Exo-Planet Transit HD 189733b on October 16, 2005 Observation by: Thomas C. Smith Dark Ridge Observatory (DRO)

Slides:



Advertisements
Similar presentations
Stars in space By Ben and Iris. Stars of space Star Constellations Constellations are groups of stars that make a shape. each constellation has it’s own.
Advertisements

Binary Systems and Stellar Parameters The Classification of Binary Stars Mass Determination using visual Binaries Eclipsing,Spectroscopic Binaries The.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
PX437 EXOPLANETS Outline 1.Before Exoplanets 2.Detecting exoplanets 1.Direct imaging 2.Reflex Motion of Star 3.Transiting exoplanets 3.Planet Formation.
Are These Stars? Definition of a Star (1) Bound by self gravity (spherical) (1) Bound by self gravity (spherical) Is this strictly true? (2)
Somak Raychaudhury  Two-body problem  Binary stars  Visual  Eclipsing  Spectroscopic  How to find extrasolar planets.
A Profusion of Exoplanets: Key Science Results from the Kepler Mission Jon M. Jenkins SETI Institute/NASA Ames Research Center Thursday September 22, 2011.
All About Exoplanets Dimitar D. Sasselov Harvard-Smithsonian Center for Astrophysics.
Lecture 14: Searching for planets orbiting other stars III: Using Spectra 1.The Spectra of Stars and Planets 2.The Doppler Effect and its uses 3.Using.
2 The Moon and Planets A Backyard View. 2 Goals How does the Moon move through the sky? What causes its phases? What really is the “dark side” of the.
Lecture 11: The Discovery of the World of Exoplanets
Reflected Light From Extra Solar Planets Modeling light curves of planets with highly elliptical orbits Daniel Bayliss, Summer Student, RSAA, ANU Ulyana.
INSTRUMENTATION AT THE GETTYSBURG OBSERVATORY….And what to do with it. American Astronomical Society 205 th meeting, San Diego, Jan 13, 2005.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
Stargazing on Mars Stargazing on Mars Cover Page Environment Constellations Polar Axis Observing Moons Observing Mars Moon to Moon Solar Eclipses Earth.
What stellar properties can be learnt from planetary transits Adriana Válio Roque da Silva CRAAM/Mackenzie.
Nadiia Kostogryz & Svetlana Berdyugina
Cuesta College Eclipsing Binary Project Briefing In support of an ongoing Eclipsing Binary Star Project Conducted by Thomas C. Smith (Dark Ridge Observatory)
July Light pollution map. If interested in astronomy, the last place you want to be is in the Northeast.
Adriana V. R. Silva CRAAM/Mackenzie COROT /11/2005.
Gravity & orbits. Isaac Newton ( ) developed a mathematical model of Gravity which predicted the elliptical orbits proposed by Kepler Semi-major.
AST 112 Motion of Objects in the Sky. The Celestial Sphere Imagine you’re where Earth is, but there’s no Earth. What do you see? Keep in mind: – Nearest.
Analysis of a Suspected Variable Star. What is a Variable Star? Variable stars are stars that change brightness. The changes in brightness of these stars.
Search for planetary candidates within the OGLE stars Adriana V. R. Silva & Patrícia C. Cruz CRAAM/Mackenzie COROT /11/2005.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
We Live Where?! Miss Napolitano. Formation of the Solar System Nebula: birthplace of stars Star leaves nebula Star is rotating: gases and material surround.
Eclipses 5/19/ c pgs IN: Which two planets do not have moons? Why not?
The Moon’s Phases. Sun The view from Earth I.Eclipses A. A solar eclipse only occurs at a _____________. B. A lunar eclipse only occurs at a ______________.
1B11 Foundations of Astronomy Extrasolar Planets Liz Puchnarewicz
SOCHIAS Santiago, January Sergio Hoyer Miranda Departamento de Astronomía Universidad de Chile 1.
Lecture 14: The Discovery of the World of Exoplanets Indirect methods for planet detection The Astrometric method The Doppler shift method The Transit.
23 November 2015what do we know from the exo-planets? Florian Rodler What do we know about the exo-planets? & How to detect direct signals from exo-planets?
AST 111 Lecture 7 Eclipses, Solar and Sidereal Days, Precession.
Extrasolar planets. Detection methods 1.Pulsar Timing Pulsars are rapidly rotating neutron stars, with extremely regular periods Anomalies in these periods.
Spin-Orbit Alignment Angles and Planetary Migration of Jovian Exoplanets Norio Narita National Astronomical Observatory of Japan.
EXAM II COMING UP Monday Oct 19 th (a week from this coming Monday!) HW5 due a week from today.
Within-Season Changes in the Periods and Light Curves of W UMa Binaries Russ Genet Orion Observatory Tom Smith Dark Ridge Observatory Dirk Terrell Southwest.
CCD Observations and Preliminary Analysis of the “End-of-the-Line” W UMa Eclipsing Binary V523 Cas Presenting Authors: Russell M. Genet, Orion Observatory.
NASA’s Kepler and K2 Missions:
PHYS 205 Multiple Star Systems PHYS 205 Binary systems Question: Why are the binaries important?? Answer: They allow us to measure the mass of other.
Today! From Earth’s Perspective: Celestial Motion: Stellar Motion Solar Motion Planetary Motion.
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.
KEPLER TABLE OF CONTENTS Table of Contents: Mission Overview Scientific Objectives Timeline Spacecraft Target Field of View Transit Method Johannes Kepler.
Observation vs. Inferences The Local Environment.
The Search for Another Earth Exoplanets and the Kepler Spacecraft.
Nebula Images. Nebula.
Astronomy 3040 Astrobiology Spring_2016 Day-7. Homework -1 Due Monday, Feb. 8 Chapter 2: 1, 3, 16 23, 24, 26 29, 30, , 54, 56 The appendices will.
How many of these ? Out there. At least One in Six stars has an Earth-size planet Francois Fressin, G. Torres, D. Charbonneau & the team.
Motions of Earth, the Moon and Planets
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.
GCSE Astronomy.
Solar and Lunar Eclipses
Jeopardy Chapter 7 Part 2 Chapter 8 Chapter 8 Part 2 Chapter 9
The Night Sky…last time, The Horizon System
Nature of Exoplanets 26 October 2016.
Last Friday: Solar System Highlights: Real footage of Saturn & Jupiter
Solar and Lunar Eclipses
Pre-Cursor Data Needed for JWST Transit and Eclipse Observations
Michael Endl Board of Visitors Meeting - July 2009
Joel E. Tohline, Alumni Professor
Goal: To learn about the Kepler Mission and the Transit Method
The universe and us the light version
Today! From Earth’s Perspective: Celestial Motion: Stellar Motion
The nature of eclipses But first… Orbits in solar System really
An Investigation of Densities of Transit Detected Exoplanets
What is an Exoplanet? Why is their search important?
Where We Are…. As of November 21, 2016, over 3400 confirmed exoplanets had been found, with over 4500 additional candidate exoplanets. We can look at these.
A Closer Look at Microlensing
Finding Asteroids in Exoplanet Data
Presentation transcript:

Exo-Planet Transit HD b on October 16, 2005 Observation by: Thomas C. Smith Dark Ridge Observatory (DRO)

HD b Field DRO HD M27 Dumbbell Nebula

Transit Light Curve DRO

Transit Perspective II I Inclination Angle HD b Angle of Inclination = 85.3 degrees to the ecliptic

Eclipsing Binary Project Status One of the target stars in our current project is V1191Cyg in the constellation Cygnus. This system is at an inclination of approximately 89 degrees to the plane of the ecliptic and is a potential system to view a planetary transit should planets exist in orbit around that system. One of the target stars in our current project is V1191Cyg in the constellation Cygnus. This system is at an inclination of approximately 89 degrees to the plane of the ecliptic and is a potential system to view a planetary transit should planets exist in orbit around that system. Over the past two years Russ and I have collects images of this system. I have collected over 53,000 images and Russ has many as well and we are well into our data analysis and potential object search. Over the past two years Russ and I have collects images of this system. I have collected over 53,000 images and Russ has many as well and we are well into our data analysis and potential object search. DRO

High Inclination W UMa Stars

Solar Radii vs. Line-of-Sight Inclination Angle

“End of the Line Binaries” DRO