Small Satellite Conference - GEMS Presentation August 12, 2009 Big Astrophysics in A Small Package...
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Transcript of Small Satellite Conference - GEMS Presentation August 12, 2009 Big Astrophysics in A Small Package...
Small Satellite Conference - GEMS Presentation August 12, 2009
Big Astrophysics inA Small Package
Erin WalterGEMS Spacecraft Lead/Orbital
Small Satellite Conference - GEMS Presentation August 12, 2009
GEMS Mission
• The GEMS mission was selected by NASA as a Small Explorers (SMEX) mission in July 2009 and is scheduled for launch in 2014 on a Pegasus-class launch vehicle
• The GEMS mission will be the first mission to use x-ray polarimetry to characterize the geometry and behavior of x-ray sources, including supermassive black holes and magnetars.
• Answers to important questions– How does the spin of a black hole warp space
time?– What powers magnetars?– How are cosmic rays accelerated in supernova
remnants?
• Polarization measurements allow us to study: Scattering Magnetic fields Strong gravity
GEMS will use these processes to probe black holes, neutron stars and supernova remnants
X-Ray Polarization
Small Satellite Conference - GEMS Presentation August 12, 2009
GEMS Mission Overview
Small Satellite Conference - GEMS Presentation August 12, 2009
Spacecraft Design
Omni Antenna (1 of 2)
Instrument Mount Points
• Rotating Entire Vehicle at 0.1 RPM• Instrument interface: 3-point mount brackets
on top deck• Spacecraft bus provides:
– 16 Gbits of data storage– 106 W of power provided– 4 RS-422 data interfaces– ACS Control and Knowledge– Ample throughput with RAD 750 processor– Fuses and power switches (including for
instrument cover and boom actuation)• Instrument is thermally isolated• Instrument has no FOV impingements• 2 Omni antennas mounted on instrument
support structure for FOV optimization
Pegasus-ClassLaunch Vehicle
Small Satellite Conference - GEMS Presentation August 12, 2009
Payload Design
• 0.1 rpm Rotation reduces systematic errors• Three Telescopes
– High signal to noise– Redundancy
• Three Mirrors– Light weight aluminum foil optics– Proven heritage from ASCA and Suzaku– Technology pioneered at GSFC– 4.5m focal length from extendable optical bench
• Three Time Projection Chambers Polarimeters– Photoelectric effect sensitive to polarization– Technology pioneered at GSFC
• ATK Boom• Student collaboration Bragg Reflection
Polarimeter
Small Satellite Conference - GEMS Presentation August 12, 2009
Mission Operations