The Date Equation. Estimate the number of people at a party who are willing to go out with you afterwards. From David Grinspoon: Lonely Planets
|
|
- Gillian Hill
- 5 years ago
- Views:
Transcription
1 The Drake Equation
2 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards From David Grinspoon: Lonely Planets
3 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards N = R f p f at f av f n f i L
4 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards N = R f p f at f av f n f i L R: rate at which people arrive at party
5 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards N = R f p f at f av f n f i L R: rate at which people arrive at party f p : fraction who meet your sexual preference
6 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards N = R f p f at f av f n f i L R: rate at which people arrive at party f p : fraction who meet your sexual preference f at : fraction you find attractive
7 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards N = R f p f at f av f n f i L R: rate at which people arrive at party f p : fraction who meet your sexual preference f at : fraction you find attractive f av : fraction who are available to go out
8 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards N = R f p f at f av f n f i L R: rate at which people arrive at party f p : fraction who meet your sexual preference f at : fraction you find attractive f av : fraction who are available to go out f n : fraction you get up the nerve to ask
9 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards N = R f p f at f av f n f i L R: rate at which people arrive at party f p : fraction who meet your sexual preference f at : fraction you find attractive f av : fraction who are available to go out f n : fraction you get up the nerve to ask f i : fraction who are interested in you
10 The Date Equation Estimate the number of people at a party who are willing to go out with you afterwards N = R f p f at f av f n f i L R: rate at which people arrive at party f p : fraction who meet your sexual preference f at : fraction you find attractive f av : fraction who are available to go out f n : fraction you get up the nerve to ask f i : fraction who are interested in you L : length of time people stay at the party From David Grinspoon: Lonely Planets
11 N = N * f s f p n h f l f i f c L/T The Drake equation, formulated by Dr. Frank Drake in about 1960, provides a framework for estimating the number of intelligent civilizations in the Galaxy
12 N = N * f s f p n h f l f i f c L/T N: Number of civilizations in our Galaxy capable of interstellar communication. N * : Number of stars in the Galaxy f s : Fraction of stars suitable for supporting life f p : Fraction of stars with planets n h : number of habitable planets per star f l : fraction of habitable planets on which life evolves f i : fraction of cases where intelligent life develops f c : fraction of intelligent life that develops technological civilizations L : lifetimes of a technological civilization T : age of the Galaxy Note: N * /T = R *, the rate of star formation in the Galaxy.
13 N = N * f s f p n h f l f i f c L/T N: Number of civilizations in our Galaxy capable of interstellar communication. N * : Number of stars in the Galaxy f s : Fraction of stars suitable for supporting life f p : Fraction of stars with planets n h : number of habitable planets per star f l : fraction of habitable planets on which life evolves f i : fraction of cases where intelligent life develops f c : fraction of intelligent life that develops technological civilizations L : lifetimes of a technological civilization T : age of the Galaxy Terms we know well
14 N = N * f s f p n h f l f i f c L/T N: Number of civilizations in our Galaxy capable of interstellar communication. N * : Number of stars in the Galaxy f s : Fraction of stars suitable for supporting life f p : Fraction of stars with planets n h : number of habitable planets per star f l : fraction of habitable planets on which life evolves f i : fraction of cases where intelligent life develops f c : fraction of intelligent life that develops technological civilizations L : lifetimes of a technological civilization T : age of the Galaxy Terms we can estimate with some precision
15 N = N * f s f p n h f l f i f c L/T N: Number of civilizations in our Galaxy capable of interstellar communication. N * : Number of stars in the Galaxy f s : Fraction of stars suitable for supporting life f p : Fraction of stars with planets n h : number of habitable planets per star f l : fraction of habitable planets on which life evolves f i : fraction of cases where intelligent life develops f c : fraction of intelligent life that develops technological civilizations L : lifetimes of a technological civilization T : age of the Galaxy Terms that depend on biology and evolution
16 N = N * f s f p n h f l f i f c L/T N: Number of civilizations in our Galaxy capable of interstellar communication. N * : Number of stars in the Galaxy f s : Fraction of stars suitable for supporting life f p : Fraction of stars with planets n h : number of habitable planets per star f l : fraction of habitable planets on which life evolves f i : fraction of cases where intelligent life develops f c : fraction of intelligent life that develops technological civilizations L : lifetimes of a technological civilization T : age of the Galaxy Terms that we can only speculate about
17 N = N * f s f p n h f l f i f c L/T The Drake Equation: a way of encapsulating a lot of ignorance in a small space! We know: N * f p T We can estimate: f s n h We guess: f l f i f c L
18 Can you estimate? Number of piano tuners in Chicago? (this was the original Fermi problem) Number of pizzerias on Long Island? Number of cars on the New Jersey Turnpike? Number of bathroom stalls at Yankee Stadium?
Expected Value - Revisited
Expected Value - Revisited An experiment is a Bernoulli Trial if: there are two outcomes (success and failure), the probability of success, p, is always the same, the trials are independent. Expected Value
More informationExtrasolar Planets What are the odds?
Honors 228: Astrobiology using Bennett and Shostak Chapter 12 overview Spring 2007 Dr. H. Geller What s talked about The Drake Equation (12.1) The Question of Intelligence (12.2) Searching for Intelligence
More informationExtraterrestrial Life Group Discussion
Extraterrestrial Life Group Discussion Group Assignment Meet with the other members of your group. Assign group roles. Print names below. Your name must appear below in order to receive credit. Recorder
More informationA New Empirical Constraint on the Prevalence of Technological Species in the Universe. - A. Frank 1 & W.T. Sullivan, III 2
A New Empirical Constraint on the Prevalence of Technological Species in the Universe - A. Frank 1 & W.T. Sullivan, III 2 Abstract: In this paper we address the cosmic frequency of technological species.
More informationASTR 380 The Drake Equation
ASTR 380 The Drake Equation Aside: Rosetta Mission - Landing on a Comet! Aside: Rosetta Mission - Landing on a Comet! ASTR 380 The Drake Equation Drake Equation Methodology Reviewing Drake Equation factors
More informationNSCI EXTRASOLAR PLANETS (CONTINUED) AND THE DRAKE EQUATION. Dr. Karen Kolehmainen Department of Physics, CSUSB
NSCI 314 LIFE IN THE COSMOS 14 - EXTRASOLAR PLANETS (CONTINUED) AND THE DRAKE EQUATION Dr. Karen Kolehmainen Department of Physics, CSUSB http://physics.csusb.edu/~karen/ METHODS FOR DETECTING EXTRASOLAR
More informationSearch for Extra-Terrestrial Intelligence
Search for Extra-Terrestrial Intelligence Life in the Universe? What is life? (as we know it) Auto-regulation (ex. : sweating) Organization (A cell is more organized than a bunch of atoms) Metabolism :
More informationThe Jamie Drake Equation
The Science of The Jamie Drake Equation From wafer- sized spaceships to the extraterrestrial Wow! signal, here s more about the real- life science in The Jamie Drake Equation. Aliens don t really exist,
More informationThe Quest for Extraterrestrial Signals. Ron Maddalena National Radio Astronomy Observatory Green Bank, WV
The Quest for Extraterrestrial Signals Ron Maddalena National Radio Astronomy Observatory Green Bank, WV Associated Universities, Inc; April/2016 2 Preliminary thoughts a. How certain are you that other
More informationASTR 380 The Drake Equation
ASTR 380 The Drake Equation 1 ASTR 380 The Drake Equation Drake Equation Methodology Reviewing Drake Equation factors that we know The star formation rate Estimating the number of Earth-like planets or
More informationSearching for Life: Chapter 20: Life on Other Worlds. Life in the Universe. Earliest Fossils. Laboratory Experiments.
Chapter 20: Life on Other Worlds Searching for Life: What does life look like here? How did Earth get life? Is Earth ordinary or extraordinary? If Earth is ordinary, where is everyone else? Life in the
More informationSex in Space: Astronomy 330 TR Astronomy Building. Outline. The Planet Eris? What is a planet?
Sex in Space: Astronomy 330 TR 1100-1120 134 Astronomy Building Leslie Looney Phone: 244-3615 Email: lwl1@1uiuc1.1edu Office: Astro Building #218 Office Hours: W: 11:00 a.m. noon or by appointment This
More informationCopyright 2009 Pearson Education, Inc. Life in the Universe
Life in the Universe Life in the Universe The only place we know life exists is here on Earth One of humanity s Big Questions is whether it exists elsewhere We can get some clues by considering life s
More information-- Lewis Carroll, Alice in Wonderland
Where Are They? There s no use trying, she said: one can t believe impossible things. I daresay you haven t had much practice, said the Queen. When I was your age, I always did it for half-anhour a day.
More informationAstronomy 330 HW 2. Outline. Presentations. ! Kira Bonk ascension.html
Astronomy 330 This class (Lecture 11): What is f p? Eric Gobst Suharsh Sivakumar Next Class: Life in the Solar System HW 2 Kira Bonk http://www.ufodigest.com/news/0308/ ascension.html Matthew Tenpas http://morphman.hubpages.com/hub/alien-
More informationThe Search for Extra-terrestrial. Is there anybody out there?
The Search for Extra-terrestrial Intelligence! Is there anybody out there? Summary: we will investigate (a) the Drake Equation and (b) the factors that determine how many, if any, other civilizations
More informationLife on Other Worlds: The Drake Equation Author: Meagan Morscher GK-12 Reach for the Stars Fellow, Northwestern University
Life on Other Worlds: The Drake Equation Author: Meagan Morscher GK-12 Reach for the Stars Fellow, Northwestern University Time 2-3 class periods (will vary depending on grade level and experience with
More informationIntelligent Life in the Universe
Intelligent Life in the Universe Lecture 33 APoD: Easter Island Eclipse In-Class Question 1) Do you think life exists elsewhere in the Universe? a) Yes b) No c) Don t know d) Don t care 2 33-1 Lecture
More informationGuesstimation: The Art of Getting About the Right Answer
Utah State University DigitalCommons@USU Presentations Materials Physics 10-7-2014 Guesstimation: The Art of Getting About the Right Answer JR Dennison Utah State Univesity Follow this and additional works
More informationAstrobiology: The Semester in Review
A Universe of Life Astrobiology: The Semester in Review Honors 228 with Dr. Harold Geller Searching for life everywhere Planets, stars, galaxies, Big Bang Conception of size and distance Stars and the
More informationhttp://www.youtube.com/watch?v=lhtsfozun Lo Explanation: Comet Lovejoy was captured last week passing well in front of spiral galaxy M63. Discovered only three months ago and currently near its maximum
More informationLecture Outlines. Chapter 28. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 28 Astronomy Today 8th Edition Chaisson/McMillan Chapter 28 Life in the Universe Units of Chapter 28 28.1 Cosmic Evolution Discovery 28-1 The Virus 28.2 Life in the Solar System
More informationA Recipe for Life on Earth... and elsewhere?
A Recipe for Life on Earth... and elsewhere? We know that life evolved on Earth. But did it also form on other planets, either in our Solar System or elsewhere? At the moment, we just don't know. But we
More informationQuestions for Dr. Harold Geller
Questions for Dr. Harold Geller Questions from Ms. Bullock Would you be able to give a brief introduction about yourself, and what has led you to your career and research. I am Dr. Harold A. Geller. I
More informationThe Search for Extraterrestrial Intelligence (SETI)
The Search for Extraterrestrial Intelligence (SETI) Our goals for learning What is the Drake equation? How many habitable planets have life? How many civilizations are out there? How does SETI work? Can
More informationASTRONOMY 202 Spring 2007: Solar System Exploration. Instructor: Dr. David Alexander Web-site:
ASTRONOMY 202 Spring 2007: Solar System Exploration Instructor: Dr. David Alexander Web-site: www.ruf.rice.edu/~dalex/astr202_s07 Class 37: Life in the Universe [4/18/07] Announcements Habitability of
More informationThe Search for Extraterrestrial Intelligence
The Search for Extraterrestrial Intelligence Methods for searching for life Direct searches for microbial life in the solar system rovers, sample return missions to Mars, Europa, etc. Indirect searches
More informationWHERE ARE THEY? The Fermi Paradox
WHERE ARE THEY? The Fermi Paradox Milan S. Dimitrijević Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia ENRICO FERMI FERMI PARADOX Or GREAT SILENCE (Brin 1983) Or ASTROSOCIOLOGICAL PARADOX
More informationPart I---Introduction: planets, and habitable planets
Part I---Introduction: planets, and habitable planets star--about 10 11 in our galaxy. Average separation is a few light years. (Compare with size of Galaxy: about 100,000 light years) planet--indirect
More informationAstronomy December, 2016 Introduction to Astronomy: The Solar System. Final exam. Practice questions for Unit V. Name (written legibly):
Astronomy 101 12 December, 2016 Introduction to Astronomy: The Solar System Final exam Practice questions for Unit V Name (written legibly): Honor Pledge: On my honor, I have neither given nor received
More informationFermi Paradox: a simulation solution
Fermi Paradox: a simulation solution YU HAIHAN, MARK Introduction The paradox was proposed by Fermi in 1950 during a lunch with Edward Teller, Hilbert York and Emil Konopinski. When they were talking about
More informationSimon P. Balm Astro 5 Test #3 Sample Questions
Simon P. Balm Astro 5 Test #3 Sample Questions 1. What do we mean by the general habitability of a planet? A. the suitability for Life on it surface B. the suitability for Life beneath its surface C. its
More informationIn-Class Question 1) Do you think that there are planets outside the solar which would be habitable for human life?
The Habitability of Worlds Lecture 31 NASA: The Visible Earth In-Class Question 1) Do you think that there are planets outside the solar which would be habitable for human life? a) 1 (yes, definitely)
More informationWhere are they (E.T.I.) anyway?
Welcome to Class 1: Drake EquaCon, SETI & Fermi Paradox Is it crazy to search for intelligent life? Where are they (E.T.I.) anyway? What would you like to spend most of our last class on? 1. Early SETI,
More informationPhysics can only take us so far!
Physics can only take us so far! The usual approach of science of constructing a mathematical model cannot answer the questions of why there should be a universe for the model to describe. Why does the
More informationUltimate Events. Galaxy clustering in ever deeper surveys. Models of universe and its fates
ASTR 1040 Accel Astro: Stars & Galaxies Ultimate Events Prof. Juri Toomre TA: Nicholas Nelson Lecture 30 Thur 28 Apr 2011 zeus.colorado.edu/astr1040-toomre toomre Allen Telescope Array Review current big
More informationLecture #26: Searching for Other Civilizations. SETI = Search for Extra-Terrestrial Intelligence Searching for signals from other beings
Lecture #26: Searching for Other Civilizations SETI = Search for Extra-Terrestrial Intelligence Searching for signals from other beings Searching for Other Civilizations Searching for signals from other
More informationYoung Solar-like Systems
Young Solar-like Systems FIG.2. Panels(a),(b),and(c)show 2.9,1.3,and 0.87 mm ALMA continuum images of other panels, as well as an inset with an enlarged view of the inner 300 mas centered on the (f) show
More informationWhat is a black hole s event horizon? What is a black hole s Schwarzschild radius? What is a black hole s singularity? How do they change with mass?
What is a black hole s event horizon? What is a black hole s Schwarzschild radius? What is a black hole s singularity? How do they change with mass? A probe/human falls into a black hole. Describe what
More informationGALACTIC CIVILIZATIONS
GALACTIC CIVILIZATIONS Prof. Dr. Hugo de Garis profhugodegaris@yahoo.com http://profhugodegaris.wordpress.com Abstract This essay considers it unlikely that there will be a single galactic civilization
More informationNov 17, 2003 Astronomy 100 Fall _tips_ html
Next week is Thanksgiving break Leonid meteor shower can be seen the night of the 18 th (really the early morning of the 19 th ). Should see dozens of meteors per hour at the peak 1:30 am CST. The shower
More informationAstronomy 330 HW 2. Presentations. Outline. ! Nicholas Langhammer esp_sociopol_washingtondc01.
Astronomy 330 This class (Lecture 13): What is n p? Anna Dorn Praneet Sahgal HW 2 Nicholas Langhammer http://www.bibliotecapleyades.net/sociopolitica/ esp_sociopol_washingtondc01.htm Next Class: Life on
More informationAstronomy 330 HW 2. Outline. Presentations. ! Alex Bara
Astronomy 330 This class (Lecture 10): Origin of the Moon Ilana Strauss Next Class: Our Planet Scott Huber Thomas Hymel HW 2! Alex Bara http://userpages.bright.net/~phobia/main.htm! Margaret Sharp http://hubpages.com/hub/proof-that-ufos-exist---
More informationHomework 13 (not graded; only some example ques!ons for the material from the last week or so of class)
Homework 13 (not graded; only some example ques!ons for the material from the last week or so of class)! This is a preview of the draft version of the quiz Started: Apr 28 at 9:27am Quiz Instruc!ons Question
More informationLife in the Universe. Key Concepts: Lecture 35: Admin. 11/21/17. All Formulae (for final):
Admin. 11/21/17 Key Concepts: Lecture 35: 1. Class website http://www.astro.ufl.edu/~jt/teaching/ast1002/ 2. Optional Discussion sections: Tue. ~11.30am (period 5), Bryant 3; Thur. ~12.30pm (end of period
More informationThe Search for Extraterrestrial Intelligence
The Search for Extraterrestrial Intelligence Methods for searching for life! Direct searches for microbial life in the solar system! rovers, sample return missions to Mars, Europa, etc.! Indirect searches
More informationStatus: Unit 1, Chapter 1
1 Status: Unit 1, Chapter 1 Measurement, Uncertainty, & Significant Figures Units, Standards and the SI System Converting Units Necessary given the U.S. system isolation.. Can be tragic: consider the 1999
More informationSociological Factors. Putting it all Together: How far away? How many stars to search?
f c = /2? Sociological Factors at least, maybe 3 intelligent species on Earth with technology for remote communication L > 75 years Longevity - how long are they detectable? leakage of VHF/UHF signals
More informationN = R *! f p! n e! f l! f i! f c! L
Leslie Looney Phone: 244-3615 Email: lwl1@1uiuc1.1edu Office: Astro Building #218 Office Hours: W: 11- noon or by appointment Sex in Space: 134 Astronomy Building This class (Lecture 3): Cosmology Next
More informationWhy is it hard to find planets?
Admin. 11/28/17 1. Class website http://www.astro.ufl.edu/~jt/teaching/ast1002/ 2. Optional Discussion sections: Tue. ~11.30am in Bryant 3; Thur. ~12.35pm, start in Pugh 170, then Bryant 3 3. Office hr:
More informationN = R * f p n e f l f i f c L
This Class (Lecture 33): Lifetime Next Class: Communication ET: Astronomy 230 Music: It s the End of the World R.E.M. HW 8 due today! Outline We need to estimate the average lifetime of all in our galaxy.
More informationAstrobiology. Joseph Spitale
Astrobiology Joseph Spitale 1 What is Astrobiology? Science that studies the origin, evolution, distribution, and future of life in the universe - Combines many sciences: Biology, Chemistry, Planetary
More informationN = R * f p n e f l f i f c L
Astronomy 230 Section 1 MWF 1400-1450 106 B6 Eng Hall This Class (Lecture 10): Nature of Life Next Class: Nucleic Acids Some Oral Presentation on Feb 16 th and 18 th! Mike Somers Chris Kramer Sarah Goldrich
More informationASTR-1020: Astronomy II Course Lecture Notes Section XII
ASTR-1020: Astronomy II Course Lecture Notes Section XII Dr. Donald G. Luttermoser East Tennessee State University Edition 4.0 Abstract These class notes are designed for use of the instructor and students
More informationChapter 24: Life in the Universe
Chapter 24 Lecture Chapter 24: Life in the Universe Life in the Universe 24.1 Life on Earth Our goals for learning: When did life arise on Earth? How did life arise on Earth? What are the necessities of
More informationAST 205. Lecture 23. December 8, 2003 SETI, Interstellar Travel and the Fermi Paradox. Assignments for week of Dec 8
AST 205. Lecture 23. December 8, 2003 SETI, Interstellar Travel and the Fermi Paradox Evaluation of the Drake Equation SETI: Search for Extraterrestrial Intelligence Good news Bad news Interstellar travel
More informationStart with known facts and reasonable guesses. More on order of magnitude Astronomy How many piano tuners are there in Boulder County?
ASTR 101 Introduction to Astronomy: Stars & Galaxies Prof. Rosalba Perna TA: Cameron Clarke http://amalfi.astrosunysb.edu/rosalba/ast101/ast101.html MAKE SURE TO GO OVER THE SYLLABUS (if you haven t already
More informationLecture #26: Plan. Cosmology: Search for Intelligent Life in the Universe. The Great Unanswered Questions (cont d)
Lecture #26: Plan Cosmology: The Great Unanswered Questions (cont d) Search for Intelligent Life in the Universe Reminders Course evaluations: CourseEvalUM.umd.edu Review session: Monday, December 11,
More informationN = R * f p n e f l f i f c L
Astronomy 230 Section 1 MWF 1400-1450 106 B6 Eng Hall This Class (Lecture 20): Evolution of the Worldview Next Class: Lifetime Presentations MWF: Arthur Jones Mark Piergies Matt Clarkin Gergana Slavova
More informationDetection of Earth-like planets
Planets and life Successful detections of extrasolar giant planets suggests that planetary systems may be fairly common could we detect Earthlike planets? is it likely that such planets would have life?
More informationFusion in first few minutes after Big Bang form lightest elements
Fusion in first few minutes after Big Bang form lightest elements Stars build the rest of the elements up to Iron (Fe) through fusion The rest of the elements beyond Iron (Fe) are produced in the dying
More informationLogistics. Test 3 will be 4/24 MRS 2 due Thursday 4/17
Stellar Evolution Logistics Test 3 will be 4/24 MRS 2 due Thursday 4/17 GTA Award The Graduate Teaching Assistant Excellence Award is an internal initiative which is intended to promote, recognize, and
More informationBig Bang, Black Holes, No Math
ASTR/PHYS 109 Dr. David Toback Lectures 13 & 14 1 Was Due for Today L14 Reading: (BBBHNM Unit 2) Pre-Lecture Reading Questions: Let us know if you were misgraded on any submissions End-of-Chapter Quizzes
More informationAstronomy 106, Fall September 2015
Today in Astronomy 106: Life, and its components The Drake equation: an accounting measure that suggests a path of inquiry into the emergence of life. Life as we know it. Definition of Life: how might
More informationThe Drake Equation. L, average lifetime of civilizations T, age of Galaxy (10 10 years) L/T gives the fraction of civilizations that currently exist.
The Drake Equation ns, total number of stars in Galaxy of the right type (6 billion) fp, fraction of these stars with planets (5%) ne, average number of planets orbiting those stars that have right size
More informationCopyright 2009 Pearson Education, Inc. Life in the Universe
Life in the Universe Life in the Universe The only place we know life exists is here on Earth One of humanity s Big Questions is whether it exists elsewhere We can get some clues by considering life s
More informationLife on Trappist-1-like Planets Impossible, Possible or Likely?
ESA NL 2017 Life on Trappist-1-like Planets Impossible, Possible or Likely? Joe Gale, Institute of Life Sciences Amri Wandel, Racach Institute of Physics The Hebrew University of Jerusalem Israel Some
More informationChapter 24 Life in the Universe. Earliest Life Forms. When did life arise on Earth? Fossils in Sedimentary Rock. Fossils in Sedimentary Rock
Chapter 24 Life in the Universe 24.1 Life on Earth Our goals for learning When did life arise on Earth? How did life arise on Earth? What are the necessities of life? When did life arise on Earth? Earliest
More informationMeasuring Distances to Galaxies. Galaxies in Motion. Hubble s Law. Galaxy Redshifts. Type Ia Supernovae. Supernovae are Good Standard Candles
Measuring Distances to Galaxies Too far for parallax! Standard Candles: Cepheid Variables (for Local Group) Type Ia Supernovae Redshifts Type Ia Supernovae These are another standard candle used to measure
More informationThe evolution of a Solar-like system. Young Solar-like Systems. Searching for Extrasolar Planets: Motivation
Young Solar-like Systems The evolution of a Solar-like system FIG.2. Panels(a),(b),and(c)show2.9,1.3,and0.87mmALMAcontinuum images of HL Tau. Panel (d) shows the 1.3 mm psf for the same FOV as the other
More informationIF A NUCLEUS IS FULL OF POSITIVELY CHARGED PROTONS, WHY DOESN T IT FLY APART?
IF A NUCLEUS IS FULL OF POSITIVELY CHARGED PROTONS, WHY DOESN T IT FLY APART? An introduction to the fundamental forces that control our world. Remembering that like charges repel each other, you may have
More informationAST 248, Lecture 23. James Lattimer. Department of Physics & Astronomy 449 ESS Bldg. Stony Brook University. November 19, 2018
AST 248, Lecture 23 James Lattimer Department of Physics & Astronomy 449 ESS Bldg. Stony Brook University November 19, 2018 The Search for Life in the Universe james.lattimer@stonybrook.edu The Drake Equation
More information29-Jul-13. Life in the Universe. Life in the Universe
Life in the Universe Life in the Universe The only place we knowlife exists is here on Earth One of humanity s Big Questions is whether it exists elsewhere We can get some clues by considering life s history
More informationAstronomy 141 Life in the Universe Professor Gaudi Homework #4 Solutions
Astronomy 141 Life in the Universe Autumn Quarter 008 Prof Gaudi Homework #4 Solutions These questions concern the concept of targets for searches for extrasolar planets specifically (a) the number of
More informationET: Astronomy 230 Section 1 MWF Astronomy Building. Outline. Presentations. Presentations. HW #2 is due on Friday First Presentations on
This Class (Lecture 8): Planet Formation Next Class: ET: Astronomy 230 Section 1 MWF 1400-1450 134 Astronomy Building Nature of Solar Systems HW #2 is due on Friday First Presentations on 19 th and 23
More informationWhat I know today about the Final
What I know today about the Final Tuesday, December 10, 8 11 am, same place Around 90 mul9ple choice ques9ons Closed book and closed note No smartphones allowed Calculators of any kind are permiced, but
More informationBig Bang, Black Holes, No Math
ASTR/PHYS 109 Dr. David Toback Lecture 33 1 Was due Today L33 Reading: (Unit 5) Pre-Lecture Reading Questions (PLRQ) Unit 5 Revision (if desired): Was due today before class End-of-Chapter Quizzes: Chapter
More informationOkay! I know this book is called Earth Science, but before you can understand how the earth works, you have to look at something much larger...
Chapter One: Page 0 Chapter One: Page 1 Okay! I know this book is called Earth Science, but before you can understand how the earth works, you have to look at something much larger... The universe is a
More informationLecture 12: Science fiction meets science..
Lecture 12: Science fiction meets science.. David Aldous October 12, 2017 Probability and X where today X = science fiction. The Fermi paradox is: The Universe is very big and very old; given there is
More informationN = R * f p n e f l f i f c L
This Class (Lecture 31): Lifetime Next Class: Brad Rockwell Sean Boyer Patrick Sawica Astronomy 230 Section 1 MWF 1400-1450 106 B1 Eng Hall Music: It s the End of the World REM Presentations on Nov 12
More informationFinal Exam. 12:30 2:30 pm, Friday, May 6th, in this room. Written Questions covering all the material from this semester.
Final Exam 12:30 2:30 pm, Friday, May 6th, in this room. Written Questions covering all the material from this semester. Dark Matter Black Holes Dark matter is noninteracting, so it has no way of losing
More informationNotes 9: Extrasolar Planets and Exo-biology
Notes 9: Extrasolar Planets and Exo-biology This is an interesting section. We have all sorts of observations and data concerning extrasolar planets (planets outside the solar system), but no evidence
More informationFusion in first few minutes after Big Bang form lightest elements
Fusion in first few minutes after Big Bang form lightest elements Stars build the rest of the elements up to Iron (Fe) through fusion The rest of the elements beyond Iron (Fe) are produced in the dying
More informationASTR 380: Life in the Universe - Astrobiology Professor Sylvain Veilleux
ASTR 380: Life in the Universe - Astrobiology Professor Sylvain Veilleux Some of Life s Fundamental Questions Are we alone? How did life develop on Earth? What are the conditions for life? Could life happen
More informationLife in the Universe: More E. Coli than E.T.
Life in the Universe: More E. Coli than E.T. Dr Euan D. Bennet University of Glasgow Euan.Bennet@glasgow.ac.uk What do aliens look like? What do aliens look like? UNLIKELY* * But not impossible! MORE LIKELY**
More informationSOLUTIONS TO PROBLEM SET # 2
ASTRONOMY 294Z: The History of the Universe Professor Barbara Ryden SOLUTIONS TO PROBLEM SET # 2 1) [20 points] With a telescope here on Earth, would we ever see Venus in a crescent phase? If so, sketch
More informationUnit 2 Lesson 2: The Study of Pre-History
Unit 2 Lesson 2: The Study of Pre-History Content Expectations 6 and 7 Explain how historians use a variety of sources to explore the past (e.g., artifacts, H1.2.1: Primary and secondary sources including
More informationCosmology Overview (so far): Cosmology Overview (so far): The Age of the Universe. The Big Bang. The Age of the Universe
Cosmology Overview (so far): The Universe: Everything Observable Universe: Everything we can The Universe has no special locations No If no, then no Cosmology Overview (so far): Oblers s Paradox: The sky
More informationAn Integrated Science Approach
An Integrated Science Approach Project Director Jeffrey F. Lockwood, Ed.D. Authors Jodi E. Asbell-Clarke Daniel W. Barstow Teon E. Edwards James L. Larsen Jeffrey F. Lockwood Christopher H. Randall Contributing
More informationPS 101: Introductory Astronomy Fall 2014
PS 101: Introductory Astronomy Fall 2014 Lecture: Lab: Tues./Thurs. 12:00 pm - 1:15 pm, S166 Tues. 4:00 pm - 5:50 pm, S166 Instructor: Dr. Jon M. Saken Office: S178 (Science Bldg.) Phone: 696-2753 E-mail:
More informationSex in Space: Astronomy 330 TR English Building. Outline. Astro 330: Sex in Space? Be Careful of Science. ! The Drake equation
Sex in Space: Astronomy 330 TR 1000-1050 160 English Building Leslie Looney Phone: 244-3615 Email: lwl1@1uiuc1.1edu Office: Astro Building #218 Office Hours: W: 11:00 a.m. noon or by appointment This class
More informationAstronomy 330. Presentations. Outline
Astronomy 330 This class (Lecture 7): Why does the Sun Shine? Presentations! The presentation schedule has been decided by random selection.! It is posted in the schedule section of the webpage.! Make
More information2 Which graph shows the solution to the following
1 In order for Josh to graph the solution to the inequality 4x 2y > 6, which of the following steps does he need to use? Select all that apply. A. Shade above the line. B. Draw the line y = 2x 3 as a solid
More informationTrue or False? Lamarck s Theory of Evolution. Jean-Baptiste Pierre Antoine de Monet, Chevalier de Lamarck
True or False? We know what it is, we ve seen the evidence, but Aim: How does evolution happen? Charles Darwin was the 1 st scientist to offer an explanation for how Evolution happens. Jean-Baptiste Pierre
More informationPHYS 414 Problem Set 3: Aliens and cycles
PHYS 414 Problem Set 3: Aliens and cycles Problem 1: Are we alone in the universe? In this problem we will see how Bayesian analysis can help us estimate model parameters even in the extreme case of a
More informationGamma Ray Bursts and CETI
THEP-93-4 Feb. 1993 astro-ph/9302008 10 Feb 1993 Gamma Ray Bursts and CETI Frank D. (Tony) Smith, Jr. Department of Physics Georgia Institute of Technology Atlanta, Georgia 30332 Abstract Gamma ray burst
More information3. Recognize that when a science investigation is replicated, very similar results are expected.
STANDARD 5.1 SCIENTIFIC PROCESSES ALL STUDENTS WILL DEVELOP PROBLEM-SOLVING, DECISION-MAKING AND INQUIRY SKILLS, REFLECTED BY FORMULATING USABLE QUESTIONS AND HYPOTHESES, PLANNING EXPERIMENTS, CONDUCTING
More informationStars. 1.1 A Modern View of the Universe. What Objects Do We Find in The Universe? 8/12/2010. Our goals for learning:
1.1 A Modern View of the Universe Our goals for learning: What is our place in the universe? How did we come to be? How can we know what the universe was like in the past? Can we see the entire universe?
More informationPhys 201A. Fall Homework 1 Due Tuesday, October 2, Show all steps clearly. Leave a line between answers to problems and questions.
Phys 201A Fall 2007 Homework 1 Due Tuesday, October 2, 2007 Name Partners Show all steps clearly. Leave a line between answers to problems and questions. Formulae for sphere: Circumference = 2πR, Area
More informationHubblecast Episode 91: What does the future hold for Hubble? Part I. Visual notes
Hubblecast Episode 91: What does the future hold for Hubble? Part I Visual notes 00:00 Hubble has given us 26 years of remarkable observations. But what comes next? Over the last two years we have asked
More information