Bringing E.T. into Your Classroom The Search for Extra solar Planets Gary Lawhon Dave Baltenberger.

Slides:



Advertisements
Similar presentations
© 2005 Pearson Education Inc., publishing as Addison-Wesley Extrasolar Planets Since our Sun has a family of planets, shouldnt other stars have them as.
Advertisements

Destination: A Planet like Earth Caty Pilachowski IU Astronomy Mini-University, June 2011 Caty Pilachowski Mini-University 2011.
A few acknowledgements. When I first started reading about the Kepler mission, the Kepler website proved invaluable. It has a wealth of information, as.
Important Stuff (Section 3) The Final Exam is Monday, December 19, 1:30 pm – 3:30 pm The Final Exam will be given in Physics 150 Physics 150 (seats over.
Chapter 13 Other Planetary Systems The New Science of Distant Worlds.
A Search for Habitable Planets 1 NASA’s first mission to detect Earth-size planets orbiting in the habitable zone of sun-like stars. Launched March 6,
Tim Healy Tony Perry Planet Survey Mission. Introduction Finding Planets Pulsar Timing Astrometry Polarimetry Direct Imaging Transit Method Radial Velocity.
Other Planetary Systems. Detecting Extrasolar Planets  Extrasolar planets are planets orbiting other stars.  We usually detect these planets by the.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
© 2010 Pearson Education, Inc. Chapter 13 Other Planetary Systems: The New Science of Distant Worlds.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
The Next 25(?) Years Future Missions to Search for Extra-solar Planets and Life.
First direct image of extrasolar planets billion miles.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
Copyright © 2012 Pearson Education, Inc. Extrasolar Planetary Systems.
Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 4 : Astronomy Basics Ty Robinson.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
Extrasolar planets. Finding planets Finding planets around other stars is hard!  need to look for something very faint very close to something that is.
Today’s APODAPOD  Begin Chapter 8 on Monday– Terrestrial Planets  Hand in homework today  Quiz on Oncourse The Sun Today A100 – Ch. 7 Extra-Solar Planets.
6.5 Other Planetary Systems Our goals for learning: How do we detect planets around other stars? How do extrasolar planets compare with those in our own.
Lecture 34. Extrasolar Planets. reading: Chapter 9.
Astro 101 Slide Set: Kepler’s Exoplanet Discoveries Exceed 1,000 0 Topic: Exoplanets Concepts: Transit Detection, Exoplanet Statistics Mission: Kepler.
AST 111 Exoplanets I.
Extra Solar Planets Just some introductory materials. A very fast moving field. My favorite website:
ISNS Phenomena of Nature 1. Imaging –use a camera to take pictures (images) –Photometry  measure total amount of light from an object 2.Spectroscopy.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
The same frequency of planets inside and outside open clusters of stars S. Meibom, G. Torres, F. Fessin et al. Nature 499, 55–58 (04 July 2013)
Hi-Tech Classrooms: Using Technology to Engage Students in Inquiry Learning GEARS: Georgians Experiencing Astronomy Research in Schools Michelle Davis.
Blayne Chang Aaron Fujioka Pd. 3. Exoplanets  “Extra-solar”  A planet that orbits a star other than our sun  Therefore is beyond the solar system with.
Lecture Outline Chapter 10: Other Planetary Systems: The New Science of Distant Worlds © 2015 Pearson Education, Inc.
Copyright © 2012 Pearson Education, Inc. How do we detect planets around other stars?
2011: TWO MAJOR DEVELOPMENTS IN ASTRONOMY AND THE SPACE PROGRAM.
Intelligent life in the Universe? The end of the class.
Bringing E.T. into Your Classroom The Search for Extra solar Planets Gary Lawhon Dave Baltenberger.
Extrasolar Planets Instructor: Calvin K. Prothro; P.G., CPG (John Rusho) Section 003: F343, T Th 11:00 p.m. to 12:15 p.m. Section 004: F381, T Th 12:30.
Lecture 14: The Discovery of the World of Exoplanets Indirect methods for planet detection The Astrometric method The Doppler shift method The Transit.
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.
Extrasolar Planets Exo planets are planets outside the Solar System. They orbit another star. 861 confirmed…18,000 identified, but likely billions exist.
Lecture 34 ExoPlanets Astronomy 1143 – Spring 2014.
The Search for Life in the Universe. Criteria Defining Life 1.Made up of one or more cells 2.Organized 3.Grows & develops 4.Reproduces 5.Responds to stimuli.
Atoms & Starlight (Chapter 6).
NASA’s Kepler and K2 Missions:
2003 UB313: The 10th Planet?. Extra-Solar or Exoplanets Planets around stars other than the Sun Difficult to observe Hundreds discovered (> 2000 so far)
2003 UB313: The 10th Planet?. Extra-Solar or Exoplanets Planets around stars other than the Sun Difficult to observe Hundreds discovered (> 2000 so far)
Kepler Mission. Transit Method Planetary transits cause some light from a star to be blocked. The change in light is small for exoplanets. –Hard to detect.
 Understand how our view of the solar system has changed over time and how discoveries made have led to our changing our view of the solar system.  Learn.
The Search for Another Earth Exoplanets and the Kepler Spacecraft.
Lecture Outline Chapter 10: Other Planetary Systems: The New Science of Distant Worlds.
Extrasolar planets - exoplanets Planets have been discovered orbiting other stars. The list of confirmed exoplanets has over 1900.list Evidence comes from.
Exoplanets: Direct Search Methods 31 March 2016 © 2014 Pearson Education, Inc.
The Search for Another Earth. Exoplanets and the Kepler Space Telescope An exoplanet or extrasolar planet is a planet that orbits a star other than the.
Searching for Alien Worlds. Methods of Searching for Alien Planets Pulsar Timing Astrometry Radial Velocity Transits Lensing Imaging.
Chapter 10: Other Planetary Systems: The New Science of Distant Worlds
Exoplanets: Indirect Search Methods
Chapter 13 Other Planetary Systems
Our Solar System & Exoplanets
Exoplanets: The New Science of Distant Worlds
Exoplanets EXOPLANETS Talk prepared by: Santanu Mohapatra(14PH20032)
Last Friday: Solar System Highlights: Real footage of Saturn & Jupiter
extrasolar = outside of (external to) our solar system
Our Solar System & Exoplanets
Goal: To learn about the Kepler Mission and the Transit Method
Extrasolar Planets.
Knowledge: meeting the learning goals and expectations.
Current Event Due Friday!
Extrasolar planets - exoplanets
Pulsar Timing Score = 33 How it works
Our Solar System & Exoplanets
11/28/17—Astronomy Warm-Up: Write 3 things you know about the Milky Way galaxy. Bring laptops/project materials MONDAY!! SCSh1. Students will evaluate.
Presentation transcript:

Bringing E.T. into Your Classroom The Search for Extra solar Planets Gary Lawhon Dave Baltenberger

Nebular theory of solar system formation would lead us to believe planets should be associated with most stars.

Why are these planets so hard to find?

Planets are really small If the Sun is a grapefruit on the West coast of US then The Earth is a pinhead about 15 meters away and Jupiter is a marble 80 meters away and The nearest star to our solar system is on the East coast………….so You are trying to find a pinhead on a grapefruit about 2500 miles away plus the star is a billion times brighter than its planets

How can we find Extra solar Planets? Direct Detection Despite advances in technology it is difficult to find extra solar planets using direct detection

Direct Detection First image of an exoplanet? In July 2004 a group of astronomers led by Gael Chauvin took this image of a planetary-mass object in orbit around brown dwarf 2M1207. Credit: NaCo, VLT, ESO

How can we find Extra solar Planets? If we can’t just find these extra solar planets in a telescope how do we know they exist? Whiteboard What other methods could astronomers use to find extra solar planets?

Does a Planet influence its Star? All objects in the solar system orbit a common center of mass Sun is so large that this center of mass is inside the Sun

Center of Mass

Orbiting planet causes its star to “wobble”

Doppler Effect Worksheet

Can We Detect Extrasolar Planets using other Methods? Transit method: A planet passing it front of its star produces a change in brightness of 1/10,000 lasting for 2 to 16 hours Can we detect that? Credit: NASA

Kepler mission The Kepler spacecraft lifted off March 6, 2009

Kepler field of view

Based on simulator, which criteria makes it easier to find planets using the transit method. If it doesn't matter, write EQUAL CHANCE 1.Less massive stars or more massive stars. 2.Planets with orbits that are closer to circular or highly elliptical orbits. 3.Face-on orbits or edge-on orbits. 4.Small diameter planets or large diameter planets. 5.Small mass planets or large mass planets. 6.Planets close to star or planets far from star.

Whiteboard Based on these observations in the simulator, what types of planets around what types of stars would be easier to find?

Analyze Kepler data Download data from Kepler website for first five extra solar planets found by Kepler Make graph in Excel Determine period of planet Calculate: –Distance of planet from star –Surface temperature of planet –Radius of planet

Kepler Data Analysis

Excel graph from Kepler data

Answers

Habitable zone Simulator mations/stellarHabitableZone.html Discussion Biology: silicon / arsenic based life Water needed???

Where are we now in search for extra solar planets? ssions_index.cfmhttp://planetquest.jpl.nasa.gov/missions/mi ssions_index.cfm

Kepler Mission “Follow Up Observing Program” Program of ground based observations to confirm that a Kepler planet candidate is actually a planet Possible false positive = Binary star system

Kepler Mission “Follow Up Observing Program” Detecting False Positives Image of star using “adaptive optics” of the 5-meter Palomar telescope and the MMT telescope on Mt. Hopkins. These high quality images are able to detect an eclipsing binary star

Kepler Mission “Follow Up Observing Program” Detecting False Positives Eclipsing binary stars exhibit two distinct spectra one on top of the other, but displaced from each other by the Doppler Effect. An eclipsing binary star would exhibit two different speed readings in its spectrum of colors, betraying the existence of two orbiting stars whizzing around each other.

Kepler Mission “Follow Up Observing Program” Doppler Effect used to: 1.Verify a planet candidate by the wobble it causes on host star 2.Calculate the mass of planet; more massive planet causes more Doppler shift 3.Density using mass and diameter (from transit measurement)

Extra Solar planet news s/gliese_581_feature.html

New Method to Validate Extra solar Planets Action=ShowNews&NewsID=127 s/gliese_581_feature.html

planethunters.org

Detecting Extra solar Planets Use star wobble to detect planets –Wobbling star models Kepler looks for dimming of the star to detect presence of extra solar planet –Use Kepler data to create Excel graphs to identify pattern of star dimming –Use websites to recreate hunt for extra solar planets

GPS Standards Astronomy – SAST6 – Students will explore connections between cosmic phenomena and conditions necessary for life. Physical Science - SPSP9 – Students will investigate the properties of waves. f) Explain the Doppler Effect in terms of everyday interactions. (Doppler shift of spectral lines & radial velocity) Biology – SB1 – Students will analyze the nature of relationships between structures and functions in living cells. d) Explain the impact of water on life processes. SB5 – Students will evaluate the role of natural selection in the development of the theory of evolution. (concepts of what defines the “habitable zone” can be brought in here)

GPS Standards Earth Systems – SES1 – Students will investigate the composition and formation of Earth systems, including Earth’s relationship to the solar system. (habitable zone) Chemistry SC3 – Students will use modern atomic theory to explain the characteristics of atoms. f) Relate light emission and movement of electrons to element identification. (spectroscopy and detection by radial velocity/Doppler shift) SC4 – Student will use the organization of the Periodic Table to predict properties of elements. b) Compare and contrast trends in the chemical and physical properties of elements and their placement on the Periodic Table. (concepts of Habitable Zone, carbon-based life vs. thoughts on silicon-based life. Also water vs. ammonia)

GPS Standards Environmental Science – SEV2 – Students will demonstrate an understanding that the Earth is one interconnected system. a) Describe how the abiotic components (water, air, and energy) affect the biosphere. (Habitable Zone)

Astronomy Themed Summer Workshops: Chem., Physics, Phys. Sci. GPS High School Teachers Only This Year Search for Life in the Universe Sun Earth Connection: Space Weather Stars: Formation of the Elements Crash, Bang, Galaxies! for This workshop funded by NASA Office of Education Grant NNX09AH83A and supported by the Georgia Department of Education, Columbus State University, and Georgia Southern University