%0 Journal Article %1 kawahara2011 %A Kawahara, Hajime %A Fujii, Yuka %D 2011 %K maps %R 10.1088/2041-8205/739/2/L62 %T Mapping Clouds and Terrain of Earth-like Planets from Photometric Variability: Demonstration with Planets in Face-on Orbits %U http://arxiv.org/abs/1106.0136 %X We develop an inversion technique of annual scattered light curves to sketch a two-dimensional albedo map of exoplanets in face-on orbits. As a test-bed for future observations of extrasolar terrestrial planets, we apply this mapping technique to simulated light curves of a mock Earth-twin at a distance of 10 pc in a face-on circular orbit. A primary feature in recovered albedo maps traces the annual mean distribution of clouds. To extract information of other surface types, we attempt to reduce the cloud signal by taking difference of two bands. We find that the inversion of reflectivity difference between 0.8-0.9 and 0.4-0.5 micron bands roughly recover the continental distribution, except for high latitude regions persistently covered with clouds and snow. The inversion of the reflectivity difference across the red edge (0.8-0.9 and 0.6-0.7 micron) emphasizes the vegetation features near the equator. The planetary obliquity and equinox can be estimated simultaneously with the mapping under the presence of clouds. We conclude that the photometric variability of the scattered light will be a powerful means for exploring the habitat of a second Earth.

@article{kawahara2011, abstract = {We develop an inversion technique of annual scattered light curves to sketch a two-dimensional albedo map of exoplanets in face-on orbits. As a test-bed for future observations of extrasolar terrestrial planets, we apply this mapping technique to simulated light curves of a mock Earth-twin at a distance of 10 pc in a face-on circular orbit. A primary feature in recovered albedo maps traces the annual mean distribution of clouds. To extract information of other surface types, we attempt to reduce the cloud signal by taking difference of two bands. We find that the inversion of reflectivity difference between 0.8-0.9 and 0.4-0.5 micron bands roughly recover the continental distribution, except for high latitude regions persistently covered with clouds and snow. The inversion of the reflectivity difference across the red edge (0.8-0.9 and 0.6-0.7 micron) emphasizes the vegetation features near the equator. The planetary obliquity and equinox can be estimated simultaneously with the mapping under the presence of clouds. We conclude that the photometric variability of the scattered light will be a powerful means for exploring the habitat of a second Earth.}, added-at = {2018-01-31T22:19:31.000+0100}, author = {Kawahara, Hajime and Fujii, Yuka}, biburl = {https://www.bibsonomy.org/bibtex/2f7e92a77b3ca4882c40e2d2ea3c4e26f/clairemarie}, description = {Mapping Clouds and Terrain of Earth-like Planets from Photometric Variability: Demonstration with Planets in Face-on Orbits}, doi = {10.1088/2041-8205/739/2/L62}, interhash = {6124757dbb6843e65f89018ec9e5f912}, intrahash = {f7e92a77b3ca4882c40e2d2ea3c4e26f}, keywords = {maps}, note = {cite arxiv:1106.0136Comment: Accepted for publication in ApJL. Discussion about feasibility for future missions and the red-edge detection is added}, timestamp = {2018-01-31T22:20:34.000+0100}, title = {Mapping Clouds and Terrain of Earth-like Planets from Photometric Variability: Demonstration with Planets in Face-on Orbits}, url = {http://arxiv.org/abs/1106.0136}, year = 2011 }