Dr. Tracy L. Beck Exploring the Universe and Our Origins.

Slides:



Advertisements
Similar presentations
The Solar System By Level Two.
Advertisements

OUR COSMIC ADDRESS Each of us has an address. Ours is: The Denver Museum of Nature and Science 2001 Colorado Blvd. Denver, Colorado But what.
Exoplanet Atmospheres: Insights via the Hubble Space Telescope Nicolas Crouzet 1, Drake Deming 2, Peter R. McCullough 1 1 Space Telescope Science Institute.
National College RomaniaCassiopeiae Team Made by Alexandra Birladeanu and Gina Ioana Ursu.
Tim Healy Tony Perry Planet Survey Mission. Introduction Finding Planets Pulsar Timing Astrometry Polarimetry Direct Imaging Transit Method Radial Velocity.
Ch Viewing the Universe
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,
Caty Pilachowski Mini-University 2013 Our Milky Way in Space and Time.
Chapter 3. The Scale of the Universe  Astonomers deal with very large numbers on a regular basis. For this reason, they use scientific notation to make.
Astronomy Introduction. What is Astronomy? The scientific study of celestial (sky/space) objects like stars, comets, planets, and galaxies Astronomy is.
The Size and Distance Scale Of The Solar System Our Earth is just one of several Planets that revolve around our Sun, the primary and central object of.
The James Webb Space Telescope. Introduction The James Webb Space Telescope  The James Webb Space Telescope, also called Webb or JWST, is a large, space-based.
A student project. What is a space telescope?  A space telescope is a telescope that orbits around Earth in space.  Like other telescopes they take.
Part I: A Trip Through the Universe “Our Transportation” STARS AND GALAXIES 1.
The Eye of Our Universe The Whirlpool Galaxy, starburst type. NASA and the Space Telescope Science Institute unitedstreaming. 2 November 2005 Marianne.
The top image, which shows half of the surveyed area, displays nine different stars, circled in green, that contain planets. The planets were discovered.
Cosmic Survey: What are Your Ideas about the Universe?
NEXT Player 1 Player 2 Player 3 Player
Stars, Galaxies, and the Universe.  To understand how telescopes work, its useful to understand the nature of the electromagnetic radiation. Light is.
PLUTO AND THE KUIPER BELT Beyond Neptune, the most distant major planet, are a large number of smaller objects, all of which currently known are smaller.
Components of the Universe Lesson 3. Universe All of the things that exist in space.
The three brighter objects are Venus (center), Mercury (below) and Saturn (left). What is the difference between stars and planets?
Our Solar System Assignment #44. The Universe The universe is everything that is. The universe is comprised of billions of galaxies, which are comprised.
Galaxies Hubble Deep Field – taken by the Hubble telescope above the Earth.
Just how big is big? To do this, we need to make a model.
Galaxies & Star Systems Astronomy 2. Star Systems Our solar system only has one star (our sun); however, most are grouped together to groups of two or.
STARS BY SEYMOUR SIMON. Stars are huge balls of hot gases Our sun is a star, and it is the star nearest our planets Earth and our solar system Other stars.
Assessment 9: Size of the Universe
Astronomy and the Electromagnetic Spectrum
SPACE SYSTEMS UNIT Chapters 26 & 30.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
NASA and us Ms. Wood. Things you should know Moon revolves around sun as it revolves around Earth Millions of galaxies Solar system is made of: Sun Planets.
 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.
Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ The First Images of Exoplanets New images show planets orbiting bright young nearby.
Our Solar system YouTube - The Known Universe by AMNH.
What is the Big Bang? The Big Bang theory is an effort to explain what happened at the very beginning of our universe about 15 Billion years ago.
Key Ideas Describe characteristics of the universe in terms of time, distance, and organization. Identify the visible and nonvisible parts of the electromagnetic.
Worlds around Distant Suns Mini University June 16, 2003 Among the most significant discoveries of the 20th Century.
2011: TWO MAJOR DEVELOPMENTS IN ASTRONOMY AND THE SPACE PROGRAM.
The Stars Chapter 14 Great Idea: The Sun and other stars use nuclear fusion reactions to convert mass into energy. Eventually, when a star’s nuclear fuel.
Exploring the far reaches of the universe. Hubble Telescope By Blake Shaffer.
6.3 Telescopes and the Atmosphere 6.4 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does Earth’s atmosphere affect ground-based observations?
Search for Extra-Solar Planets. Background 1995 first discovered evidence that other stars have planets first discovered evidence that other stars.
Our Universe Billions of galaxies made up of billions of stars.
Extrasolar Planets The Search For Ever since humans first gazed into the night sky, the question of whether we are alone in the universe has remained unanswered.
Telescopes Key Words Optical Telescopes: make use of electromagnetic radiation in the range of visible light Refraction Telescopes: use lenses Reflecting.
Astronomy Astronomy the scientific study of the universe Scientists who study the universe are called astronomers Early Astronomers includes: Nicolaus.
1 The Milky Way Galaxy We live on the quiet outskirts of a galaxy of approximately 100 Billion stars. This galaxy, the Milky Way, is roughly disk-shaped.
The Basic Structure of the Universe. What is the Universe? All matter and energy, including the earth, all the galaxies, and the contents of intergalactic.
Theme 6 – Space Telescopes and Adaptive Optics ASTR 101 Prof. Dave Hanes.
Answer the following question about yesterday’s activity at the bottom of page 21 Explain how you decided how many groups of galaxies you would have. What.
Welcome to the Milky Way Galaxy
2003 UB313: The 10th Planet?. Extra-Solar or Exoplanets Planets around stars other than the Sun Difficult to observe Hundreds discovered (> 2000 so far)
Satellites, Telescopes, Probes and Rovers
The Search for Another Earth Exoplanets and the Kepler Spacecraft.
How astronomers study space. Electromagnetic Radiation (EMR) Light can travel through empty space All EMR travels at the speed of light  3 x 10 8 m/sec.
Exploring the Universe, Galaxies. What were some things you noticed about the cards you sorted yesterday? How were the cards from yesterday different.
Exploring Space: The Universe Exploring Space: The Universe.
The Universe & Galaxies Key Point (Std 8-4.9): Recall the Sun’s position in the universe, the shapes and composition of galaxies, and the distance measurement.
Unit 2 The Earth in Space The Universe. “ A book of knowledge is spread out before us in the pageant of the heavens, but we cannot turn the pages. All.
The Solar System. Our Solar System The Sun Mercury 0 moons Venus 0 moons Earth 1 moon Mars 2 moons Jupiter 67 moons Saturn 62 moons Uranus 27 moons Neptune.
The Universe and Electromagnetic Spectrum
Galaxies This lesson deals with important topics relating to galaxies. Each of these topics represents a great body of knowledge and areas of interest.
The Universe in the Infrared
Galaxies This lesson deals with important topics relating to galaxies. Each of these topics represents a great body of knowledge and areas of interest.
The Universe and Electromagnetic Spectrum
Astronomy-Part 1 Notes The Structure of the Universe
The Universe.
Copy week schedule into your agenda and answer the Question of the Day
Our Solar System.
Presentation transcript:

Dr. Tracy L. Beck Exploring the Universe and Our Origins

The Nature of Light…

Why We go to space - Earth’s Atmospheric Transmission! Gamma Rays X Rays UltraViolet InfraRed Many kinds Of light are Blocked by earth’s Atmosphere ! Where Hubble works Radio

Why we go to space - Hubble vs. ground-based telescopes - image quality! Air in the earth’s atmosphere causes astronomical images to be blurry! Twinkle, twinkle little star…! Subaru Observatory (~27ft!) HST

After SM4 in May 2009 we have 2 new instruments! 2 Fixed Instruments! We The NEW and Improved Hubble!! Ultraviolet Infrared Wide Field Camera 3 (WFC3) Advanced Camera for Surveys (ACS) Gas flowing away from a dying star! Dense gas lit by nearby stars! Spiral Galaxy Galaxy Cluster

Hubble Space Telescope - the single most productive and popular Astronomical Tool… EVER! HAPPY 20th Anniversary, HUBBLE! Launched April 24, 1990

The James Webb Space Telescope (JWST) Scheduled for launch in 2014, JWST is the successor to Hubble - (there’s NO REPLACING it!) Goal of JWST - Continue the spirit of Hubble to explore our universe, from understanding comets and planets in our own solar system, to the most distant stars and galaxies in our universe…

Who was James Webb? Organized and Oversaw the first manned space missions in the Mercury and Gemini programs Had the foresight and knowledge to push for robotic missions, searching the moon and paving the way for all future remote studies of Venus, Mars and more recently Jupiter, Saturn… etc… He did more for organized space science research than any other person in the US ever has! James E. Webb He was the Second NASA Administrator, from 1961 to 1968.

The James Webb Space Telescope… Telescope Primary Mirror Sun Shield Telescope Secondary Mirror Sun Shield = size of a Tennis Court! Life-Size GSFC

How is JWST different? - the telescope size! Learn more at

How is JWST different? - the telescope LOCATION! The Hubble Space telescope orbits around earth at a height of ~350 miles! This is so the astronauts can reach Hubble, and fix it or upgrade it, if needed! In the infrared, we want much darker skies with no earthshine or moonshine to compete with - so JWST is going to orbit at the sun-earth “Lagrange - 2” point - roughly 930,000 miles away! Photograph of Hubble Artist Drawing of JWST ! Learn more at

What’s a “Langrange” point, and why should we put our telescope out there? “Lagrange Point” - very stable orbit point where gravity and orbital energies are perfectly balanced! There are 5 L- points, JWST is going to “L2” Not much spacecraft fuel is needed to keep JWST in orbit here! Far away from earth = very dark sky! Sun Earth L2 Learn more at

How is JWST Different - INFRARED! Many wavelengths of infrared light sampled by JWST can’t be seen by Hubble or on the ground! Learn more at

How is JWST Different - INFRARED! Some infrared light measures the HEAT from an object! (the warm dog has a cold nose!) Visible light Infrared light

How is JWST Different - INFRARED! Light at some Infrared wavelengths can pierce through clouds of dust… view in visible light is not the same as IR!

The REAL Driver for JWST is the SCIENCE! 4 Key Goals for JWST! 1) The formation of star and planet systems 2) Extra-solar planets and the origin of life in our Universe 4) The first stars and the origin of our Universe! 3) The formation of galaxies and large structures in our universe

Star and Planet Formation Clouds of gas and dust collapse due to gravity form a flattened circumstellar “disk” planets coalesce out of dust and gas in the disk Animation courtesy of M. Ressler, JPL Animation of Star+Planet Formation Large Cloud of Gas and Dust, imaged by HST+WFC3

Fomalhaut - an outer ring of dust… indicative of planet formation? Ring of Dust Light from the Young Star is blocked and subtracted off ACS Images Simulated JWST Image

Fomalhaut B!? Kalas et al. (2008) Holy cow! Is that a planet!? JWST will be able to image and study wide extent planets, as in the planet in the Fomalhaut system!

Extra-solar Planets and the Origin of LIFE in the Universe! In the very first two strong candidate exo- planets were discovered! Today, 15 years later, 429 exoplanets are known! 41 multiple planet systems! New planets are Discovered ALL THE TIME! What was science fiction a mere 15 years ago, is reality today ! One of the most rapidly growing and highest profile realms of study in modern Astronomy! JWST can have a HUGE Impact here! See more at

How are exoplanets detected? 1) Direct Imaging (as in the HST images of Fomalhaut) 2) Planet passes in front of it’s star (transit, or eclipsing planets) 3) Radial Velocity Searches 4) Microlensing (see more info at Exoplanets.org) Main methods for exo-planet detection with JWST!

What is a Transiting, or Eclipsing Exoplanet? Animation from the HST SWEEPS Project - Sagittarius Window Eclipsing Exo-Planet Survey!

What is a Transiting, or Eclipsing Exoplanet? Animation from the HST SWEEPS Project - Sagittarius Window Eclipsing Exo-Planet Survey!

How can we find an Earth-like Planet? O Type = Brightest stars M Type = Faintest Stars It’s easiest to try to find Earth- like planets around the faintest stars! Sun!

JWST will aggressively seek to study earth-like planets as they pass in front of their “M star” hosts - by measuring starlight that passes through the atmosphere of the planet! Planet atmosphere

Our sphere of search for planets is just a small area of the Milky Way! The Milky Way galaxy is a BIG place… the universe is a huge place…! Key question for JWST - How common are earth-like planets? Our Milky Way Galaxy!

The Milky way & Galaxies Galaxies - BIG Huge conglomerations of stars - Milky Way is >200,000,000 stars! We are here! Artist Image of our Milky Way Galaxy

Hubble Space Telescope Images of Galaxies… Elliptical Galaxies It’s believed that some of the galaxies that we see today formed by merging of two different galaxies at some time in the past! Spiral Galaxies Test your Galaxy Classification skills! & Help Merging Galaxies

Distance in Astronomy Light takes time to travel… so looking at objects that are further and further away means that we are looking backwards in time! This is because light travels at a fixed speed - the speed of light! Distance from… Sun to Earth 8.3 light minutes Sun to Proxima Centauri4.26 light years Sun to the center of the Milky Way26,000 light years Sun to the Andromeda Galaxy2.5 Million light years!!!

The Hubble Ultra Deep Field! WOW! Some of the faint fuzzy blobs in this picture are the most distant galaxies known in our universe - 13 BILLION light-years away! Total Exposure time = days!!

The JWST Ultra Deep Field! Astronomer simulation of what the comparable JWST deep field will look like! How deep will we see?

Will JWST Detect the First Stars Ever Formed in Our Universe? Comparison of the Hubble deep field (left) to JWST deep field (right). HST Image - 30 hrs JWST Simulation - 17 mins

The James Webb Space Telescope! From planets to the most distant galaxies, this Infrared optimized observatory scheduled for launch in 2014 will revolutionize our understanding of the universe!! We Hope to Know in ~2014!

Thanks for your attention! JWST Deploying in 2014!!

We Hubble!! Glowing gas lit by massive stars! Eruption from a dying star! Gas flowing away from a dying star! Cluster of Stars! Pillars of dense gas lit by nearby stars!