National Science Olympiad Solar System B Event 2015 Planetary Science.

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National Science Olympiad Solar System B Event 2015 Planetary Science

Chandra X-Ray E/PO Office Donna L Young, NSO Astronomy Event Supervisor – Dusty Schroeder, NSO Solar System Event Supervisor –

The American Association of Variable Observers aavso.org

SOLAR SYSTEM, DIVISION B: Planetary Science DESCRIPTION: Students will demonstrate an understanding and knowledge of the properties and evolution of extraterrestrial ice and water in the solar system. A TEAM OF UP TO: 2 APPROXIMATE TIME: 50 minutes EVENT PARAMETERS: Each team may bring only two 8.5” x 11” two-sided pages of information in any form from any source. THE COMPETITION: This event is divided into two parts. Notes may be used during both parts.

Part I: Participants may be asked to identify planets, moons, and features included in the lists below as they appear on maps or imagery and must be knowledgeable about the history and processes involving ice and water for the objects below. (1) Mars: North & South Polar Ice Caps, Equatorial Glaciers, Permafrost (2) Europa: Thrace Macula, Thera Macula, Conamara Chaos, Ridges, Cycloids, Plains, Ocean (3) Enceladus: Plumes, Tiger Stripes (4) Iapetus, Titan, Triton, Ceres, (5) Comets, The Kuiper Belt, The Oort Cloud Part II: Participants will be asked to complete one or more hands-on or interpretive tasks selected from the following topics: i: The history and process of formation for specific features ii: The use of remote sensing, imagery, and satellite measurements of objects and features iii: The physical, thermal, and chemical properties of potential habitats for life iv: Past, current, and planned future missions to explore these objects

Part I: Identification Mars

North Polar Ice Cap

Seasonal Changes

ESA Mars Express Infrared Mineralogical Mapping Spectrometer (OMEGA) – phyllosilicates High Resolution Stereo Camera (HRSC) – volcanism Planetary Fourier Spectrometer (PFS) – Methane Summer Solstice Transition

South Polar Ice Cap – Mars Odyssey Mission

Sand Jets – spring thaw Thermal Emission Imaging System (THEMIS)

Equatorial Glaciers Mars Reconnaissance Orbiter

permafrost – polygons The Phoenix Mission

Europa

Thera Macula & Thrace Macula

Conamara Chaos

Ridges

Cycloids

Plains

Oceans

Enceladus:

Plumes

Tiger Stripes

Iapetus

Transition Zone

The Wall

Titan

Triton

Ice Volcanoes

Ceres

Comets

The Oort Cloud

The Kuiper Belt

Part II: Interpretation History and Process of Formation for Specific Features

Mars

Titan Europa

Remote Sensing, Imagery, Satellite Measurements of Objects & Features

Physical, Thermal, and Chemical Properties of Potential Habitats for Life

EXTREMOPHILES Psychrophiles, Thermophiles, Radioresistant, Alkaliphiles, Acidophiles, Halophiles, Xerophiles, Barophiles, Endoliths AND gravity!

Missions

Missions to Mars

Future Missions?

Future Missions – JUICE

chandra.harvard.edu – Webinars – Everything Solar System apod.nasa.gov – Images, Content aavso.org – 2014 Events, Flash Cards, PPTs h ttp://soinc.org

National Astronomy Event Supervisor – Dusty Schroeder Rules clarifications: available at under event information Event Preparation: 1.Read the Event Description for content and allowable resources. 2.Use the Webinar and PowerPoint for an overview of the content topics, landforms, features, planets and moons. 3. Use the JPL website for images and content. 4. Download the 2014 event and flash card set from the AAVSO website, and watch the webinar on the Chandra website.