Sponsors —
Lunar and Planetary Institute
NASA Science Mission Directorate
NASA Mars Exploration Program

Conveners —
Allan Treiman,
   Lunar and Planetary Institute
Adriana Ocampo,
   NASA Science Mission Directorate
Ellen Stofan,
   Proxemy, VEXAG
Stephen Mackwell,
   Lunar and Planetary Institute

Science Organizing
Committee —
Allan Treiman,
   Lunar and Planetary Institute
Linda Elkins-Tanton,
   Massachusetts Institute of Technology
George Hashimoto,
   Kobe University
Natasha Johnson,
   NASA Goddard Space Flight Center
Eric Essene,
   University of Michigan
Stephen Mackwell,
   Lunar and Planetary Institute

MEETING LOCATION AND DATE

The Workshop on Venus Geochemistry: Progress, Prospects, and New Missions will be held February 26–27, 2009, at the Gilruth Center at NASA Johnson Space Center. The workshop will be held after the general VEXAG meeting, planned for Wednesday, February 25.

Invited presentations scheduled to date include plenary addresses by Dr. M. Marov on the Soviet Venus mission, Dr. J. Helbert on Venus Express results, and Dr. D. Grinspoon on the importance of Venus and of new spacecraft missions.

KEY POINTS:
  When:
     February 26–27, 2009
  Where:
     Houston, Texas

Although Venus is the “Terra Incognita” of the inner solar system, it is supremely important for understanding the formation and evolution of terrestrial planets. Venus, which is Earth’s twin in size (and possibly bulk composition), is fundamentally different in its surface geology, tectonics and internal processes, and atmosphere composition and dynamics. These differences contain clues to the evolution of Earth’s geology/climate system, Earth’s current habitability, and the detectability and habitability of planets circling other stars.

Our understanding of Venus’ origins and evolution is hampered by the dearth of data about its surface. The few images and chemical analyses from the Venera and VEGA landers (crucial but limited) show that Venus’ lowland plains are basaltic, with some unusual (and unexplained) compositions. To date, we know nothing of the geochemistry of Venus’ highlands, central volcanos, coronae, domes, etc. Venus’ atmosphere provides significant constraints on its history (e.g., noble gases and light isotopes), but its chemical interactions with surface materials are poorly constrained.

Given the limited knowledge about Venus’ geochemistry, along with NASA’s interest in Venus, as demonstrated in the recent Venus Science and Technology Definition Team study, the Venus Geochemistry workshop has several objectives:

• to assess current knowledge of Venus’ geochemistry
• to consider Earth-based investigations (laboratory and theoretical) that will enhance understanding of current data and enable future investigations
• to explore concepts for spacecraft instruments and missions that will increase knowledge of Venus’ geochemistry
• to energize and reconstitute the Venus geochemistry community in preparation for future spacecraft investigations.

To support these objectives, the workshop sessions will focus on:

• present knowledge of Venus’ geochemistry: atmosphere, surface, mantle core, and whole planet
• chemical interactions between Venus’ surface and atmosphere
• laboratory investigations (solids, fluids, gases) to further understanding of Venus’ geochemistry
• recent Venus missions and remote sensing of its surface and interior
• geochemistry on future missions to Venus: concepts, investigations, and instruments
  
  

The workshop will include invited and contributed talks and contributed poster presentations. Oral presentations will be limited to 15 minutes including discussion. Plenary lectures will be 30 minutes including discussion. Oral sessions will start Thursday morning, February 26, and continue through Friday, February 27. On Thursday evening there will be a reception and poster session. Posters will be displayed during the entire workshop.

A general VEXAG meeting is planned for Wednesday, February 25, 2009, before the workshop.

Researchers in scientific disciplines appropriate to the purpose and scope of this workshop are invited to submit abstracts for oral and poster presentation.

All abstracts, whether invited or contributed, must be submitted electronically to the Lunar and Planetary Institute via the electronic submission form by 5:00 p.m. U.S. Central Standard Time on Thursday, December 4, 2008 (see timezone map). Abstracts will be limited to two pages, including graphics, tables, and references, and MUST be submitted in PDF format. Templates and detailed instructions for formatting and submitting your abstract are provided.

Note:  It is in your best interest to submit early to allow for possible technical problems or delays in transmission. Please do not wait until the last minute to access the system; access to the web form will terminate at 5:00 p.m. CST.

The program and abstracts will be available in electronic format and accessible via the meeting website by January 6, 2009. These files will be in PDF format. Authors should check the online program to find out when their abstract has been scheduled.

To encourage student participation and help renew the Venus science community, NASA is providing support for students to attend the Venus Geochemistry Workshop. Student support can include travel, lodging, and per diem expenses, and will be arranged through the Jet Propulsion Laboratory. To apply for support, students should:

• e-mail a short letter (1–2 pages) to Dr. Allan Treiman, describing how Venus would be included in their future research and/or is in their present work
• provide a brief e-mail of support from an academic advisor or professor

KEY POINTS:
Registration through Jan. 23:
     Professional — $125.00
     Student — $75.00
Registration Jan. 24–Feb. 22:
     Professional — $150.00
     Student — $100.00

Onsite Registration:
      Professional — $175.00
      Student — $125.00

Participants are responsible for making their own travel and hotel reservations. For your convenience, a list of local hotels and a local area map showing their locations are provided.

For further information regarding the format and scientific objectives of the meeting, contact

Allan Treiman
Lunar and Planetary Institute
phone: 281-486-2117
e-mail: treiman@lpi.usra.edu

For further information regarding meeting logistics, please contact

Kimberly Taylor
Lunar and Planetary Institute
phone:  281-486-2151
e-mail:  taylor@lpi.usra.edu

For further information regarding abstract submission or registration, please contact

Linda Tanner
Lunar and Planetary Institute
phone:  281-486-2142
e-mail:  tanner@lpi.usra.edu