Abstract
During the last few years, considerable effort has been directed towards large-scale (>> 1BillionUS)missionstodetectandcharacterizeearth−likeplanetsaroundnearbystars,suchastheTerrestrialPlanetFinderInterferometer(TPF−I)andDarwinmissions.However,technologicalandbudgetaryissuesaswellasshiftingscienceprioritieswilllikelypreventthesemissionsfromenteringPhaseAuntilthenextdecade.ThesecondaryeclipsetechniqueusingtheSpitzerSpaceTelescopehasbeenusedtodirectlymeasurethetemperatureandemissionspectrumofextrasolarplanets.However,onlyasmallfractionofknownextrasolarplanetsareintransitingorbits.Thus,asimplifiednullinginterferometer,whichproducesanartificialeclipseoroccultation,andoperatesinthenear−tomid−infrared(e.g. 3to8or10microns),cancharacterizetheatmospheresofthismuchlargersampleoftheknownbutnon−transitingexoplanets.Manyotherscientificproblemscanbeaddressedwithasystemlikethis,includingimagingdebrisdisks,activegalacticnuclei,andlowmasscompanionsaroundnearbystars.Wediscusstherationaleforaprobe−scalemissioninthe600-800 Million range, which we name here as the Small Prototype Planet Finding Interferometer (SPPFI).
8 pages, 4 figures, white paper for Exoplanet Task Force, March 2007