Towards a Small Prototype Planet Finding Interferometer: The next step in planet finding and characterization in the infrared
| dc.creator | Danchi, W. C. | |
| dc.creator | Deming, D. | |
| dc.creator | Carpenter, K. G. | |
| dc.creator | Barry, R. K. | |
| dc.creator | Hinz, P. | |
| dc.creator | Johnston, K. J. | |
| dc.creator | Lawson, P. | |
| dc.creator | Lay, O. | |
| dc.creator | Monnier, J. D. | |
| dc.creator | Richardson, L. J. | |
| dc.creator | Rinehart, S. | |
| dc.creator | Traub, W. | |
| dc.date | 2008-01-30 | |
| dc.date.accessioned | 2026-07-07T08:57:20Z | |
| dc.date.available | 2026-07-07T08:57:20Z | |
| dc.description | During the last few years, considerable effort has been directed towards large-scale (>> $1 Billion US) missions to detect and characterize earth-like planets around nearby stars, such as the Terrestrial Planet Finder Interferometer (TPF-I) and Darwin missions. However, technological and budgetary issues as well as shifting science priorities will likely prevent these missions from entering Phase A until the next decade. The secondary eclipse technique using the Spitzer Space Telescope has been used to directly measure the temperature and emission spectrum of extrasolar planets. However, only a small fraction of known extrasolar planets are in transiting orbits. Thus, a simplified nulling interferometer, which produces an artificial eclipse or occultation, and operates in the near- to mid-infrared (e.g. ~ 3 to 8 or 10 microns), can characterize the atmospheres of this much larger sample of the known but non-transiting exoplanets. Many other scientific problems can be addressed with a system like this, including imaging debris disks, active galactic nuclei, and low mass companions around nearby stars. We discuss the rationale for a probe-scale mission in the $600-800 Million range, which we name here as the Small Prototype Planet Finding Interferometer (SPPFI). | |
| dc.description | 8 pages, 4 figures, white paper for Exoplanet Task Force, March 2007 | |
| dc.identifier | https://arxiv.org/abs/0801.4752 | |
| dc.identifier | http://arxiv.org/abs/0801.4752 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/146931 | |
| dc.subject | Astrophysics | |
| dc.title | Towards a Small Prototype Planet Finding Interferometer: The next step in planet finding and characterization in the infrared | |
| dc.type | text |