1 / 5

Bio-signature Test in Search for Exolife: Slim Hamdani EGO VSF School, VIRGO, May 2006

Explore the planet spectrum to detect bio-signatures for exolife. The future of detections lies in planet-integrated spectra. An Earth-integrated spectrum is crucial for testing bio-signatures. Earthshine, Moon, and Earth integrated spectra mirror an Exo-planet spectrum. Key features include 03 Huggins band, Rayleigh scattering, 03 Chappuis band, H2O, O2, vegetation Red-Edge, and Earth Spectra (integrated) for future detections. Dive into the world of bio-signatures with insights from the Darwin mission.

hinto
Télécharger la présentation

Bio-signature Test in Search for Exolife: Slim Hamdani EGO VSF School, VIRGO, May 2006

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Bio-signature test in search for exolife Slim Hamdani EGO VSF School, VIRGO, 22-26 May 2006

  2. Planet spectrum The future detections will be planet integrated spectra So… We need an Earth integrated spectrum to test bio-signatures

  3. Earthshine Moon Earth integrated spectra like an Exo-planet spectra

  4. 03 Huggins band Rayleigh scattering 03 Chappuis band H2O O2 Vegetation Red-Edge Earth Spectra(integrated)

  5. futur detection.... The Darwin mission

More Related