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Vacuum, Extreme Radial Velocity Experiment: VERVE An instrument for ultra-precise radial velocity measurements J. Kent Wallace (JPL) 28 July 2015
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Fellow Contributors Michael Randolph, LCHS Rebecca Jensen-Clem, CIT Gautam Vasisht, JPL Phil Muirhead, BU Lynne Hillenbrand, CIT Erik Hovland, JPL Richard Dekany, CIT 2
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Outline 1.Radial Velocity Measurement Overview 2.Instrument Description 3.Preliminary Data 4.Performance Predictions 5.Conclusion 3
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Outline 1.Radial Velocity Measurement Overview 2.Instrument Description 3.Preliminary Data 4.Performance Predictions 5.Conclusion 4
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Radial Velocity Measurement Overview 5 Traditional Spectroscopy Traditional Spectroscopy 1 1 Intensity Wavelength Iodine spectral reference Grating spectrograph The Goal ΔRV=10cm/s Δλ = 1x10 -5 Å The Requirement: Δλ = 2x10 -6 Å The State of the Art: 70cm/s
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Radial Velocity Measurement Overview 6 E xternally D ispersed I nterferometry (EDI) 2 2 spectralfringe.org Scanning Interferometer Time λ Grating spectrograph Absorption lines Moire pattern Interferometer transmission comb Traditional Spectroscopy Traditional Spectroscopy 1 1 Intensity Wavelength Iodine spectral reference Grating spectrograph
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One Pixel 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux 7 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Delay Change [μm] 0.00.51.01.52.02.5 8 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 9 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 10 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 11 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 12 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 13 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 14 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 15 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 16 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 18 Image Credit: Phil Muirhead
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One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 19 Image Credit: Phil Muirhead
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1 km/s Doppler Shift One Pixel Flux 5499.915499.9555005500.055500.09 Wavelength [Å] Relative Flux Flux Delay Change [μm] 0.00.51.01.52.02.5 20 Image Credit: Phil Muirhead
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Outline 1.Radial Velocity Measurement Overview 2.Instrument Description 3.Preliminary Data 4.Performance Predictions 5.Conclusion 21
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Instrument Description 22 BS2 Grating Fiber-Fed OAP Lens Imaging Array Fold Mirror BS1 Prism Fold Mirror PZT Flexure Stage
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Instrument Description 23 BS2 Grating Fiber-Fed OAP Lens Fold Mirror BS1 Prism Fold Mirror PZT Flexure Stage Imaging Array
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Outline 1.Radial Velocity Measurement Overview 2.Instrument Description 3.Preliminary Data 4.Performance Predictions 5.Conclusion 24
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Preliminary Data 25
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Preliminary Data
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Outline 1.Radial Velocity Measurement Overview 2.Instrument Description 3.Preliminary Data 4.Performance Predictions 5.Conclusion 37
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Performance Predictions 38 The Palomar 200” telescope would take about 0.075 seconds to reach an SNR=8 resolution element, given the assumptions in the above tables. For 425 scans, each with 200 0.075 sec phase steps, the 200” telescope would require about 1.8 hours to reach a radial velocity precision of 10 cm/sec.
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Outline 1.Radial Velocity Measurement Overview 2.Instrument Description 3.Preliminary Data 4.Performance Predictions 5.Conclusion 39
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Conclusion Radial velocity precision of 10 cm/sec appears achievable with externally dispersed interferometry. We are developing instrumentation to demonstrate this. Low-noise detectors are critical to demonstrating this new instrument. 40
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