Balloon-based observations of stellar occultations Cathy Olkin Southwest Research Institute April 27, 2007.

Slides:



Advertisements
Similar presentations
Downs 4 th Grade Science Solar System Review The Planets & Other Objects in Space.
Advertisements

The Solar System By Level Two.
RECON: Research and Education Cooperative Occultation Network This material is based upon work supported by the NSF under Grant No
09/06/ Unit E Space Exploration 09/06/20153 Background YOU are RESPONSIBLE for the MATERIAL. NOT ALL the material will be presented in class- only.
2002 PLUTO OCCULTATIONS J. Elliot et al. Observations were made of an occultation of the star by Pluto. Previous observations in 1988 showed an isothermal.
Earth Science Unit Overview: Chapter 4 – Earth’s Water
Probing the Dynamics of Saturn’s Rings A.S. Bosh (Lowell Obs.), J.L. Elliot, C.B. Olkin, R.G. French, J. Rayner.
Astronomy 1 – Winter 2011 Lecture 17; February
 The solar system has 8 planets.  The solar system has 1dwarf planet named Pluto.
Tuesday Do Now: What are the biggest and smallest planets?
Observational Astronomy. Astronomy Primary Goal: Understanding the nature of the universe and its constituents Means: Equipment building, research, teaching.
1 D. Lester Eventful Universe Symposium March 19, 2010 The Stratospheric Observatory for Infrared Astronomy (SOFIA) and the Transient Universe Dan Lester.
THE SOLAR SYSTEM. WHAT IS A PLANET? “ According to Webster’s dictionary a planet is a large, round object in space (such as Earth) that travels around.
Chapter 8, Astronomy. Identify planets by observing their movement against background stars. Explain that the solar system consists of many bodies held.
UNIT NINE: Matter and Motion in the Universe  Chapter 26 The Solar System  Chapter 27 Stars  Chapter 28 Exploring the Universe.
Neptune BY ALYSSA. ~Neptune is so faraway that it took the space probe Voyager 2-12 years to reach it. Facts About Neptune.
Telescopes and the Atmosphere Our goals for learning How does Earth’s atmosphere affect ground-based observations? Why do we put telescopes into space?
< BackNext >PreviewMain Studying Space Chapter 18 Preview CRCT Preparation.
Solar System. MILKY WAY 200 billion stars Diameter LY Height at center LY Solar System is LY from center.
Just how big is big? To do this, we need to make a model.
The Solar System Astronomy!!. What is the geocentric model? The Earth is stationary while objects in the sky move around it.
What YOU can see of the Solar System With Images by Fred Klein Member of Amateur Astronomers Association of Pittsburgh.
Halfway Around the World for 5 Minutes of data
The Solar System Mercury l Closest to the sun l Revolves around sun in 88 days l Dark and rocky surface l Vast sheets of ice in polar regions l One-third.
Do Not Write What is in Yellow APPARENT MOTIONS OF THE CELESTIAL OBJECTS.
Chapter 10 Earth’s Place in the Solar System
Earth, Moon, and Beyond Chapter 9.
The full electromagnetic spectrum …. Temperature determines the main type of radiation emitted … (left to right: Compton, Chandra, Hubble, and Spitzer.
(62.03) Observational Results from the 2007 March 18 Pluto Stellar Occultation Jay M. Pasachoff, B. A. Babcock, S. P. Souza, A. J. McKay (Williams College),
The REAL OCCULT: Lunar & Solar Eclipses and Asteroid & Stellar Disappearances Sometimes Involving Luna By Dr. Harold Williams of Montgomery College Planetarium.
Cathy Olkin.  Determine size and shape  This requires multiple chords  With only one chord you only get lower limit on size 2009/11/19 Occultation.
The Solar System The Sun’s Family - the Giants The Sun’s Family - the Dwarfs Earth Venus Mars GanymedeTitanMercury Callisto Io Moon EuropaTriton Pluto.
Our Solar Neighbourhood “protoplanet hypothesis” = model to explain the birth of solar systems 1. cloud of dust and gas begins to swirl 2. most material.
Other Solar System Bodies Moons Asteroids Comets Meteors and Meteorites.
Cascadia Airless body Research Institute (CARI) Near Earth Asteroid (NEA) National Science Foundation (NSF) Research Grant Proposal Presentation by Tony.
Space Science Space Science. How many planets are in our Solar System?
Voyagers (1970s) 1800 lbs, dish >12 ft diameter data rates ~115,000 bits/sec (twice dial-up!) Radioisotope Power Generators.
Worlds around Distant Suns Mini University June 16, 2003 Among the most significant discoveries of the 20th Century.
Stars vs Planets in the Night Sky Both appear as bright dots How would we tell them apart?
SIRTF and SOFIA Spaced out, or simply on a higher plane? John Storey UNSW.
Space Science – Lesson 1: Components of Space. What are you made of? Space Science – Lesson 1: Components of Space.
Space platform and Orbits Introduction to Remote Sensing Instructor: Dr. Cheng-Chien LiuCheng-Chien Liu Department of Earth Sciences National Cheng Kung.
2003 DPS KBO Workshop Program 1:00 - 1:10 Introductory comments - Asantha Cooray (Caltech) 1:10 - 1:30 Formation of KBOs and expectations for their size.
Earth’s Solar System Astronomy. *8 Planets Go Around The Sun *Satellites (Moons) of Planets *Asteroid Belt *Comets Sun = Star.
Planet Transits Lecture Thirty, Apr. 16, Projects due April 25 Background papers have been graded (out of 15 points). Background papers have been.
Space and the planets.
Adaptive Optics for Astronomy Kathy Cooksey. AO Basics Photons –Travel in straight lines Wavefront –Line perpendicular to all photons’ paths Atmospheric.
Astro4Girls Sunnyvale Library Mar 20, What is Infrared light? Light itself is made up of lots of different “colors”. Raindrops and prisms pull.
February 18, 1930 Pluto discovered by Clyde Tombaugh. It was the first planet discovered by an American. Tombaugh was hired to search for proof of theories.
Multiple Spacecraft Observatories for 2020 and Beyond: Breaking a Tradition of Four Centuries Webster Cash University of Colorado.
5 th Grade MidYear Science Review, Space Science Aldine ISD 2009/2010.
“What are the tools used to study the universe? Andres F. Clemente V 7 - Amorsolo Andres F. Clemente V 7 - Amorsolo.
Turning Forces Circular, Satellite & Planetary Motion
Characteristics of Earth Reasons for the Seasons Name.
►O►One rotation takes 59 years. ►O►One year takes 88 days. ►I►It is 57.9 million km. from the sun. ►I►It is 4900 km. across.
THE SOLAR SYSTEM. BODIES IN THE SOLAR SYSTEM Our planet, Earth, is part of a system of planets that orbit a star, the sun. The solar system is comprised.
Transit of Mercury May 9, Outline A transit of Mercury is about to happen May 9, 2016 Very rare event Visually impressive event Shows the solar.
Modelling Celestial Motion. Using Models Designers and engineers use models to help them solve problems without having to construct the real thing. Designers.
The Science Case Hubble Space Telescope CELT+AO HDF.
Star behind Uranus’s rings
Observing a Planet.
A spectacular lunar graze
SATELLITES.
STELLAR OCCULTATIONS Version 01, 14/10/2016
Summer of `(MU)69 Marc W. Buie Southwest Research Institute +
Unit E – Space Exploration
CRITICAL GAPS: OCEANS IN THE EARTH SYSTEM
CHEOPS - CHaracterizing ExOPlanet Satellite
Presentation transcript:

Balloon-based observations of stellar occultations Cathy Olkin Southwest Research Institute April 27, 2007

What is a stellar occultation? A stellar occultation is a planet passing in front of a star. This star light probes the planet’s atmosphere or ring system at a higher spatial resolution than available any other ways near Earth observations.

What science can be derived from this technique? -Sizes of asteroids or other airless bodies. KBOs in the future. -Discovery and kinematic models of ring systems - Discovery of the rings around Uranus - Improved kinematic models of ring systems HST FOC stellar occultation light curve of Saturn’s rings (Bosh, Olkin, French, Nicholson 2003)

What science can be derived from this technique? -Sizes of asteroids or other airless bodies - Discovery and kinematic understanding of ring systems - Discovery and characterization of planetary atmospheres R (km) v. T (K) R (km) v. dT/dr (K/km) dry adiabat

An example of how we do this now  We choose events with shadow paths goes over arid locations - severely limits possible events  Accurate, timely prediction critical for for success Pluto June 12, 2006

An example of how we do this now, cont.  Expensive to cover all these sites and ship portable telescopes. Pluto June 12, 2006

Predicted occultations More than half the events happen during daylight More than half the events happen during daylight More than half the events happen over the ocean or otherwise not amenable locations More than half the events happen over the ocean or otherwise not amenable locations

Other ways to make this measurement Advantages Advantages-mobile -above most weather Disadvantages Disadvantages -KAO de- commissioned -awaiting SOFIA -SOFIA will be a heavily desired resource - does not give multiple chords - does not give multiple chords

Our idea Deploy balloons out of an airplane traveling perpendicular across the shadow path

Advantages  Nearly global access  Day and night events possible Depends on background level Depends on background level  Multiple chords  Above clouds  Good seeing

Questions?  What is the background level at wavelengths of 8000 Angstroms at both day and night at ballooning altitude Impacts telescope aperture; payload weight; expense Impacts telescope aperture; payload weight; expense  Stability and telescope pointing  Feasibility of deploying from airplanes  Communications/Operations of multiple balloons  Cost per unit Balloon Balloon Instrumentation/Telescope Instrumentation/Telescope Campaign costs Campaign costs