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X-Ray Astronomy

Jan 01, 2016

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Lesley Crawford

X-Ray Astronomy. X-Rays Light at high energies Takes lots of energy to produce them Atmosphere absorbs X-Rays Most of the matter that we “see” is known to us from its X-Ray emission. X-Ray Astronomy. Solar Studies in late 40’s Discovery of first extra solar source in 1962 - PowerPoint PPT Presentation
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Page 1: X-Ray Astronomy
Page 2: X-Ray Astronomy

X-Ray Astronomy

• X-Rays – Light at high energies– Takes lots of energy to produce them

• Atmosphere absorbs X-Rays

• Most of the matter that we “see” is known to us from its X-Ray emission

Page 3: X-Ray Astronomy
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X-Ray Astronomy

• Solar Studies in late 40’s

• Discovery of first extra solar source in 1962– Also discovery of faint glow (the “diffuse

background)

Page 6: X-Ray Astronomy

Project History

• Began in 1976

• Launch in 1999

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Chandra –Line Drawing

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The Optics

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Mirror Polishing

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Optical Bench

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InstrumentsAdvanced Ccd Imaging Spectrometer

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InstrumentsHigh Resolution Camera

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X-Ray Calibration Facility

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Preparing For Thermal Vacuum Test

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The Crew

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Chandra/IUS in Cargo Bay

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Launch (7-19-99) Almost

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Launch at Last!7-23-1999

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Chandra Deployed

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The Orbit

From above, with radiation belts & Moon Side view, showing radiation belts

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First Light

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First Light

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Planets

• Jupiter– Hot spots at high latitudes

• Big surprise

– Pulsates (45 minute period)

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Venus

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Supernova Schematic

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Monitoring Sn1987a

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Crab Nebula

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Crab Pulsar Always on!

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Vela Pulsar

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Globular Cluster M15

• Chandra resolved 2 sources in center

• Explained contradictory observations

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Galactic Center

•First high-resolution X-ray panorama of the Galactic center

•Detection of about 1,000 discrete X-ray sources

•Detection of large amounts of hot gas

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Sgr A*

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Sgr A*

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Normal Galaxies – M81

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Active Galaxies - NGC 1068

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Multi-wavelength Jets: M87

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X-Ray-Bright Highest-Redshift Quasars

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Clusters of Galaxies - Hydra

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Clusters of Galaxies – Dark Matter

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The Deep Surveys

• 1Million seconds on Chandra Deep Field-South and 2 Million on CDF-N– Probe is 80 times deeper at low energies– 800 times deeper at hard energies– All data publicly available

• CDF-N detects about 500 discrete sources and 6 extended sources

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Summary

• Operations are running smoothly

• Mission success – Design of the Observatory – Excellent and committed staff– Team effort involving all the players– Exciting and fundamental scientific results– Papers at a rate of ~10 per week

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Education and & Outreach

Public Web Site http://chandra.harvard.edu

– Access to Chandra images & information

Products – posters, coloring books, – lithographs & other

printed items– educational videos– CD-ROMs