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TPF-I SWG Report - Exoplanet Exploration Program - NASA

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C HAPTER 3<br />

3.3 Conclusions<br />

Darwin/<strong>TPF</strong>-I will open a gateway to future space-based interferometry to deliver ever increasing angular<br />

resolution throughout the electromagnetic spectrum. The baseline design will provide order-of-magnitude<br />

improvements in angular resolution over any other instrument. Combined with sensitivity to objects as<br />

faint as magnitude 20, Darwin/<strong>TPF</strong>-I capabilities have the potential for revolutionary advances in all areas<br />

of astrophysics and planetary science. This mission will transform our understanding of galaxy formation<br />

and evolution, stellar and planetary system origins, the cycles of matter and energy in the cosmos; and it<br />

will enable the detailed mapping of surfaces and weather patterns in Solar System objects. The utility of<br />

this instrument for general astrophysics and planetary science will only be limited by the lack of available<br />

observing time.<br />

Acknowledgements: We thank Marc Kuchner for providing selected material from the <strong>NASA</strong> / JPL<br />

Publication 05-01, General Astrophysics and Comparative Planetology with the Terrestrial Planet Finder<br />

Missions.<br />

3.4 References<br />

Adams, F. C., Proszkow, E. M., Fatuzzo, M., and Myers, P. C., “Early evolution of stellar groups and<br />

clusters: Environmental effects on forming planetary systems,” Astrophys. J. 641, 504–525<br />

(2006).<br />

Barger, A. J., Cowie, L. L., Sanders, D. B., et al., “Submillimetre-wavelength detection of dusty starforming<br />

galaxies at high redshift,” Nature 394, 248–251 (1998).<br />

Boden, A. F., Shao, M., and van Buren, D., “Astrometric observations of MACHO gravitational<br />

microlensing,” Astrophys. J. 502, 538–549 (1998).<br />

Dalal, N., and Lane, B. F., “Bringing closure to microlensing mass measurements,” Astrophys. J. 589,<br />

199–209 (2003).<br />

De Breuck, C., van Breugel, W., Röttgering, H., et al., “Spectroscopy of ultra-steep-spectrum radio<br />

sources,” Astron. J. 121, 1241–1265 (2001).<br />

Dray, L. M., Tout, C. A., Karakas, A. I., and Lattanzio, J. C., “Chemical enrichment by Wolf-Rayet and<br />

asymptotic giant branch stars,” Mon. Not. R. Astron. Soc. 338, 973–989 (2003).<br />

Dwek, E., “The evolution and elemental abundances in the gas and dust phases of the Galaxy,” Astrophys.<br />

J. 501, 643–665 (1998).<br />

Edmunds, M. G., “An elementary model for the dust cycle in galaxies,” Mon. Not. R. Astron. Soc. 328,<br />

223–236 (2001).<br />

Franx, M., Labbé, I., Rudnick, G., et al., “A significant population of red, near-infrared high-redshift<br />

galaxies,” Astrophys. J. 587, L79–L82 (2003).<br />

54

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