NASA Joint Programs Update Astronomy and Astrophysics Advisory
- Slides: 18
NASA Joint Programs Update Astronomy and Astrophysics Advisory Committee Meeting NSF Headquarters October 15, 2009 Dr. Jon Morse Director, Astrophysics Division Science Mission Directorate NASA Headquarters
NASA/DOE: Fermi Gamma-Ray Space Telescope [JDEM, separate presentation] NASA/NSF OPP: Ballooning
NASA and NSF: Ballooning Update • New 5 -year Memorandum of Agreement between NASA/SMD and NSF/OPP on Antarctic ballooning signed in May 2009 • Flight program update • New 2009 science result from Antarctic flight: BLAST (Balloon Large Aperture Submillimeter Telescope) (PI=Mark Devlin)
NASA/NSF Mo. A on Antarctic Ballooning • Mo. A signed in May 2009, operative for five years. • Enables continuation of long-standing cooperation between the NSF/Office of Polar Programs and NASA/SMD for support of scientific ballooning in Antarctica. • Annual requirement for support of two large science missions launched from Mc. Murdo, with possible third mission in some years. • NSF provides housing, transportation, meals, medical. • NSF maintains Long Duration Balloon launch site infrastructure. • NSF provides support for payload recovery. • NSF and NASA shall meet annually to review changes, lessons learned, and improvements toward Antarctic balloon operations. • NASA provides NSF with funds to defray campaign support costs.
FY 2010 Recommended Flight Program • 16 Missions / 20* Flights approved by SMD * BARREL mission (Antarctica) is comprised of 5 separate hand-launches • 2 Foreign & 2 Domestic Flight Campaigns • 16 Science flights (Plus 2 flights left over from FY 2009) 1 (+2) 3 5 2 5 • Ft. Sumner, NM Antarctica Australia Palestine Ft. Sumner, NM (Fall 09) Airship Test (Winter 09) LDB/SP/Mo. O (Spring 10) Conventional/SP (Summer 10) Conventional (Fall 10) Conventional Antarctic campaign includes 14 MCF Super Pressure Balloon Test (goal of > 100 days) and planned recovery of BESS payload left on the Ice for two winters
FY 10 Antarctic Balloon Flight Program • FY 2010 Flight Program: 3 Antarctic flights (Winter 09): • 14 MCF super-pressure balloon test (> 100 days? ) • CREAM (Cosmic Ray Energetics and Mass) -5 – precise measurements of elemental spectra for z = 1 to 26 in 1011 to 1015 e. V region • BARREL – five hand-launched balloons (~0. 25 MCF) – measures precipitating electrons from radiation belts (Heliophysics Division) • Antarctic campaign includes: • Planned recovery of BESS payload left on the ice for 2 years
2009 Super Pressure Balloon Test Flight • 54 days of flight • Balloon remained pressurized- no apparent gas loss. • It could have flown indefinitely. • Largest super pressure balloon ever successfully flown • Longest large NASA balloon flight ever
FY 2010 Flight Schedule STATUS AS OF: 09/15/09
BLAST Balloon Science Result (Sept. 2009; flew 2006): Resolving the Cosmic Submillimeter Background—individual, distant galaxies are the source
NASA and DOE: Fermi Gamma-Ray Space Telescope Update The one-year Fermi-LAT sky: Over 1000 new high-energy gamma-ray sources
Fermi accomplishments include • Detected the moon and the quiet Sun • Detected dozens of pulsars, many pulsing only in gamma-rays and several millisecond pulsars • Detected the globular cluster 47 Tucanae • Detected orbital variations in gamma-ray emission from several binary systems • Resolved the gamma-ray emission from the LMC and several SNR – Significant implications for understanding the origin of cosmic-rays • Resolved in gamma-rays the radio lobes of Cen A • Detected over 270 GRB including 12 above 100 Me. V – Use relative arrival times of high and low energy gamma-ray photons to set stringent constraints on Lorentz invariance violation. • Detected new gamma-ray AGN population ((Narrow-Line Seyfert galaxies) • Data release on Aug 25 - all LAT and GBM data are now public within 72 hours. • First Fermi symposium Nov 2 -5 in Washington, DC. Fermi charts courtesy of Julie Mc. Enery
Gamma-ray bursts • 10 long and 2 short bursts detected by LAT at Ge. V energies – Both types of GRB show similar phenomenology at high energies – Swift XRT has detected X-ray afterglows from the 7 brightest LAT bursts resulting in the determination of the burst redshift/distance. Short GRB 081024 B Long GRB 090323 (>200 s), radio - Ge. V afterglow Short GRB 090510 Intense, z=0. 9, to 31 Ge. V Long GRB 080916 C Intense, z=4. 35, to 13 Ge. V
Fermi Gamma-Ray Space Telescope Status • The LAT and GBM are both working well • First LAT Ge. V catalog (currently being validated/checked) contains over 1000 new gamma-ray sources! – New classes of gamma-ray sources (millisecond pulsars, gamma-ray binaries, globular clusters, starburst galaxies…) • field of gamma-ray astrophysics is rapidly expanding • GBM is detecting many kinds of Me. V transients – >250 GRB/year, three SGRs (SGR 0501+4516, SGR 1806 -20 and SGR 1 E 1547. 0 -5408), >10 TGFs and a solar flare. • Science returns in solar system studies, Galactic astrophysics, extragalactic astrophysics, cosmic-ray physics and fundamental physics. • The full data release was last month, software to assist with data analysis is also available. – http: //fermi. gsfc. nasa. gov/ssc • Lots more science to come… (Gamma-ray pulsars, 0. 1 -1 Te. V electrons, Testing Einstein’s Theory of Special Relativity, etc. )
Upcoming One-Year Symposium • Fermi symposium – Washington DC, Nov 2 -5 • http: //fermi. gsfc. nasa. gov/ssc/resource s/newsletter/ – General news – Multiwavelength – Data/software • LAT data became public on Aug 25 – http: //fermi. gsfc. nasa. gov/ssc
Backup Slides
Cosmic Ray Energetics and Mass (CREAM-IV) Eun-Suk Seo, University of Maryland • 19. 5 days of flight • First instrument ever to exceed 100 days of exposure (119 Days) • Invited Highlight talk, 31 st ICRC, Lodz, Poland (Submitted for Publication)
Fermi Cycle-2 Program • 199 proposals received, 80 selected – 79 grants – 8 “Progress Reports”, all passed • 3 multi-year “Large Projects” selected – Down from 8 selections in Cycle-1 – $1. 5 M in m-yr obligations from Cycle-1 • Average grants: $174 k (large) $78 k (regular) • No pointed observations approved (2 requests) • NRAO: ~650 hours awarded – ~50% of proposed amount • NOAO: under-utilized resource – 3 requests, 1 award (24 hrs)
Limits on Lorentz Invariance Violation • Heuristic modification of the photon dispersion relation : – c 2 P 2 = E 2 ( 1+ f(E/EQG )) EQG : effective LIV energy scale – For E<<EQG : c 2 P 2 = E 2 ( 1+ (E/EQG )n+1) • n=1 or 2 in current studies v= E/ P ~ c ( 1+ (E/EQG )n) • is just a constant (can disappear in EQG) • : subluminal regime (high energy photons arrive later) • : superluminal regime (high energy photons arrive earlier) • Simple case : n=1, : – Consider a photon of energy E observed at t. –If it belongs to the GRB, at the very least it has been emitted after the trigger t 0. – Thus the maximal time delay due to LIV is t-t 0 : dt<t-t 0 – With a distance estimate, this results in a “conservative” lower limit on EQG • Independent of intrinsic time lags in GRBs
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