne Hillenbrand Caltech Vermeer s The Astronomer (1688) Mauna Kea (last week) photos by: Sarah Anderson and Bill Bates Context: Our Sun The Sun is a completely average

More information

Chapter 26 Section 1 pages Directed Reading Section: Viewing the Universe

Chapter 26 Section 1 pages Directed Reading Section: Viewing the Universe Name: Period: Chapter 26 Section 1 pages 659-666 Directed Reading Section: Viewing the Universe 1. How did observations of the sky help sailors in the past? 2. What is the main reason people study the

More information

Astronomical Research at the Center for Adaptive Optics. Sandra M. Faber, CfAO SACNAS Conference October 4, 2003

Astronomical Research at the Center for Adaptive Optics. Sandra M. Faber, CfAO SACNAS Conference October 4, 2003 Astronomical Research at the Center for Adaptive Optics Sandra M. Faber, CfAO SACNAS Conference October 4, 2003 Science with Natural Guide Stars Any small bright object can be a natural guide star: Examples:

More information

Exoplanet Detection and Characterization with Mid-Infrared Interferometry

Exoplanet Detection and Characterization with Mid-Infrared Interferometry Exoplanet Detection and Characterization with Mid-Infrared Interferometry Rachel Akeson NASA Exoplanet Science Institute With thanks to Peter Lawson for providing material Sagan Workshop July 21, 2009

More information

The Stratospheric Observatory for Infrared Astronomy (SOFIA)

The Stratospheric Observatory for Infrared Astronomy (SOFIA) The Stratospheric Observatory for Infrared Astronomy (SOFIA) R. D. Gehrz,2,* and E. E. Becklin 2 1 Department of Astronomy, 116 Church Street, S. E., University of Minnesota, Minneapolis, MN 55455, USA

More information

Chapter 6 Light and Telescopes

Chapter 6 Light and Telescopes Chapter 6 Light and Telescopes Guidepost In the early chapters of this book, you looked at the sky the way ancient astronomers did, with the unaided eye. In chapter 4, you got a glimpse through Galileo

More information

AN INTRODUCTIONTO MODERN ASTROPHYSICS

AN INTRODUCTIONTO MODERN ASTROPHYSICS AN INTRODUCTIONTO MODERN ASTROPHYSICS Second Edition Bradley W. Carroll Weber State University DaleA. Ostlie Weber State University PEARSON Addison Wesley San Francisco Boston New York Cape Town Hong Kong

More information

Telescopes. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. Key Ideas:

Telescopes. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. Key Ideas: Telescopes A Warm Up Exercise If we measure the wavelengths of emission lines and absorption lines from the same gas, we find that (ignoring any Doppler shifts) a) Some emission lines shift to the red

More information

Telescopes have Three Powers

Telescopes have Three Powers Telescopes have Three Powers 1. Light Gathering Power: The ability to collect light 2. Resolving Power: The ability to see fine details 3. Magnifying Power: The ability to make objects look bigger Pizzas!!!

More information

Universe Now. 9. Interstellar matter and star clusters

Universe Now. 9. Interstellar matter and star clusters Universe Now 9. Interstellar matter and star clusters About interstellar matter Interstellar space is not completely empty: gas (atoms + molecules) and small dust particles. Over 10% of the mass of the

More information

GISMO. (Giant IR and SubMm Space Observatory) Tim Hawarden. UK Astronomy Technology Centre, Royal Observatory, Edinburgh

GISMO. (Giant IR and SubMm Space Observatory) Tim Hawarden. UK Astronomy Technology Centre, Royal Observatory, Edinburgh GISMO (Giant IR and SubMm Space Observatory) by Tim Hawarden UK Astronomy Technology Centre, Royal Observatory, Edinburgh (tgh@roe.ac.uk) WHY BUILD A GIANT FIR/subMM SPACE TELESCOPE? λ Fir/subMM? (difficult)

More information

Astronomy 114. Lecture 27: The Galaxy. Martin D. Weinberg. UMass/Astronomy Department

Astronomy 114. Lecture 27: The Galaxy. Martin D. Weinberg. UMass/Astronomy Department Astronomy 114 Lecture 27: The Galaxy Martin D. Weinberg weinberg@astro.umass.edu UMass/Astronomy Department A114: Lecture 27 18 Apr 2007 Read: Ch. 25,26 Astronomy 114 1/23 Announcements Quiz #2: we re

More information

Sombrero Galaxy. The Sombrero Galaxy is located on the southern edge of the rich Virgo cluster of galaxies.

Sombrero Galaxy. The Sombrero Galaxy is located on the southern edge of the rich Virgo cluster of galaxies. Sombrero Galaxy The Sombrero Galaxy is located on the southern edge of the rich Virgo cluster of galaxies. Sombrero Galaxy This galaxy is 28 million light-years away. For comparison, it takes sunlight

More information

The first six years of SOFIA Science. Observatory status and science highlights. Stratospheric Observatory For Infrared Astronomy

The first six years of SOFIA Science. Observatory status and science highlights. Stratospheric Observatory For Infrared Astronomy The first six years of SOFIA science: Observatory status and science highlights Stratospheric Observatory For Infrared Astronomy Robert Simon (I. Physikalisches Institut, Universität zu Köln) SOFIA status

More information