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Direct Observation of Exo-planets Enabled by Return to the Moon Webster Cash University of Colorado November 30, 2006 1 2 How Can We Make Use of Return to the Moon? Future of Astrophysics is in Large Structures and Formations Will use Exo-planet Studies with Occulters as Example 3 A Core Principle of Science Fastest route to the science wins Fastest is almost always the Cheapest If we can’t save money using RTM, we should not even consider it. i.e. Nobody would ever again observe from the ground if it weren’t vastly cheaper. 4 What is the Financial Advantage of RTM? What can manned or robotic presence do to lower costs? What can “Luna Firma” do to lower cost? 5 How Do We Save Money Using Surface? General Infrastructure –Power, Communications, Maintenance Astronomy Infrastructure –Low Cost Instruments –Permanent Telescope Mounts Large Stable Platform –Long Baseline Interferometry –Vacuum Beamline 6 Exo-Planets Exo-planets are the planets that circle stars other than our Sun. There are probably 10,000 exo-planets within 10pc (30 light years) of the Earth. Indirect means have now found over 200. If we can observe them directly, we will have a new field of astronomy every bit as rich as extragalactic. 7 Occulter Diagram Planet Target Star NWD Starshade JWST Telescope big enough to collect enough light from planet Occulter big enough to block star – Want low transmission on axis and high transmission off axis Telescope far enough back to have a properly small IWA No outer working angle: View entire system at once 8 Fly the Telescope into the Shadow 9 Dropping It In 10 Occulters Several previous programs have looked at occulters – First look by Spitzer (1962) Used simple geometric shapes – Achieved only 10-2 suppression across a broad spectral band With transmissive shades – Achieved only 10-4 suppression despite scatter problem http://umbras.org/ BOSS Starkman (TRW ca 2000) 11 The Apodization Function This Function Extinguishes Poisson’s Spot to High Precision A 0 for a and A 1 e a b n for a 12 Off Axis Performance The off axis performance shows a rapid rise to unit transmission for the radii greater than the inner edge of the habitable zone 13 Suppression of Edge Diffraction Can Be Understood Using Fresnel Zones and Geometry The occulter is a true binary optic –Transmission is unity or nil Edge diffraction from solid disk is suppressed by cancellation –The power in the even zones cancels the power in the odd zones b a Need enough zones to give good deep cancellation • Sets the length of the petals –Petal shape is exponential b is scale of petal shape n is an index of petal shape a is the diameter of the central circle 14 Doing the Math (Cash, Nature 2006) The Residual Intensity in the Shadow is By Babinet’s Principle Es 1 EA Is E 2 s where EA is field over Aperture So We Must Show 2 a ik 2 2 ik 2 ik s cos ik s cos a k e 2 F e F d d e 2 F e F e b d d i 2 F 0 0 0 a n F is distance to starshade, s is radius of hole, k is 2/ To one part in C 105 15 Contrast Ratio Preceding integral shows the contrast ratio is – n! F R n n a b 2 n 2 – n is an integer parameter, typically n=6 To keep R small a~b – this is the reason the occulter has that symmetric look 16 Scale Model Lab Demo 17 Data from Heliostat by Doug Leviton Shadow Map Bottom at 1x10-7 Image of Backlit Starshade 18 Starshade Tolerances Position Lateral Distance Several Meters Many Kilometers Angle Rotational Pitch/Yaw None Many Degrees Shape Truncation Scale Blob 1mm 10% 3cm2 or greater Holes Single Hole Pinholes 3cm2 3cm2 total 19 Simulated Solar System (Using NIRCam of JWST) 20 Discoverer Science Simulations Starshade Shadow Jupiter Exo-Zodiacal Jupiter Saturn Mars Earth Saturn 21 NWD Sensitivity Planet Mass (ME) 100 10 Habitable Zone 1 0.1 10.0 1.0 Semi-Major Axis (AU) 22 The First Image of Solar System Uranus Galaxies Zodiacal Light Jupiter Saturn Neptune 10 arcseconds 23 Spectroscopy R > 100 spectroscopy will distinguish terrestrial atmospheres from Jovian with modeling H2O O2 CH4 NH3 S. Seager 24 Photometry Calculated Photometry of Cloudless Earth as it Rotates It Should Be Possible to Detect Oceans and Continents! 25 What Will RTM Provide Up To This Point? Refueling Fly starshade back from L2 to rendezvous Hugely extend life of instrument Thousands of targets instead of just hundreds Repair Patch micrometeor holes Replace/Upgrade Electronics & Instruments Telescope on Lunar Surface? Difficult to hold starshade in position No Financial Advantage Probably Not… 26 TRUE PLANET IMAGING 3000 km 1000 km 300 km 100 km Earth Viewed at Improving Resolution 27 Solar System Survey at 300km Resolution 28 New Worlds Imager Concept starshades 50,000km primary collector combiner collector craft 1500km field star collimator planet collimator to combiner field star beams Delay Lines – Mixers - Detectors planet beams 29 Hypertelescope Problem How Many Apertures Needed? One per pixel (no!) Cost control of multiple craft Formation Flying to Tolerance Labeyrie has worked on this Amazing telescope even without starshades 30 Sims Established that information is present in the fringes and detectable. How do we invert into images? Is this enough? 31 Lunar Option Planet Imaging is exciting enough to justify the expense level Appropriate Level of Challenge for 20+ years from now Starshades in Orbit 1m Collectors Delay Lines, Beam Combiner, Detector 1m Collimator Surface of Moon 4m Telescope 32 Tradeoff Pro Con Infrastructure Moon Stable Bench Predictable Bench Refuel Starshades Moon Rotates 100km class delay lines 33 Can We Avoid Long Delay Lines? Should We Look at Hybrids? Takes out First Order Effects Farther Away, Lower OPD Starshades in Orbit Relay Delay Lines, Beam Combiner, Detector 1m Collimator Surface of Moon 4m Telescope 34 Return to Moon Engineering presence in deep space via humans and robots will greatly extend the lifetime and range of New Worlds Should we place some telescopes on surface? – Perhaps tiny telescopes make sense – Can we image planets and black holes from surface? Stability, predictability and Infrastructure are Positives Rotation of Moon is a huge negative 35 This is a new box. We have to think outside the old box. The old solutions and ways of thinking should be suspect. Perhaps, with enough work, we can find new solutions to the problem that will tilt the answer toward the surface. Have we given this enough thought? – NO! 36