2006 Annual Science Report
Astrobiology Roadmap Objective 1.2 Reports Reporting | JUL 2005 – JUN 2006
Roadmap Objective 1.2—Indirect and direct astronomical observations of extrasolar habitable planets
Project Reports
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Characterization of Terrestrial Planets From Disk-Averaged Spectra: Spatially and Spectrally Resolved Planetary Models
ROADMAP OBJECTIVES: 1.2 7.2 -
Planetary Biology, Evolution, and Intelligence
Chris Chyba, Cynthia Phillips, Kevin Hand- The project has two components. The first, an overview of the astrobiological potential of various geological features on Europa, is proceeding well — we are continuing the study of various proposed formation mechanisms for different feature types such as ridges, bands, and chaotic terrain.
ROADMAP OBJECTIVES: 1.1 1.2 2.1 2.2 3.1 3.2 4.1 4.2 5.1 5.2 5.3 6.1 6.2 7.1 -
Disks and Dips
ROADMAP OBJECTIVES: 1.1 1.2 -
Project 1. From Molecular Clouds to Habitable Planetary Systems
The work this year of Co-Investigator Chambers involved the development of a model for the oligarchic growth stage of planet formation, a key stage that determines many of the final characteristics of a planetary system
ROADMAP OBJECTIVES: 1.1 1.2 2.1 3.1 7.2 -
A 1-D Climate Model for Extrasolar Terrestrial Planets
ROADMAP OBJECTIVES: 1.1 1.2 7.2 -
Climate, Habitability, and the Atmosphere on Early Mars
ROADMAP OBJECTIVES: 1.1 1.2 2.1 4.1 7.1 -
Module 3: Nature of Planetary Systems
Direct detection for extrasolar planets is fast becoming a reality, and LAPLACE is well-poised to be the forefront of this new area of research. Using multiple techniques we are now in the process of carrying out surveys for young planets as well as developing new techniques which will push our sensitivity to older planets around more nearby stars.
ROADMAP OBJECTIVES: 1.1 1.2 -
Direct Detection and Characterization of Extrasolar Planets
Drake Deming and collaborators expanded their direct detection of “hot Jupiter” planets orbiting other stars
ROADMAP OBJECTIVES: 1.2 -
No Title Given
We have been observing circumstellar environments around
other stars to learn about the formation and evolution of extrasolar planetary systems. There are two highlights of our workROADMAP OBJECTIVES: 1.2 -
Habitable Planets
ROADMAP OBJECTIVES: 1.1 1.2 2.1 4.1 4.3 -
Database of Stellar Spectra to Support Extrasolar Planet Modeling
We established a database of stellar spectra during the past year to serve as a
dynamic repository within the VPL website for accurate reference spectra of stars
that are considered relevant hosts in the search for habitable exoplanets.ROADMAP OBJECTIVES: 1.2 4.1 6.2 7.2 -
Model Synthesis and Architecture
The VPL integrated model to develop self-consistent planetary environments has acquired several separate components into its model suite over the past year, including weathering, land model, and tectonic/solid earth components. These are now housed in a version controlled online database of all VPL software components, including the coupled online model as well as other model components under development.
ROADMAP OBJECTIVES: 1.1 1.2 4.1 4.3 7.2 -
Modeling Terrestrial Planet Formation and Composition
We have run the most realistic simulations of the final stages in the formation of Earth-like planets to date (Raymond), including 10 times as many particles as previous simulations.
ROADMAP OBJECTIVES: 1.1 1.2 3.1 -
Planetary Habitability and Life Detection (Sigurdsson)
ROADMAP OBJECTIVES: 1.1 1.2 -
Extrasolar Planet Detection and Characterization
ROADMAP OBJECTIVES: 1.2 7.2 -
Search for Planets Around Evolved Stars (Wolszczan)
ROADMAP OBJECTIVES: 1.2 -
A Search for H3+ Emission From Close-In Exoplanets
ROADMAP OBJECTIVES: 1.2