Gaia ESA's billion star telescope

Similar documents
cheops Assemble your own planet watcher cheops Paper Model Scale 1:15

TESS: Transiting Exoplanet Survey Satellite.

Planck microwave space telescope. 1:48 scale

COBE: Cosmic Background Explorer

Gaia Status & Early Releases Plan

Picometre metrology. The Gaia mission will create an ultra-precise three-dimensional map of about one billion stars

SPITZER SPACE TELESCOPE

WMAP Wilkinson Microwave Anisotropy Probe 1:24 scale

The James Webb Space Telescope

The Gaia Mission. Coryn Bailer-Jones Max Planck Institute for Astronomy Heidelberg, Germany. ISYA 2016, Tehran

Gaia, the universe in 3D: an overview of the mission. Gaia, the universe in 3D: an overview of the mission. X. Luri, ICCUB/IEEC

Educational Product Teachers Grades K-12 EG MSFC

13 - EXTRASOLAR PLANETS

GAIA: THE SATELLITE AND PAYLOAD. Oscar Pace European Space Agency, ESA-ESTEC, Keplerlaan 1, 2200AG Noordwijk, The Netherlands

Scientific Capability of the James Webb Space Telescope and the Mid-InfraRed Instrument

High-performance computing in Java: the data processing of Gaia. X. Luri & J. Torra ICCUB/IEEC

Plato, Euclid and the New Hard X-Ray mission

The Main Point(s) Lecture #36: Planets Around Other Stars. Extrasolar Planets! Reading: Chapter 13. Theory Observations

Astronomy. Optics and Telescopes

V. Astronomy Section

INAF-Osservatorio astronomico di Torino Technical Report nr.156

The Arabs: The visible universe is times larger than Tycho Brahe believed. Translation of Greek texts and Science

The Secret Behind the Nobeyama 45-m Radio Telescope s Excellent

Star clusters before and after Gaia Ulrike Heiter

Astronomy 102: Stars and Galaxies Examination 3 Review Problems

Chapter 23: Dark Matter, Dark Energy & Future of the Universe. Galactic rotation curves

Selection of stars to calibrate Gaia

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

Exploring Dark Matter through Gravitational Lensing. Exploring the Dark Universe Indiana University June 2007

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

Chapter 19 Galaxies. Hubble Ultra Deep Field: Each dot is a galaxy of stars. More distant, further into the past. halo

Gaia: Mapping the Milky Way

Our Galaxy. Milky Way Galaxy = Sun + ~100 billion other stars + gas and dust. Held together by gravity! The Milky Way with the Naked Eye

How to Understand Stars Chapter 17 How do stars differ? Is the Sun typical? Location in space. Gaia. How parallax relates to distance

Modelling the Milky Way: challenges in scientific computing and data analysis. Matthias Steinmetz

Chapter 13 Other Planetary Systems. Why is it so difficult to detect planets around other stars? Brightness Difference

Chapter 23 The Milky Way Galaxy Pearson Education, Inc.

Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe

Chapter 13 Lecture. The Cosmic Perspective Seventh Edition. Other Planetary Systems: The New Science of Distant Worlds Pearson Education, Inc.

Chapter 13 Lecture. The Cosmic Perspective Seventh Edition. Other Planetary Systems: The New Science of Distant Worlds Pearson Education, Inc.

Chapter 0 Introduction X-RAY BINARIES

Facts Underlying the High Performance of the 188-cm Reflector Telescope

Herschel Mission Overview and Key Programmes

Searching for Other Worlds

EUCLID Mission Baseline Design

The FAME Mission: An Adventure in Celestial Astrometric Precision

8. Which of the following can not be detected by modern telescopes? A. radio waves B. heat waves (infrared) C. light waves D.

The table summarises some of the properties of Vesta, one of the largest objects in the asteroid belt between Mars and Jupiter.

Astro 1010 Planetary Astronomy Sample Questions for Exam 3

Optics and Telescopes

Astronomical Techniques

Telescopes, Observatories, Data Collection

= λ. Topics for Today. Clicker Q: Radio Waves. Radios. Light Pollution. Problems in Looking Through Our Atmosphere

Area 1: Space Exploration and Cosmology. 2. The weather information satellite NOAA-15 has a period of 99 minutes and an orbital height of 833 km.

ANSWER KEY. Stars, Galaxies, and the Universe. Telescopes Guided Reading and Study. Characteristics of Stars Guided Reading and Study

X-ray Astronomy F R O M V - R O CKETS TO AT HENA MISSION. Thanassis Akylas

JAMES WEBB SPACE TELESCOPE (JWST) - FINE GUIDENCE SENSOR AND TUNABLE FILTER IMAGER OPTICAL DESIGN OVERVIEW AND STATUS

Properties of the Solar System

From VOA Learning English, this is Science in the News. I m June Simms.

Space astrometry with the Joint Milliarcsecond Astrometry Pathfinder

Chapter 13 Other Planetary Systems. The New Science of Distant Worlds

The color of a star provides a measure of its A. size B. mass C. composition D. surface temperature

AST 101 Intro to Astronomy: Stars & Galaxies

James Webb Space Telescope (JWST)

Chandra Fun Facts. Chandra Fun Facts. Chandra Fun Facts. Chandra Fun Facts. Chandra Fun Facts. Chandra Fun Facts

2010 Pearson Education, Inc.

THE MILKY WAY GALAXY BACKGROUND READING FOR MIDDLE AND HIGH SCHOOL SCIENCE

The Three Dimensional Universe, Meudon - October, 2004

SCIENTIFIC CASE: Study of Hertzsprung-Russell Diagram

TELESCOPES POWERFUL. Beyond the Book. FOCUS Book

Simulations of the Gaia final catalogue: expectation of the distance estimation

First Cycle Processing of Gaia data

Writing very large numbers

National Aeronautics and Space Administration. Glos. Glossary. of Astronomy. Terms. Related to Galaxies

Foundations of Astronomy 13e Seeds. Chapter 6. Light and Telescopes

The James Webb Space Telescope Overview

Directions: For numbers 1-30 please choose the letter that best fits the description.

Lecture #15: Plan. Telescopes (cont d) Effects of Earth s Atmosphere Extrasolar planets = Exoplanets

Exoplanetary transits as seen by Gaia

Science In Action 9 Unit 5 Space Exploration Summary of Key Concepts and Review Questions Booklet

Hubble Space Telescope

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

chapter 31 Stars and Galaxies

gaia THE BILLION STAR SURVEYOR GAIA DATA RELEASE 2 Media kit

LISA Pathfinder: experiment details and results

LESSON 1. Solar System

Technology and Space Exploration

10/16/ Detecting Planets Around Other Stars. Chapter 10: Other Planetary Systems The New Science of Distant Worlds

The Milky Way Galaxy

BepiColombo Mission to Mercury - コロンボ. October Jan van Casteren, Mauro Novara.

How Light Beams Behave. Light and Telescopes Guiding Questions. Telescopes A refracting telescope uses a lens to concentrate incoming light at a focus

Cosmic Microwave Background Radiation

What is the solar system?

On to Telescopes. Imaging with our Eyes. Telescopes and cameras work much like our eyes. ASTR 1120 General Astronomy: Stars & Galaxies !

Jodrell Bank Discovery Centre Answers to worksheets

Fermi Paper Model. Material Lists. A. Spacecraft and GBM. Parts Supplied. Parts Needed. Spacecraft and GBM. Fig. 1

Aperture Door. Model Wrappers. Aft Bulkhead. Page 1

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

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

Astronomy 182: Origin and Evolution of the Universe

Transcription:

Gaia ESA's billion star telescope Gaia is an unmanned space observatory of the European Space Agency (ESA) designed for astrometry. The mission aims to compile a 3D space catalogue of approximately 1 billion astronomical objects (approximately 1% of the Milky Way population) brighter than 20 G magnitudes, where G is the Gaia magnitude passband between about 400 and 1000 nanometres light wavelengths. Successor to the Hipparcos mission, it is part of ESA's Horizon 2000 Plus long-term scientific program. Gaia will monitor each of its target stars about 70 times over a period of five years. Gaia will create a precise three-dimensional map of stars throughout the Milky Way and map their motions, which encode the origin and subsequent evolution of the Milky Way. The spectrophotometric measurements will provide the detailed physical properties of each star observed, characterising their luminosity, effective temperature, gravity and elemental composition. This massive stellar census will provide the basic observational data to tackle a wide range of important questions related to the origin, structure and evolutionary history of our galaxy. Large numbers of quasars, galaxies, extrasolar planets and Solar System bodies will be measured at the same time. Gaia was launched on 19 December 2013 by Arianespace using a Soyuz ST-B/Fregat- MT rocket flying from Kourou in French Guiana. The spacecraft will be operated in a Lissajous orbit around the Sun Earth L2 Lagrangian point. Telescopes: M1, M2 and M3: Mirrors of telescope 1 M'1, M'2 and M'3: Mirrors of telescope 2 The optical path of both telescopes is composed of six reflectors (M1-M6), two of which are common (M5-M6). The entrance pupil of each telescope is 1.45 m x 0.5 m² and the focal length is 35 m. The payload module features a common focal plane shared by both telescopes. Dimensions: 10.2 m 4.0 m

1. Cut out and glue unprinted sides together to make sunshield. 4. Cut out part and glue to the top of part 2. 1:100 scale 5. Cut out parts, roll the band into a ring and glue. Glue the circle to the band, then glue the completed assembly to the center bottom (gold side) of the sunshield. GAIA ESA billion star telescope 2. Cut out part, cut out black openings, then roll into a cylinder and glue using the tab. After inserting part 3, fold down the tabs and glue the assembly to the gray side of the sunshield. 3. Cut out part, cut out black openings, then roll into a cylinder. Slip inside part 2, lining up the openings and glue in place.

Gaia 1:50 scale SUNSHIELD - BOTTOM LAUNCH MOUNT/COMMS 9. Cut out the launch mount and comms antennae. Fold petals down and glue into a flat prism. Glue completed part to the bottom/center of the sunshield (gold & blue side). 9a. Alternate simple launch mount. Cut out parts, roll the band into a ring and glue. Glue the circle to the band, then glue the completed assembly to the center bottom (gold side) of the sunshield. 1. Cut out sunshield top and bottom and glue unprinted sides together.

Gaia 1:50 scale SUNSHIELD - TOP 8. FOCAL PLANE RADIATOR (optional). Cut out shape, cut along red lines. Fold into a box and glue to the telescope body over the printed graphic. 7. Cut out telescope body top and glue to the top of the telescope body. TELESCOPE BODY - TOP

Gaia 1:50 scale TELESCOPE BODY - EXTERIOR 2. Cut out telescope exterior and cut out the two apertures. Roll into a cylinder and glue using the tab. TELESCOPE BODY INTERIOR (SIMPLIFIED OPTICAL BENCH PARTS NOT REQUIRED) 3. Cut out telescope interior and cut out the two apertures. Roll into a cylinder, printed side in, and glue inside the exterior lining up the aperture cut outs. If building the detailed optical bench, replace this part with an equally sized piece of black paper. Glue the paper inside the body exterior and cut out the apertures.

Gaia 1:50 scale 4. OPTICAL BENCH UPPER LAYER. CUT ON RED LINES AND BEND LARGE MIRRORS UP TO FIT INSIDE BODY, BEND SMALL MIRRORS DOWN. CURVE M1 MIRRORS SLIGHTLY. GLUE THE OTHER TWO RINGS TO THE BOTTOM OF THE BENCH FOR STRENGTH. 4 CENTER 4 CENTER OPTICAL BENCH - FLOOR M1 4 CENTER M2 5. OPTICAL BENCH LOWER. ARROWS INDICATE FOLDS. PARTS ON THE DISK FOLD UP. TABS AT THE TOP OF THE MIRRORS FOLD DOWN. FOLD FOCAL PLANE INTO A BOX AND GLUE. OPTICAL BENCH UPPER LAYER ASSEMBLY GLUES TO THE THREE TABS AND TOP OF THE FOCAL PLANE, ALIGNING THE M3 MIRRORS UNDER THE M1 MIRRORS. FOLD M4 INTO A BOX AND GLUE WHERE INDICATED. M5 M3 M3 M4 COMBINER FOCAL PLANE 6.OPTICAL BENCH FLOOR SUPPORT. ROLL AND GLUE INSIDE LOWER TELESCOPE BODY, BEND TABS DOWN TO FORM LEDGE TO SUPPORT FLOOR. GLUE OPTICAL BENCH FLOOR IN PLACE. GLUE ASSEMBLED OPTICAL BENCH TO FLOOR WITH M1 MIRRORS OPPOSITE THE OPENINGS IN THE TELESCOPE BODY. GLUE THE COMPLETED TELESCOPE BODY TO THE CENTER/TOP OF THE SUNSHIELD (GRAY SIDE).