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Course: BIO 5, Fall 2008
School: Hawaii
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(6/02) REGISTRATION Rev. AMENDMENT OR UPDATE [ 1. 2. 4. 6. 8. ] REGISTRATION INVOLVES CONFIDENTIAL INFORMATION OR INTELLECTUAL PROPERTY BSPBSP-5 Principal Investigator: _______________________________________________________________________________ Department/Unit: __________________________________________ 3. Campus Code: _______________________ Building and Room No.:...

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(6/02) REGISTRATION Rev. AMENDMENT OR UPDATE [ 1. 2. 4. 6. 8. ] REGISTRATION INVOLVES CONFIDENTIAL INFORMATION OR INTELLECTUAL PROPERTY BSPBSP-5 Principal Investigator: _______________________________________________________________________________ Department/Unit: __________________________________________ 3. Campus Code: _______________________ Building and Room No.: _____________________________________________ 5. Telephone No.: _______________ Address: __________________________________________________________ 7. Fax No.: _____________________ Granting Agency: __________________________________________ 9. Laboratory Telephone: ________________ 10. 11. 12. IBC Date of Original _________________________________________________________ Authorization: Bi-Annual Update: [ ] No Changes [ ] Project Completed Amendments, changes, to original proposal: [ [ ] Staff changes (deletion and addition) ] Project amended [ [ ] Project Extended ] Other 13. TITLE: Give a Brief Description of Changes/Amendments below: (use additional pages if necessary): 14. Signature of Principal Investigat...

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Hawaii - IFA - 07
ASTROCHEMISTRY A MOLECULAR APPROACH ASTR657Ralf I. Kaiser kaiser@gold.chem.hawaii.eduThe first organizational meeting will be in Bilger Hall, Room 212, Tuesday, August 23, 10:30 am. Agenda: class schedule (regular lectures vs. block lectures) and
Hawaii - IFA - 07
Astr 734 Seminar on THE ORIGIN OF THE CHEMICAL ELEMENTS SPRING 2007 10 weeks, one 75 minute class per week Wed. 1:30 p.m. starting Feb. 14 Useful books: [on reserve at IfA library]"The Origin and Evolution of the Elements" ed. Andrew McWilliam and
Hawaii - IFA - 07
Circumstellar Disks and Planet Formation The 8 week reading seminar will focus on topics related to the study of circumstellar disks, from the primordial, through the planet building, and the debris disk phases. The format and topics to be covered wi
Hawaii - IFA - 07
Astr 736: Formation of Massive Galaxies (1 credit Reading Seminar) This seminar will focus primarily on the formation and evolution of galaxies at the top end of the mass (and luminosity) function, and cover recent observational and theoretical devel
Hawaii - IFA - 06
GG 669 Formation of Solar Systems (Spring 2006)Instructors:Sasha Krot (HIGP) Athos sasha@higp.hawaii.eduJonathan Williams (IfA) Porthos jpw@ifa.hawaii.eduEric Gaidos (GG) Aramis gaidos@hawaii.eduTime: MWF 1:30-2:20 PM First meeting, Monday J
Hawaii - IFA - 08
Course ASTR734 Spring 2008: Instructor: Bo ReipurthBINARY STARS - FORMATION AND EVOLUTIONMost stars in the Universe are binaries. This course will give an overview of our current knowledge of binary and multiple stars, with an emphasis on how bin
Hawaii - IFA - 03
Synopsis for Astronomy 734 "Field Theory for Astronomers" In this 700 level course I will give an elementary introduction to field theory for astronomers. Spontaneous symmetry breaking with a massive scalar field (the Higgs field) provides the founda
Hawaii - IFA - 03
Sub-millimeter AstronomyMonday, Wednesday 11-12:15pm January 13th February 19th 20031. Introduction what is sub-millimeter astronomy? what do you see at sub-millimeter wavelengths? what kind of science can you do? 2. Signal detection detection
Hawaii - IFA - 06
EARLY UNIVERSE PHYSICS Andrew Liddle, University of Sussex, UK 10 lectures Overview: hot big bang cosmology, thermal processes in the Universe Inflation: motivation, modelling, perturbations, observational tests Dark energy: observational status, phe
Hawaii - E - 2214
Prepared by Office of Vice President for Information Technology & CIO and the Office of Vice President for Legal Affairs and University General Counsel This is a NEW Executive Policy UNIVERSITY OF HAWAII EXECUTIVE POLICY - ADMINISTRATION November 200
Hawaii - UHH - 2005
UniversityofHawaiiatHilo FacultyHandbook20052006UpdatedSeptember2005ContentsThis handbook is arranged by major categories of information. Click on headings to go to discussions, or click here to go to the alphabetical index of individual topics.
Hawaii - EHSO - 6
IMPORTANT SAFETY NOTICE - SUUNTO D9 AND D6 DIVING INSTRUMENTSSuunto Oy has identified a software bug in the D9 and D6 diving instruments. The software bug may cause the D9 and D6 to incorrectly track dive time on rare occasions, potentially causing
Hawaii - MS - 4697
Hawaii - AST - 110
Outline of the CourseTABLE OF CONTENTS Part IDeveloping Perspective 4. Our Place in the Universe 5. Discovering the Universe for Yourself 6. The Science of Astronomy Part IIKey Concepts for Astronomy 9. Making Sense of the Universe: Understanding Mo
Hawaii - AST - 110
New Planet Definition Proposed by IAUThe IAU therefore resolves that planets and other Solar System bodies be defined in the following way: (1) A planet is a celestial body that (a) has sufficient mass for its self-gravity to overcome rigid body for
Hawaii - AST - 110
Homework, August 26, 2006AST110-6Due Date: Thursday, September 2, 20061. Review Question 11, Chapter 1 (25%) Define astronomical unit, ecliptic plane, and axis tilt. Explain how each is related to the Earths rotation and/or orbit. 2. Problem 27,
Hawaii - AST - 110
The Ever-Changing SkyThe sky is constantly changing. We experience the day-night cycle every day. Night after night, the pattern of the stars seems identical, yet it changes with the seasons. The motions of some of the celestial objects dont seem to
Hawaii - AST - 110
The Effects of PrecessionWhat changes do you expect in these things (or phenomena) 13,000 years later when the Earths rotation axis is pointed toward Vega? E. World Atlas (map of Earth)? F. Star chart (map of sky)? G. Seasons? H. Constellations? A
Hawaii - AST - 110
Homework, August 31, 2006AST110-6Due Date: Thursday, September 7, 2006 Exploring the sky with SkyGazer:This homework requires using the SkyGazer planetarium software that comes with the text book. However, if you have access to, or are already f
Hawaii - AST - 110
Retrograde motion of Mars, June to November, 2003Who is this guy? Use SkyGazer or StarCal to find out!The Four SeasonsIs the changing seasons caused by the change in the distance between the Sun and the Earth? No. If it is, then The northern an
Hawaii - AST - 110
The Science of Astronomy Ancient Civilizations Ancient Greek European Renaissance Modern ScienceAncient Astronomical KnowledgeMany of the surviving ancient structures have obvious astronomical purpose. These ancient structures clearly demonstr
Hawaii - AST - 110
Homework, September 7, 2006AST110-6Due Date: Thursday, September 14, 20061. Review Question 11, Chapter 2 of the textbook. Suppose you lived on the Sun (and could ignore the heat). Would you still see the Moon go through phases as it orbits Eart
Hawaii - AST - 110
Chapter 4 Motion, Energy, and Gravity Description of Motion Mass and Weight Newtons Law of Motion Newtons Law of Gravity Conservation LawsPrefaceSo far we have only used our knowledge on how the celestial bodies are moving in the universe and
Hawaii - AST - 110
Force, Momentum and EnergyNewtons Laws of MotionOur understanding of how an object reacts to force, or how the motion of an object is affected by force, is summarized by Newtons Laws of Motion: First Law of Motion In the absence of a net force, an
Hawaii - AST - 110
Homework, September 14, 2006AST110-6Due Date: Thursday, September 21, 20061. Chapter 3, Problem 8. Clearly state each of Keplers laws of planetary motion. For each law, describe in you own words what it means in a way that could be understood by
Hawaii - AST - 110
QuestionIf we build a very tall tower with a height of one Earth radius. What would be your weight when you make a measurement with our regular spring scale on the top of the tower? It would be only one-forth of your weight on the ground.Gmearth
Hawaii - AST - 110
Chapter 5 Basic properties of light and matter. What can we learn by observing light from distant objects? How do we collect light from distant objects?Solar SpectrumLight and MatterWhy do we need to study light? Light is the messenger that ca
Hawaii - AST - 110
Homework, September 21, 2006AST110-6Due Date: Thursday, September 28, 2006Chapter 4, Problem 8: Briefly describe and differentiate between kinetic energy, radiative energy, and potential energy. For each type of energy, give at least two example
Hawaii - AST - 110
Atomic Spectra A satellite orbiting the Earth contain gravitational potential energy. The satellite can orbit the Earth at any height. Or, it can contain any amount of gravitation energyIts gravitational potential energy is continuous. Similar to t
Hawaii - AST - 110
Chapter 6 Our Solar System and Its OriginHow was the Solar System Formed?A viable theory for the formation of the solar system must be 1. based on physical principles (conservation of energy, momentum, the law of gravity, the law of motions, etc.),
Hawaii - AST - 110
Homework, September 28, 2006AST110-6Due Date: Thursday, October 5, 20061.Decide whether each statement makes sense and explain why it does or does not. (20pt) a. Chapter 5, Problem 17. If you could view a spectrum of light reflecting off a blu
Hawaii - AST - 110
Condensation of the Solar NebulaComposition of the Solar Nebula As the protoplanetary disk cools, materials in the disk condensate into planetesimals The solar nebular contains 98% Hydrogen and Helium (produced in the Big Bang), and 2% everything e
Hawaii - AST - 110
Midterm Exam Material Covered Chapter 1 to 6 Format of Exam Multiple-Choice Questions: 40 to 50 questions Facts Concepts Reasoning Quantitative - Real Simple Kine!Review for MidtermImportant Facts: What does the universe look like, from
Hawaii - AST - 110
Homework, October 5, 2006AST110-6Due Date: Tuesday, October 17, 20061. Chapter 6, Problem 6 (20pt). Describe each of the three key processes that led the solar nebula to take the form of a spinning disk. What observational evidence supports this
Hawaii - AST - 110
Chapter 7 Earth and the Terrestrial WorldsUnderstanding the similarities and differences between the planets of the solar system, in particular, the four terrestrial planets, can tell us how Earth becomes the way it is today. The similarities and d
Hawaii - AST - 110
Homework, October 19, 2006AST110-6Due Date: Thursday, October 26, 20061. Chapter 7, Review Question 7 (25pt): Describe how Earths atmosphere protects thesurface from harmful radiation. What is the role of ozone?2. Chapter 7, Review Question 1
Hawaii - AST - 110
The Greenhouse Effect on EarthEarths atmosphere is slightly warmer than what it should be due to direct solar heating because of a mild case of greenhouse effect The ground is heated by visible and (some) infrared light from the Sun. The heated su
Hawaii - AST - 110
Chapter 8 Jovian Planet Systems Formation Internal Structure Appearance Weather-the Great Red Spot and bands of Jupiter Satellites-the Galilean Moons of Jupiter RingsOverview: Similarities and DifferencesThe jovian planets can be roughly div
Hawaii - AST - 110
Homework, October 26, 2006AST110-6Due Date: Tuesday, November 2, 20061. Chapter 8. Review Question 1. Briefly describe how the differences in composition among the jovian planets can be traced to their formation in the solar nebula. 2. Chapter 8
Hawaii - AST - 110
Chapter 10 The Sun, Our Star The Sun support life on Earth 1. The Sun provides energy for photosynthesis, which releases oxygen into the atmosphere. 2. The greenhouse effect trap some of the solar energy on Earth, keeping it warm (at the right tempe
Hawaii - AST - 110
General Properties Internal Structure Solar Atmosphere Photosphere, chromosphere, and corona Surface Features and Magnetic Fields Solar Activities Solar Cycle Sun-Earth ConnectionThe Surface of the SunIn images of the Sun, we see a sharp
Hawaii - AST - 110
Homework, November 2, 2006AST110-6Due Date: Thursday, November 9, 20061. Describe the structure of the Sun from the core, radiative zone, and convection zone in the interior to the photosphere, the chromosphere, and the corona in its atmosphere.
Hawaii - AST - 110
Chapter 11 Stars Properties of Stars Classifying Stars Hertzsprung-Russel (H-R) Diagram Star Clusters Open and Globular ClustersProperties of Stars Mass The single most important property that determines other properties of the star. Luminos
Hawaii - AST - 110
Homework, November 9, 2006AST110-6Due Date: Thursday, November 16, 20061. If nuclear fusion of hydrogen in the core of the Sun were to stop now, what would we see on the surface of the Sun tomorrow? Why? Will we be able to tell that hydrogen bur
Hawaii - AST - 110
Mass and the Properties of Main Sequence StarsMass is the most important properties of themain-sequence stars. It determine their luminosity, surface temperature, radius, and lifetime. Nuclear fusion requires high temperatures and densities in the
Hawaii - AST - 110
Star Formation Evolution of Low-Mass Stars Evolution of High-Mass StarEvolution of High-Mass Stars IM > 8 10 MThe early stages of a high-mass stars life are similar to the earlystages of the life of low-mass stars, except they proceed muc
Hawaii - AST - 110
Homework, November 16, 2006AST110-6Due Date: Tuesday, November 28, 20061. Chapter 12, Problem 23 to 28 [60pt]. Homes to Civilization? We do not yet know how many stars have Earth-like planets, nor do we know the likelihood that such planets migh
Hawaii - AST - 110
Chapter 13 The Stellar Graveyard Degeneracy Stars Brown Dwarfs White Dwarfs Neutron Stars Black HolesX-ray image of supernova remnant G11.2-03, from A.D.386.The Dead StarsThe End States of Stars Nothing White dwarfs Neutron stars Black h
Hawaii - AST - 110
Black Holes: Do They Really Exist?We cannot see black holes directly, so we have to look for indirect evidencesWhat would you look for to find a stellar-mass black hole, like those formed after the death of high mass stars? To look for black holes
Hawaii - AST - 110
Homework, November 28, 2004AST110-6Due Date: Tuesday, December 5, 20061.Chapter 14. Review Question 1. (20 pts) What is degeneracy pressure, and how is it important to white dwarfs and neutron stars? What is the difference between electron deg
Hawaii - AST - 110
Chapter 15, GalaxiesGalaxies come in different size and shape. In the previous chapter, we talked about howgalaxies provide an environment for the stars to be born and die, and enrich the heavy element content of the galaxy. In this chapter, we wil
Hawaii - AST - 110
Possible Fate of the UniverseWe already know that the universe is expanding. Only the pull of the gravitational force canslow it down. So, similar to the fate of the stars, how the universe evolves depends on how much matter we have in the universe
Hawaii - AST - 110
Science News Signs of Flowing Water on MarsTODAY!Bright new deposits seen in NASA images of two gullies on Mars suggest liquid watercarried sediment in the past several yearsThe atmosphere on Mars is so thin that liquid water cannot persist at the
Hawaii - A - 281
Astrobiology OverviewAST 281 T-Th 12:00-1:15 WAT 420Business ItemsInstructor: Karen MeechAstronomer (comets, early solar system) Participation in several space missions (DI + 2 new) NASA Astrobiology InstituteOffice & HoursWat 404 Tu/Th 13:1
Hawaii - A - 281
Light & RadiationKaren J. Meech, Astronomer Institute for AstronomyFundamentalsLight has wave propertiesOscillating electric & magnetic fieldsCharacterized byWavelength, Frequency, f [Hz] Travels at c = 3 x 105 km/s c=fLight carries energ
Hawaii - A - 281
Exogenic Terrestrial ProcessesKaren J. Meech, Astronomer Institute for AstronomyExogenicProcesses arising from outside objectInteraction with meteoroidsCratering and regolith formationApplications:Relative surface ages Excavation of material
Hawaii - A - 281
Comets, Primitive Bodies and the Real Deep ImpactKaren J. Meech, Astronomer Institute for AstronomyComet km-sized bodies with volatiles & refractories Asteroid small planetary bodies orbiting the sun (mostly refractory) Meteroid small (< km) ex
Hawaii - A - 281
Endogenic ProcessesKaren J. Meech, Astronomer Institute for AstronomyExogenic & EndogenicExogenic Processes arising from outsideImpact cratering MicrometeoritesRegolith GardeningSolar wind & cosmic raysChemical processingEndogenicTectoni
Hawaii - A - 281
Endogenic: Ices, Isotopes, DatingKaren J. Meech, Astronomer Institute for AstronomyFundamental Atomic Building Blocks# protons (Z) # neutrons (N) Atomic mass A=Z+N Isotope (equal place)Differing values of N and A, same Z Same chemical properties
Hawaii - A - 281
Atmospheric ProcessesKaren J. Meech, Astronomer Institute for AstronomyOutlineHistory and comparison of Atmospheres Atmospheric Structure & Composition Aeolian ProcessesOf or pertaining to an atmosphereWind processes Liquid surfaceSome Exampl
Hawaii - A - 281
Life and Its RequirementsKaren J. Meech, Astronomer Institute for AstronomyIs it Important that we have a definition is this possible?Life is a self-sustained chemical system capable of undergoing Darwinian evolution (Joyce, 1994) Life is a self