the astrometric promise of large a*

13
The Astrometric The Astrometric Promise of Large Promise of Large A* A* Dave Monet Dave Monet U.S. Naval Observatory - Flagstaff U.S. Naval Observatory - Flagstaff Station Station September 21, 2008 September 21, 2008

Upload: ornice

Post on 19-Mar-2016

57 views

Category:

Documents


0 download

DESCRIPTION

The Astrometric Promise of Large A* . Dave Monet U.S. Naval Observatory - Flagstaff Station September 21, 2008. Executive Summary. Is anything left to do?. Gaia and SIM promise to do everything: Microarcsecond astrometry down to 20 th . Sub-microarcsecond astrometry for planets. - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: The Astrometric Promise of Large A*

The Astrometric The Astrometric Promise of Large A*Promise of Large A*

Dave MonetDave MonetU.S. Naval Observatory - Flagstaff StationU.S. Naval Observatory - Flagstaff Station

September 21, 2008September 21, 2008

Page 2: The Astrometric Promise of Large A*

Executive SummaryExecutive Summary

Page 3: The Astrometric Promise of Large A*

Is anything left to do?Is anything left to do?• GaiaGaia and and SIMSIM promise to do everything: promise to do everything:

• Microarcsecond astrometry down to 20Microarcsecond astrometry down to 20thth..• Sub-microarcsecond astrometry for planets.Sub-microarcsecond astrometry for planets.• Francois Mignard is a tough act to follow.Francois Mignard is a tough act to follow.

Page 4: The Astrometric Promise of Large A*

Ground vs. SpaceGround vs. Space• Reasons to go to space:Reasons to go to space:

• Ultimate in astrometric accuracy.Ultimate in astrometric accuracy.• Big teams of clever folks.Big teams of clever folks.• Lots of money and glamour.Lots of money and glamour.

• Reasons to stay on the ground:Reasons to stay on the ground:• Useful astrometric accuracy.Useful astrometric accuracy.• Big apertures.Big apertures.• High data rates.High data rates.• Long duration missions.Long duration missions.

Page 5: The Astrometric Promise of Large A*

A*A* Astrometry Astrometry• A*A* is etendue (meter is etendue (meter22 degree degree2)2)::

• Metric for telescope efficiency - sort of.Metric for telescope efficiency - sort of.• New optical designs deliver large useful fields.New optical designs deliver large useful fields.• New CCD mosaics offer many 10New CCD mosaics offer many 1088 to 10 to 1099 pixels. pixels.• Parallel electronics to read in a few seconds.Parallel electronics to read in a few seconds.

• 4 projects are in construction or planning:4 projects are in construction or planning:• Pan-STARRS (U. Hawaii + USAF).Pan-STARRS (U. Hawaii + USAF).• SkyMapper (Australian National University).SkyMapper (Australian National University).• SST (DARPA + MIT/LL + USAF).SST (DARPA + MIT/LL + USAF).• LSST (LSST Corporation).LSST (LSST Corporation).

• Astrometric utility of any/all of these systems?Astrometric utility of any/all of these systems?• Several visits to all available sky - per lunation!Several visits to all available sky - per lunation!• Astrometry for all 10**9 (or maybe 10**10) objects.Astrometry for all 10**9 (or maybe 10**10) objects.• No selection effect other than photons.No selection effect other than photons.

• Photography enabled motion - A*Photography enabled motion - A* enables parallax. enables parallax.

Page 6: The Astrometric Promise of Large A*

Pan-STARRS - PS1Pan-STARRS - PS1• On Haleakala (Maui).On Haleakala (Maui).• First light: Aug 2007.First light: Aug 2007.• ORR: Dec 2008.ORR: Dec 2008.• 33 survey: 15 visits in a survey: 15 visits in a

total of 6 colors from total of 6 colors from =-30 to =-30 to =+90.=+90.

• 1.8-m aperture.1.8-m aperture.• 1.4 billion pixel camera1.4 billion pixel camera..• PS-2, PS-4.PS-2, PS-4.

Page 7: The Astrometric Promise of Large A*

SkyMapperSkyMapper• Siding Springs (Australia)Siding Springs (Australia)• First Light: Sep 2008?First Light: Sep 2008?• 6 visits in each of 6 colors 6 visits in each of 6 colors

from from =-90 to =-90 to =0.=0.• 1.3-m aperture.1.3-m aperture.• 256 million pixel camera.256 million pixel camera.

Page 8: The Astrometric Promise of Large A*

LSSTLSST• Cerro Pachon (Chile).Cerro Pachon (Chile).• First Light: 2014?First Light: 2014?• $50M raised already.$50M raised already.• 3 visits of entire visible 3 visits of entire visible

sky every lunation.sky every lunation.• 8.4-m aperture.8.4-m aperture.• 3.4 billion pixel camera.3.4 billion pixel camera.

Page 9: The Astrometric Promise of Large A*

Astrometric Utility?Astrometric Utility?• Not much legacy for huge field, short exposure Not much legacy for huge field, short exposure

astrometry.astrometry.• Data from Data from SubaruSubaru, , GeminiGemini, , SOARSOAR, others., others.• My expectation:My expectation:

• 10 milliarcseconds per star per visit - differential.10 milliarcseconds per star per visit - differential.• Limited by photons or seeing.Limited by photons or seeing.• Differential chromatic refraction is big issue.Differential chromatic refraction is big issue.• Solve sky chunk at a time - messy.Solve sky chunk at a time - messy.• Not sure about trying to solve for the sphere:Not sure about trying to solve for the sphere:

• Why bother when Why bother when Gaia Gaia will do this for us, much better.will do this for us, much better.• Faint - correction from relative to absolute is small.Faint - correction from relative to absolute is small.

• Real data starting to appear right now!Real data starting to appear right now!

Page 10: The Astrometric Promise of Large A*
Page 11: The Astrometric Promise of Large A*

SummarySummary• Astrometry at 10 Tbytes/night is fun!Astrometry at 10 Tbytes/night is fun!

• Starting now!Starting now!• Expect milliarcsecond results before Expect milliarcsecond results before GaiaGaia..• LSST will go much fainter than LSST will go much fainter than GaiaGaia..

• Astrometry at r = 26?Astrometry at r = 26?

• Synergy between ground and space.Synergy between ground and space.

Page 12: The Astrometric Promise of Large A*

KeplerKepler Astrometry - SNR Astrometry - SNR∞∞

Page 13: The Astrometric Promise of Large A*