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Computational Astrobiology Summer School Introduction

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Title: Computational Astrobiology Summer School Introduction


1
Computational Astrobiology Summer School
Introduction
  • Kim Binsted
  • NASA Astrobiology Institute
  • and
  • Information Computer Sciences Dept
  • University of Hawaii
  • binsted_at_hawaii.edu

2
Introductions
3
Admin
4
Today
  • Overview of CASS
  • Campus orientation and poster posting
  • Lunch with NAI postdocs

5
Travel expenses
  • Before you go, give me
  • WH-1 form, signed
  • Non-employee reimbursement form
  • Receipts
  • Boarding passes (if you can print them
    otherwise, send as soon as you can)
  • Youll receive a fixed amount (500), less taxes
    (if you dont give me the boarding passes).

6
Schedule
  • See
  • http//www2.hawaii.edu/binsted/CASS/schedule.html
  • There are still some readings etc. to be
    uploaded, so please check every day or so.
  • Note the two locations POST 126 (here) and the
    Waterhole (will show later)

7
Daily routine
  • 9am lecture starts
  • 1015am coffee break
  • 1030-12 Discussion
  • 12 session ends
  • The discussion is not for just asking questions
    about the lecture it is for brainstorming ideas
    for projects. Please be prepared to talk.

8
Afternoons
  • Free time, but please use productively
  • Doing readings
  • Library
  • Drafting project ideas
  • Surfing

9
Public Lecture
  • Searching for Life in the Universe
  • Seth Shotak and Chris McKay
  • Friday July 28, 730pm-9pm
  • Arts 132 (see campus map http//www.hawaii.edu/ca
    mpusmap/)
  • Reception at 630pm in the Arts building please
    attend!

10
Ocean Field Trip
  • Details to follow, but roughly
  • Carpool to Kaneohe, to arrive at noon
  • Morning Tour of Coconut Island
  • Afternoon Kayaking on Kaneohe Bay
  • Carpool back to Honolulu, returning about 7pm.

11
Big Island Field Trip
  • Sat Aug 5, 710am HNL Hilo. Be at the airport
    by 610am.
  • Drop bags at hotel, go to Mauna Kea for summit
    tour and stargazing at vistors center.
  • Sun Aug 6 Volcanoes National Park.
  • 843pm Hilo HNL.
  • Anyone NOT going, let me know now!!

12
Project Presentations
  • On the last day, please be ready to give a short
    (15min) presentation on what you plan to do for
    your project.
  • Give as much detail as possible scope,
    interface, languages, expected completion date
    etc. Dont worry, you can change your mind on
    these things!
  • Email your presentation (pref. PowerPoint) to me
    before you go.

13
On your return
  • Meet with your mentor, and discuss your project
    plan. Modify as necessary.
  • Send me a monthly progress report (casual email
    OK).
  • Youre not finished until I have a
    well-documented version of your code!
  • Aim to have something to present/demonstrate at
    Bioastronomy 2007 (July 16-20, Arecibo). Travel
    funding will (hopefully) be available.

14
Overview
15
What is Astrobiology?
  • Scientific research into the origin,
    distribution, and destiny of life in the
    universe.
  • Practically speaking astronomers, biologists,
    chemists, geologists, computer scientists, etc.
    doing their research in a larger context Earth
    as one (very rich!) data point, rather than the
    whole story.
  • Inherently interdisciplinary.

16
Drake equation
  • NRfp ne fl fifcL , where
  • N number of civilizations in our galaxy whose
    electromagnetic emissions are detectable.
  • R rate of formation of stars.
  • fp fraction of those stars with planetary
    systems.
  • ne number of planets, per solar system, with an
    environment suitable for life.

17
Drake equation (2)
  • fl fraction of suitable planets on which life
    actually appears.
  • fi fraction of life bearing planets on which
    intelligent life emerges.
  • fc fraction of civilizations that develop a
    technology that releases detectable signs of
    their existence into space.
  • L The length of time such civilizations release
    detectable signals into space.

18
Astrobiology and SETI
  • Either sharply distinguished or muddled together,
    depending on funding atmosphere (currently one
    happy family)
  • Roughly, astrobiology works on the first four
    factors of the Drake equation, and SETI works on
    the last three (as well as attempts at direct
    detection)
  • The SETI Institute is a team member in the
    distributed NASA Astrobiology Institute.

19
Astrobiology at UH
  • Part of (and funded by) the NAI
  • 18 co-Is, from astronomy, chemistry, planetary
    geology, biology, oceanography, computer science
  • 11 postdocs
  • Many grad students
  • Theme The origin, history, distribution and role
    of water as it relates to life in the universe.

20
How does CS fit in?
  • Astrobiology research can benefit from using
    up-to-date computational techniques and resources
  • Astrobiologists may or may not be aware of
    developments in computer science/engineering
  • Computer scientists may or may not be aware of
    what astrobiologists need
  • We need to bring them together!

21
Our approach
  • Encourage computer science students to tackle
    problems in astrobiology, via
  • NASA Space Grants for undergraduate research
  • ICS 691 Graduate seminar/project course,
    Computational Astrobiology
  • CASS Computational Astrobiology Summer School
    2006
  • Encourage astrobiologists to talk to ICS
    students, especially those that need to do
    capstone projects.

22
Some current/past student projects
  • From fairly basic web interfaces to ongoing
    research

23
Web interface for Deep Impact ground based
observation database
  • with Karen Meechstudent Johnny Saucedo

24
Deep Impact
25
Requirements
  • Search for observations by institution,
    telescope, observatory, observer, operator,
    and/or instrument
  • Edit magnitude, filter type, and error for any
    observation
  • Help available via pop-up windows

26
Status
  • Completed
  • Funded by UH-NASA Space Grant Fellowship for
    undergraduate research
  • Won a UH undergraduate research prize

27
Lowell Telescope Scheduler
  • with Marc Buie (Lowell), Karen Meech, Mary
    Kadooka
  • students Derek Shirae, Scott Ibara, Nick Bradley

28
Motivation
  • Many large and medium-size research telescopes
    are devoted to particular projects (e.g. Pluto
    observations), so sit unused when its target
    observations are not possible.
  • Principal Investigators (PIs) would be happy to
    share with other observers, but are unwilling to
    spend time scheduling amateur observations every
    night.

29
Telescope scheduler interface
  • Needed
  • A night-by-night observation scheduler for an
    automatic telescope
  • A database of requested observations
  • An interface that allows amateur astronomers to
    request a wide range of observations from the
    telescope, and retrieve the resulting data

30
Scheduling Constraints
  • The scheduler must
  • Prioritize the PIs observations.
  • Use observing time efficiently.
  • Take advantage of unusual conditions.
  • Complete observation sequences, even when
    disperse.
  • Complete background tasks (e.g. calibration).
  • Avoid damaging the telescope.
  • Run quickly at the beginning of each observation
    period.

31
Interface Requirements
  • The interface must help students
  • Decide what they want to observe.
  • Specify observation constraints (preferably
    soft rather than hard)
  • Make practical requests (i.e. likely to be
    granted)
  • Use the telescopes capabilities (e.g. filters)
    effectively.

32
Status
  • Database Done.
  • Interface Done, but should be improved to make
    easier for students to use.
  • Scheduler Done, but PI needs improvements.
  • Next steps
  • Multi-night, dynamic scheduler
  • Adaptive user interface
  • Paper (co-authored by students) presented at
    IMSA05.

33
Calibration/processing tool for in-situ
voltammeter
  • with Brian Glazer, Jim Cowen
  • students Kayo Fujiwara, Bryan Norman

34
Requirements
  • Consistently detect peaks and peak heights from
    voltammeter probe
  • Determine calibration curve for each probe and
    element
  • Efficiently process data, returning quantities of
    each element detected
  • Interface to improve ease of use

35
Status
  • Peak detection algorithm done
  • Calibration curve calculation done, needs
    improvement
  • Interface done
  • Future work In-situ data processing, allowing
    adaptive data gathering

36
Simulation of adaptive intelligence
  • with Sam Joseph
  • student Cliff Tomosada

37
Problem how adaptive is intelligence?
  • To what range of conditions is intelligence
    adaptive?
  • Is it just a peacocks tail?
  • Is there a range of conditions under which we
    should expect intelligence to evolve?
  • Hypothesis There are ideal frequency/severity
    profiles of environmental challenges that drives
    the evolution of intelligence.

38
Our approach
  • Define intelligence as
  • adaptation on an individual time scale
  • on-board simulation of environment
  • ability to pass acquired information over
    generations
  • Simulate species with varying intelligence,
    generation length, energistic requirements etc.
    under varying environmental regimes
  • Compare simulation to known histories of species
    with varying brain/body ratios.

39
Results (1)
40
Results (2)
41
Problems
  • Sea lion EQ problematic due to difference in size
    between males and females (we used female size)
  • Scaling factors on environmental disruptions
    principled, but need stronger justification.
  • Simulation is crude, and arguably doesnt take
    into account differential effects of various
    kinds of disruptions.

42
Status
  • Beta version of simulation complete
  • Seal / sea lion population comparisons not ideal
    looking for other data sources
  • Next steps
  • Refine simulation
  • More species
  • Make predictions re just right conditions for
    intelligence

43
Wireless sensor networks for extreme environments
  • with Edo Biagioni
  • students Nitin Nagar, Faye Yuen, Mary Liang

44
Problem
  • Want to monitor conditions in extreme
    environments with minimal personal attention from
    humans
  • Maximize data return by extending sensor life
  • Prioritize any repair/maintenance attempts by
    sensors/robots/humans

45
Status
  • Adaptive protocol for sensor network developed,
    tested, deployed on small scale
  • Basic hardware development in progress
  • Hope to deploy in Atacama (Chris McKay),
    Kamchatka (Gilichinsky)
  • Looking for funding

46
Bioinformatics Tools
  • with Andy Boal, Mark Brown
  • students Derek Shirae, Charles Hall, Jimmy Saw

47
Problem
  • Andy Boals research (protein adaptation to
    extreme environments) requires efficient search
    and analysis tools.
  • Also, can we generate/discover novel proteins
    that should be robust under extreme conditions?

48
Status
  • Basic bioinformatics tools (scripts) developed
    and used.
  • More advanced version(s) with streamlined user
    interface developed by ICS 691 students.
  • Three papers submitted, using analysis
  • Genetic algorithm generates novel robust proteins
    with interesting features

49
AFAR Adaptive Framework for Astrobiology Research
  • with Rich Gazan
  • student Marc LePape

50
Problem
  • Astrobiology is highly interdisciplinary no one
    person knows it all
  • Identifying interesting unknowns (esp. for
    collaborative research) is difficult
  • An in-depth overview would be useful for
    outreach/education efforts

51
Our approach
  • Develop adaptive, zoomable knowledge map of the
    state of astrobiology
  • Make adding new knowledge automatic when
    possible, trivially easy when not
  • Bootstrap with existing resources (e.g.
    astrobiology handbook, roadmap, etc.)

52
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53
Status
  • Funding proposals submitted
  • Hope to entice PhD student or CASS participant

54
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