Stellar and Planetary aberration Working Model

Size: px
Start display at page:

Download "Stellar and Planetary aberration Working Model"

Transcription

1 Stellar and Planetary aberration Working Model Bart Leplae Updated on 2-Dec-2011 (Org. 7-Apr-2011) This paper describes why we can observe stars that are actually behind the moon and provides an alternative interpretation of stellar and planetary aberration. 1

2 Introduction Bradley s discovery of Stellar aberration explains: why stars appear up to 20.5 arc seconds from their true position how this displacement can be calculated as a function of the Earth s orbital velocity Bradley assumed stellar aberration to occur near the observer, but this does not explain why we can observe stars that are actually behind the moon. An alternative explanation resolves the anomaly while maintaining the validity of the calculations 2

3 Stellar aberration true position (or geometric position) apparent position of a star Source: Wikipedia Light from location 1 will appear to be coming from location 2 for a moving telescope due to the finite speed of light, a phenomenon known as the aberration of light. Angle between apparent and true position is determined by the Earth's speed, divided by the speed of light, times the sine of the angle between the direction to the star, and the direction of the Earth's motion. 3

4 Stellar aberration Light appears to come from a location that is slightly ahead of the direction of movement of the Earth Diagram illustrating aberration of a star at the north ecliptic pole Source: Wikipedia 4

5 Stellar aberration Diagram illustrating the effect of annual aberration on the apparent position of three stars at ecliptic longitude 270 degrees, and ecliptic latitude 90, 45 and 0 degrees, respectively Star appears to be up to 20 arcseconds ahead of true position. (adding up to 40 arc seconds over the course of a year) Source: Wikipedia Stellar aberration is the same for every star in a given region, regardless of its distance to the Earth 5

6 Stellar aberration The apparent position of all stars surrounding the moon is displaced with the same amount and in the same direction (relative their true positions) BUT the Moon is NOT Subject to stellar aberration. (because the Moon is moving with the Earth in nearly the same direction and at nearly the same speed) 6

7 Paradox Apparent position = 10 arcsec separated from the moon While True position = 10 arcsec behind the moon 7

8 Paradox How can a star that is behind the moon be visible? 8

9 Watch the paradox Search Google for Video s using the keywords: moon star occultation 9

10 Anomaly True position Apparant position A star that is behind the moon cannot become visible as a result of stellar aberration that would take place near the observer Moves with speed of Earth 10

11 Explanation True position apparent position 1. Stellar aberration must be taking place, far before the light reaches the moon. static Medium Medium moves with speed of Earth Aberration due to difference in speed 2. The location where stellar aberration occurs is where a medium that has the same speed as the Earth comes is in contact with a medium having a different speed (because the formula s for stellar aberration prove to be valid and include the orbital velocity of the Earth) Moves with speed of Earth 11

12 apparent position Rotating Medium Model True position Model introduced in paper: Working model Magnetism Gravity on: Bart Leplae Medium above and below the orbit of the Earth has the same angular speed as the Earth 12

13 Rotating Medium Model Stellar aberration is no different for the other planets (but is more pronounced for the inner planets) Medium rotates around the sun with the same speed as the planets 13

14 Rotating Medium Model In reality, this is a curve as the speed is lower for the outer planets True direction apparent direction Border of Solar System 14

15 Rotating Medium Model Border of Solar System The light goes in a curve. The curve is a function of the progressive difference in orbital speed while moving through the Solar System. From the perspective of an observer on Earth, the difference between apparent and true position does not depend on this complex curve=> only the oribtal velocity of the Earth needs to be accounted for. 15

16 Rotating Medium Model The apparent direction of a star depends on the orbit and is different for every planet. Apparent direction (observed from Earth) Apparent direction (observed from Saturn) 16

17 Planetary Aberration Wikipedia: Planetary aberration is the combination of the aberration of light (due to Earth's velocity) and light-time correction (due to the object's motion and distance). Both are determined at the instant when the moving object's light reaches the moving observer on Earth. It is so called because it is usually applied to planets and other objects in the solar system whose motion and distance are accurately known. More precisely: planetary aberration depends on the relative motion between source (planet) and observer (Earth). As a specific example, if the source and observer move with the same relative transverse velocity (e.g. moon), the aberration term is zero (and only light-time correction remains). 17

18 Planetary Aberration Images of Planets don t overlap with the moon... Neither do they show a gap with the moon So the same paradox applies. (according to Bradley s model) 18

19 Planetary Aberration Planetary aberration depends on the relative motion between source (planet) and observer (Earth). Apparent direction of Uranus (as observed from Earth) = Apparent direction of any star behind Uranus (as observed from Earth) minus (vector operation) Apparent direction of the same star (as observed from Uranus) In other words: to calculate the aberration for Uranus as seen from the Earth, the curve already described by the light travelling between boundary of Solar System and Uranus needs to be substracted. 19

20 Planetary Aberration The calculation described on the previous page is elaborated in more detail on: The effect of planetary aberration examined for Jupiter occultation by the moon on 7-Dec-2004:

21 Diurnal Aberration Wikipedia: Diurnal aberration is caused by the velocity of the observer on the surface of the rotating Earth. It is therefore dependent not only on the time of the observation, but also the latitude and longitude of the observer. Its effect is much smaller than that of annual aberration, and is only 0".32 in the case of an observer at the equator, where the rotational velocity is greatest. Diurnal Aberration is a local / apparent effect (as described by Bradley) that adds upon the effect of annual Aberration which is causing a true displacement of the path followed by light coming from stars. In contrast with Stellar Aberration: Diurnal Aberration also applies to the light reflected by the moon. As a consequence: diurnal aberration will not allow an observer to see more stars that are actually behind the border of the moon since the observed star and border of the moon displace with exactly the same amount. 21

22 Michelson Morley experiment Conceptual model used by MM: Earth Sun According to Wikipedia: Light traveling along with the motion of the Earth would have a different speed than light traveling backward, as they would both be moving against the unmoving aether. Even if the aether had an overall universal flow, changes in position during the day/night cycle, or over the span of seasons, should allow the drift to be detected Conceptual model with rotating medium: Through the MM experiment, the speed of light was observed to be the same from any direction Earth Sun If the medium rotates around the sun with the same speed as the planets, the speed of light is expected to be the same when measured from any direction. 22

23 Summary Stellar Aberration does not occur near the observer Stellar Aberration occurs while light propagates through of the solar system. Diurnal Aberration is a local effect adding upon the effect of Stellar Aberration. This Model of Stellar Aberration is consistent with the outcome of the Michelson Morley experiment 23

The Michelson Morley experiment explained by means of a Higgs Field that rotates around the Solar System

The Michelson Morley experiment explained by means of a Higgs Field that rotates around the Solar System The Michelson Morley experiment explained by means of a Higgs Field that rotates around the Solar System Bart Leplae - bartleplae@hotmail.com 18-Aug-2013 This paper touches upon various topics covered

More information

Solar Cycle induced by Rotating Medium. Bart Leplae 23-Apr-2011 hotmail.com

Solar Cycle induced by Rotating Medium. Bart Leplae 23-Apr-2011 hotmail.com Solar Cycle induced by Rotating Medium Bart Leplae 23-Apr-2011 Bartleplae @ hotmail.com 1 Introduction Scientific Publication: Does a Spin Orbit Coupling Between the Sun and the Jovian Planets Govern the

More information

Solar Cycle induced through Coriolis Effect. Bart Leplae 22-May-2011 hotmail.com

Solar Cycle induced through Coriolis Effect. Bart Leplae 22-May-2011 hotmail.com Solar Cycle induced through Coriolis Effect Bart Leplae 22-May-2011 Bartleplae @ hotmail.com 1 Introduction This paper shows a correlation between the Solar Cycle and the velocity variations of the Sun

More information

Planetary Motion from an Earthly Perspective

Planetary Motion from an Earthly Perspective 1 Planetary Motion from an Earthly Perspective Stars appear fixed from night-to-night providing the familiar background of the constellations and asterisms. We see the same star patterns that were visible

More information

PHYS 160 Astronomy Test #1 Fall 2017 Version B

PHYS 160 Astronomy Test #1 Fall 2017 Version B PHYS 160 Astronomy Test #1 Fall 2017 Version B 1 I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. An object has the same weight,

More information

Lecture 5. Motions of the Planets

Lecture 5. Motions of the Planets Lecture 5 Motions of the Planets; Geometric models of the Solar System Motion of Planets Opposition, Conjunction Retrograde Motion Scientific Method and "Models" Size of the Earth Geocentric vs Heliocentric

More information

Yes, inner planets tend to be and outer planets tend to be.

Yes, inner planets tend to be and outer planets tend to be. 1. Planet Density Make some general comments about inner and outer planets density Inner Planets Density Outer Planets Density Is there a pattern or a trend in planet density? Yes, inner planets tend to

More information

TEKS Cluster: Space. identify and compare the physical characteristics of the Sun, Earth, and Moon

TEKS Cluster: Space. identify and compare the physical characteristics of the Sun, Earth, and Moon 5.8 Earth and space. The student knows that there are recognizable patterns in the natural world and among the Sun, Earth, and Moon system. 5.8(C) 5.8(D) demonstrate that Earth rotates on its axis once

More information

Chapter 8 MOONS, RINGS, AND PLUTO Small Worlds Among Giants

Chapter 8 MOONS, RINGS, AND PLUTO Small Worlds Among Giants Chapter 8 MOONS, RINGS, AND PLUTO Small Worlds Among Giants 8.1 THE RINGS AND MOONS OF SATURN Figure 65 shows the rings and moons when Titan is sufficiently close to Saturn to be included in the field.

More information

Chapter 0 2/19/2014. Lecture Outline. 0.1 The Obvious View. Charting the Heavens. 0.1 The Obvious View. 0.1 The Obvious View. Units of Chapter 0

Chapter 0 2/19/2014. Lecture Outline. 0.1 The Obvious View. Charting the Heavens. 0.1 The Obvious View. 0.1 The Obvious View. Units of Chapter 0 Lecture Outline Chapter 0 Charting the Heavens Earth is average we don t occupy any special place in the universe Universe: Totality of all space, time, matter, and energy Astronomy: Study of the universe

More information

Astronomy Test Review. 3 rd Grade

Astronomy Test Review. 3 rd Grade Astronomy Test Review 3 rd Grade Match the vocabulary word to its definition. Outer Planets The path a planet takes around the sun. Inner Planets Orbit Sun The center of our solar system. Small, rocky

More information

Uranus & Neptune: The Ice Giants. Discovery of Uranus. Bode s Law. Discovery of Neptune

Uranus & Neptune: The Ice Giants. Discovery of Uranus. Bode s Law. Discovery of Neptune Uranus & Neptune: The Ice Giants Discovery of Uranus Discovery of Uranus & Neptune Properties Density & Composition Internal Heat Source Magnetic fields Rings Uranus Rotational Axis by William Herschel

More information

Observational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws

Observational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws Observational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws Craig Lage New York University - Department of Physics craig.lage@nyu.edu February 24, 2014 1 / 21 Tycho Brahe s Equatorial

More information

Exercise 4.0 PLANETARY ORBITS AND CONFIGURATIONS

Exercise 4.0 PLANETARY ORBITS AND CONFIGURATIONS Exercise 4.0 PLANETARY ORBITS AND CONFIGURATIONS I. Introduction The planets revolve around the Sun in orbits that lie nearly in the same plane. Therefore, the planets, with the exception of Pluto, are

More information

Stellar Astronomy Sample Questions for Exam 3

Stellar Astronomy Sample Questions for Exam 3 Stellar Astronomy Sample Questions for Exam 3 Chapter 7 1. A protostar is formed by a) the rapid expansion of gas from an exploding star. b) the gravitational collapse of a rotating interstellar cloud.

More information

Dive into Saturn.

Dive into Saturn. Dive into Saturn http://www.pbs.org/wgbh/nova/space/death-dive-to-saturn.html Read Ch. 3 By next class time Do practice online quiz 01 Axis tilt changes directness of sunlight during the year. Why Does

More information

Observing the Universe for Yourself

Observing the Universe for Yourself Observing the Universe for Yourself Figure 6-20 Solar-System Formation What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as well as the Milky Way. A constellation

More information

Remember that for one of your observing projects you can go to a star party (stargazing). This is available at the Lawrence Hall of Science every 1st

Remember that for one of your observing projects you can go to a star party (stargazing). This is available at the Lawrence Hall of Science every 1st Observing Project Remember that for one of your observing projects you can go to a star party (stargazing). This is available at the Lawrence Hall of Science every 1st and 3rd Saturday of the month. For

More information

Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky

Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

Key Concepts Solar System, Movements, Shadows Recall that Earth is one of many planets in the solar system that orbit the Sun.

Key Concepts Solar System, Movements, Shadows Recall that Earth is one of many planets in the solar system that orbit the Sun. Key Concepts Solar System, Movements, Shadows 4-3.1 Recall that Earth is one of many planets in the solar system that orbit the Sun. It is essential for students to know that Earth is a planet that orbits

More information

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

Test 1 Review Chapter 1 Our place in the universe

Test 1 Review Chapter 1 Our place in the universe Test 1 Review Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the scantrons Formulas will be projected on the screen You can use

More information

Unit 12 Lesson 1 What Objects Are Part of the Solar System?

Unit 12 Lesson 1 What Objects Are Part of the Solar System? Unit 12 Lesson 1 What Objects Are Part of the Solar System? The Solar System Earth, other planets, and the moon are part of a solar system. A solar system is made up of a star and the planets and other

More information

Interactive Minds Solar System Review

Interactive Minds Solar System Review Interactive Minds Solar System Review Solar System Use the Solar System App and your class notes to complete this study guide and prepare for your upcoming Science Test! 1. Earth s solar system is in what

More information

Data for Best Viewing of the Planets July 15, 2018

Data for Best Viewing of the Planets July 15, 2018 Data for Best Viewing of the Planets 2018-2050 July 15, 2018 Traditionally, the best time to view a planet was reckoned to be when it was at opposition the time when the line from the Sun to the Earth

More information

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Chapter 2 Lecture The Cosmic Perspective Seventh Edition Discovering the Universe for Yourself Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the

More information

3. The diagram below shows the Moon at four positions in its orbit around Earth as viewed from above the North Pole.

3. The diagram below shows the Moon at four positions in its orbit around Earth as viewed from above the North Pole. 1. Which object orbits Earth in both the Earth-centered (geocentric) and Sun-centered (heliocentric) models of our solar system? (1) Polaris (3) the Sun (2) Venus (4) the Moon 2. A cycle of Moon phases

More information

Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc.

Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc. Chapter 2 Discovering the Universe for Yourself 1 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations

More information

STANDARD. S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position.

STANDARD. S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position. STANDARD S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position. S6E2 b. Explain the alignment of the earth, moon, and sun during solar and lunar eclipses. c. Relate the

More information

8.9 Observing Celestial Objects from Earth

8.9 Observing Celestial Objects from Earth 8.9 Observing Celestial Objects from Earth Celestial objects are visible from Earth both by day and by night. In the daytime you can see the Sun and, sometimes, the Moon. Looking up at the night sky on

More information

Gravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the

Gravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the Gravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the Geocentric-Heliocentric debate (Brahe s data and Kepler s analysis)

More information

Motions in the Sky. Stars Planets Sun Moon. Photos - APOD. Motions in the Sky - I. Intro to Solar System

Motions in the Sky. Stars Planets Sun Moon. Photos - APOD. Motions in the Sky - I. Intro to Solar System Motions in the Sky Stars Planets Sun Moon Photos - APOD 1 STARS: background for motion of other objects patterns - constellations zodiac: special set of constellations trace the apparent path of the Sun

More information

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley ASTR 200 : Lecture 6 Introduction to the Solar System 1 2004 Pearson Education Inc., publishing as Addison-Wesley Comparative Planetology Studying the similarities among and differences between the planets

More information

Introduction To Modern Astronomy I: Solar System

Introduction To Modern Astronomy I: Solar System ASTR 111 003 Fall 2007 Lecture 01 Aug. 27, 2007 Introduction To Modern Astronomy I: Solar System Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-15) Chap. 16: Our Sun Chap. 28: Search for

More information

Astronomy 111 Review Problems Solutions

Astronomy 111 Review Problems Solutions Astronomy 111 Review Problems Solutions Problem 1: Venus has an equatorial radius of 6052 km. Its semi-major axis is 0.72 AU. The Sun has a radius of cm. a) During a Venus transit (such as occurred June

More information

A2 Principi di Astrofisica. Coordinate Celesti

A2 Principi di Astrofisica. Coordinate Celesti A2 Principi di Astrofisica Coordinate Celesti ESO La Silla Tel. 3.6m Celestial Sphere Our lack of depth perception when we look into space creates the illusion that Earth is surrounded by a celestial sphere.

More information

Planets in the Sky ASTR 101 2/16/2018

Planets in the Sky ASTR 101 2/16/2018 Planets in the Sky ASTR 101 2/16/2018 1 Planets in the Sky 2018 paths of Jupiter among stars (2017/2018) Unlike stars which have fixed positions in the sky (celestial sphere), planets seem to move with

More information

is a revolution relative to a fixed celestial position. is the instant of transit of mean equinox relative to a fixed meridian position.

is a revolution relative to a fixed celestial position. is the instant of transit of mean equinox relative to a fixed meridian position. PERIODICITY FORMULAS: Sidereal Orbit Tropical Year Eclipse Year Anomalistic Year Sidereal Lunar Orbit Lunar Mean Daily Sidereal Motion Lunar Synodical Period Centenial General Precession Longitude (365.25636042

More information

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc.

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc. Chapter 2 Lecture The Cosmic Perspective Seventh Edition Discovering the Universe for Yourself Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the

More information

Chapter 06 Let s Make a Solar System

Chapter 06 Let s Make a Solar System like? Big picture. Chapter 06 Let s Make a Solar System How did it come to be this way? Where did it come from? Will I stop sounding like the Talking Heads? The solar system exhibits clear patterns of

More information

Introduction to Astronomy

Introduction to Astronomy Introduction to Astronomy AST0111-3 (Astronomía) Semester 2014B Prof. Thomas H. Puzia Theme Our Sky 1. Celestial Sphere 2. Diurnal Movement 3. Annual Movement 4. Lunar Movement 5. The Seasons 6. Eclipses

More information

Physics 1305 Notes: The Outer Solar System

Physics 1305 Notes: The Outer Solar System Physics 1305 Notes: The Outer Solar System Victor Andersen University of Houston vandersen@uh.edu April 5, 2004 Copyright c Victor Andersen 2004 1 The Gas Giant Planets The predominant feature of Jupiter,

More information

What is in outer space?

What is in outer space? What is in outer space? Celestial Objects are any natural objects that move through space. Star:_a huge sphere of gas in space _Nuclear fusion within stars give off enormous amounts of energy such as light

More information

4 Solar System and Time

4 Solar System and Time 4 olar ystem and Time 4.1 The Universe 4.1.1 Introduction The Universe consists of countless galaxies distributed throughout space. The bodies used in astro navigation belong to the Galaxy known as the

More information

OCCULTATIONS OF PLANETS AND BRIGHT STARS BY THE MOON January 27, 2018

OCCULTATIONS OF PLANETS AND BRIGHT STARS BY THE MOON January 27, 2018 OCCULTATIONS OF PLANETS AND BRIGHT STARS BY THE MOON January 27, 2018 The moon, as our nearest neighbor, sometimes blocks the light coming from a planet, a star, or the sun. Occultations are listed below

More information

Observing the Night Sky: Locating Objects

Observing the Night Sky: Locating Objects Observing the Night Sky: Locating Objects As I left the house this morning, there was a bright bluish light above and to the left of my neighbors house (approximately East) and a big very bright object

More information

MARS GOING RETROGRADE December 20, By Michael Erlewine

MARS GOING RETROGRADE December 20, By Michael Erlewine MARS GOING RETROGRADE December 20, 2011 By Michael Erlewine (Michael@Erlewine.net) Retrograde planets in astrology always gets the buzz going. Mercury is retrograde; that explains it, and so on. Well,

More information

How did it come to be this way? Will I stop sounding like the

How did it come to be this way? Will I stop sounding like the Chapter 06 Let s Make a Solar System How did it come to be this way? Where did it come from? Will I stop sounding like the Talking Heads? What does the solar system look like? Big picture. The solar system

More information

Position 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.

Position 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set. Position 3 None - it is always above the horizon. N E W S Agree with student 2; star B never crosses horizon plane, so it can t rise or set. Imaginary plane No; the Earth blocks the view. Star A at position

More information

UNIT 6 CELESTIAL SPHERE AND EQUINOCTIAL SYSTEM OF COORDINATES

UNIT 6 CELESTIAL SPHERE AND EQUINOCTIAL SYSTEM OF COORDINATES UNIT 6 CELESTIAL SPHERE AND EQUINOCTIAL SYSTEM OF COORDINATES Structure 6.1 Introduction Objectives 6.2 References 6.3 Apparent Annual Motion of the Sun and the Concept of the Ecliptic and the Obliquity

More information

Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are

Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are concept questions, some involve working with equations,

More information

Solar System Test Review

Solar System Test Review Solar System Test Review There are several planets in the solar system. What do all of these planets have in common? A.They all orbit the Sun. B. They are all close to the Moon. C.They are all called Earth.

More information

Physics Lab #4: Learning Starry Night, Part 3

Physics Lab #4: Learning Starry Night, Part 3 Physics 10293 Lab #4: Learning Starry Night, Part 3 Introduction In this lab, we will continue using Starry Night to explore some of the most important concepts we will cover in lecture. Continue with

More information

Astronomy 241: Foundations of Astrophysics I. The Solar System

Astronomy 241: Foundations of Astrophysics I. The Solar System Astronomy 241: Foundations of Astrophysics I. The Solar System Astronomy 241 is the first part of a year-long introduction to astrophysics. It uses basic classical mechanics and thermodynamics to analyze

More information

Name: Date: 5. The bright stars Vega, Deneb, and Altair form A) the summer triangle. B) the winter triangle. C) the Big Dipper. D) Orion, the Hunter.

Name: Date: 5. The bright stars Vega, Deneb, and Altair form A) the summer triangle. B) the winter triangle. C) the Big Dipper. D) Orion, the Hunter. Name: Date: 1. If there are about 6000 stars in the entire sky that can be seen by the unaided human eye, about how many stars would be seen at a particular instant on a given dark night from a single

More information

ES - Astronomy Part 2 Post-Test

ES - Astronomy Part 2 Post-Test ES - Astronomy Part 2 Post-Test True/False Indicate whether the statement is true or false. 1. Compared to the human eye, telescopes can collect light over longer periods of time. 2. The inner planets

More information

Class VIII Chapter 17 Stars and the Solar System Science

Class VIII Chapter 17 Stars and the Solar System Science Question 1: Which of the following is NOT a member of the solar system? (a) An asteroid (b) A satellite (c) A constellation (d) A comet (c) Constellation A constellation is not a member of the solar system.

More information

What is it like? When did it form? How did it form. The Solar System. Fall, 2005 Astronomy 110 1

What is it like? When did it form? How did it form. The Solar System. Fall, 2005 Astronomy 110 1 What is it like? When did it form? How did it form The Solar System Fall, 2005 Astronomy 110 1 Fall, 2005 Astronomy 110 2 The planets all orbit the sun in the same direction. The Sun spins in the same

More information

The Copernican Revolution

The Copernican Revolution The Copernican Revolution Nicolaus Copernicus (1473-1543) De Revolutionibus Orbium Coelestium (1543) [ On the Revolutions of the Celestial Spheres ] The Ptolemaic Cosmology: Geocentric and Geostatic The

More information

Stellar Aberration, Relative Motion, and the Lorentz Factor. Copyright 2010 Joseph A. Rybczyk

Stellar Aberration, Relative Motion, and the Lorentz Factor. Copyright 2010 Joseph A. Rybczyk Stellar Aberration, Relative Motion, and the Lorentz Factor Copyright 2010 Joseph A. Rybczyk Abstract Presented are the results of an in-depth investigative analysis conducted to determine the relationship

More information

Planets & The Origin of Science

Planets & The Origin of Science Planets & The Origin of Science Reading: Chapter 2 Required: Guided Discovery (p.44-47) Required: Astro. Toolbox 2-1 Optional: Astro. Toolbox 2-2, 2-3 Next Homework Due. Sept. 26 Office Hours: Monday,

More information

Outline. Question of Scale. Planets Dance. Homework #2 was due today at 11:50am! It s too late now.

Outline. Question of Scale. Planets Dance. Homework #2 was due today at 11:50am! It s too late now. Outline Homework #2 was due today at 11:50am! It s too late now. Planetarium observing is over. Switch Gears Solar System Introduction The Planets, the Asteroid belt, the Kupier objects, and the Oort cloud

More information

Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest).

Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest). Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest). Rotation The movement of one object as it turns or spins around a central point or axis. Revolution The movement

More information

Planetarium observing is over. Nighttime observing starts next week.

Planetarium observing is over. Nighttime observing starts next week. Homework #2 was due today at 11:50am! It s too late now. Planetarium observing is over. Solar observing is over. Nighttime observing starts next week. Outline Switch Gears Solar System Introduction The

More information

AST Section 2: Test 1

AST Section 2: Test 1 AST1002 - Section 2: Test 1 Date: 10/06/2009 Name: Equations: c = λ f, λ peak = Question 1: A star with a declination of +40.0 degrees will be 1. east of the vernal equinox. 2. west of the vernal equinox.

More information

Lecture 2 Motions in the Sky September 10, 2018

Lecture 2 Motions in the Sky September 10, 2018 1 Lecture 2 Motions in the Sky September 10, 2018 2 What is your year in school? A. New freshman B. Returning freshman C. Sophomore D. Junior E. Senior F. I ve been here, like, forever 3 What is your major?

More information

Astronomy Club of Asheville January 2016 Sky Events

Astronomy Club of Asheville January 2016 Sky Events January 2016 Sky Events The Planets this Month - page 2 Planet Highlights - page 7 All 5 Naked-Eye Planets in the Dawn Sky - page 10 Moon Phases - page 11 Earth Reaches Perihelion on Jan. 4 - page 12 Quadrantid

More information

CHAPTER 6. The Solar System

CHAPTER 6. The Solar System CHAPTER 6 The Solar System 6.1 An Inventory of the Solar System The Greeks knew about 5 planets other than Earth They also knew about two other objects that were not planets or stars: meteors and comets

More information

Uranus and Neptune. Uranus and Neptune Properties. Discovery of Uranus

Uranus and Neptune. Uranus and Neptune Properties. Discovery of Uranus Uranus and Neptune Uranus and Neptune are much smaller than Jupiter and Saturn, but still giants compared to Earth Both are worlds we know relatively little about Voyager 2 is the only spacecraft to visit

More information

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

Welcome back. Scale. Week 2 Updates. PHYS 1302 Astronomy of the Solar System

Welcome back. Scale. Week 2 Updates. PHYS 1302 Astronomy of the Solar System Week 2 Updates Two in-class quizzes now completed Introductions List-serve Quick review of Chapter 1 Discuss Chapter 2 Chapter 3 next week (9/9). Welcome back Week 2 of PHYS 1302 Como se dice The h Syllabus:

More information

Planetary Rings (cont.) Rings / Galilean Satellites 4/10/07

Planetary Rings (cont.) Rings / Galilean Satellites 4/10/07 Planetary Rings (cont.) + Galilean Satellites Announcements Reading Assignment Finish Chapter 15 5 th homework due Thursday. Reminder about term paper due April 17. A sample planet fact sheet has been

More information

ASTR 2310: Chapter 2

ASTR 2310: Chapter 2 Emergence of Modern Astronomy Early Greek Astronomy Ptolemaic Astronomy Copernican Astronomy Galileo: The First Modern Scientist Kepler's Laws of Planetary Motion Proof of the Earth's Motion Early Greek

More information

The Celestial Sphere. GEK1506 Heavenly Mathematics: Cultural Astronomy

The Celestial Sphere. GEK1506 Heavenly Mathematics: Cultural Astronomy The Celestial Sphere GEK1506 Heavenly Mathematics: Cultural Astronomy Helmer Aslaksen Department of Mathematics National University of Singapore aslaksen@math.nus.edu.sg www.math.nus.edu.sg/aslaksen/ The

More information

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS) Page1 Earth s Formation Unit [Astronomy] Student Success Sheets (SSS) HS-ESSI-1; HS-ESS1-2; HS-ESS1-3; HS-ESSI-4 NGSS Civic Memorial High School - Earth Science A Concept # What we will be learning Mandatory

More information

IB Physics - Astronomy

IB Physics - Astronomy Solar System Our Solar System has eight planets. The picture below shows their relative sizes, but NOT their relative distances. A planet orbits the sun, and has gravitationally cleared its orbital area

More information

Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 What Objects Are Part of the Solar System? Florida Benchmarks SC.5.E.5.2 Recognize the major common characteristics of all planets and compare/contrast the properties of inner and outer

More information

Lecture 2: Motions of the Earth and Moon. Astronomy 111 Wednesday August 30, 2017

Lecture 2: Motions of the Earth and Moon. Astronomy 111 Wednesday August 30, 2017 Lecture 2: Motions of the Earth and Moon Astronomy 111 Wednesday August 30, 2017 Reminders Online homework #1 due Monday at 3pm Labs start next week Motions of the Earth ASTR111 Lecture 2 Observation:

More information

astronomy A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.

astronomy A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. astronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 5. If the distance between the Earth and the Sun were

More information

One sine wave is 7.64 minutes peak to peak variation. Two sine waves is 9.86

One sine wave is 7.64 minutes peak to peak variation. Two sine waves is 9.86 WHY THE SUN IS SOMETIMES FAST AND SOMETIMES SLOW As the earth orbits the sun in an ellipse, it goes faster approaching the sun and slower when receding, just like when you throw a ball up in the air and

More information

AST111, Lecture 1b. Measurements of bodies in the solar system (overview continued) Orbital elements

AST111, Lecture 1b. Measurements of bodies in the solar system (overview continued) Orbital elements AST111, Lecture 1b Measurements of bodies in the solar system (overview continued) Orbital elements Planetary properties (continued): Measuring Mass The orbital period of a moon about a planet depends

More information

Space Science Jeopardy!

Space Science Jeopardy! Space Science Jeopardy! Structure of the Universe Stars & HR Diagram Seasons, Tides, Phases, Eclipses Astronomical Bodies The Sun & Gravity 10 10 10 10 10 20 20 20 20 20 30 30 30 30 30 40 40 40 40 40 50

More information

EEn Explain the Earth s motion through space, including precession, nutation, the barycenter, and its path about the galaxy.

EEn Explain the Earth s motion through space, including precession, nutation, the barycenter, and its path about the galaxy. EARTH IN SPACE EEn.1.1.1 Explain the Earth s motion through space, including precession, nutation, the barycenter, and its path about the galaxy. I Can Explain the origin of the Earth s motion based on

More information

Other Planetary Systems (Chapter 13) Extrasolar Planets. Is our solar system the only collection of planets in the universe?

Other Planetary Systems (Chapter 13) Extrasolar Planets. Is our solar system the only collection of planets in the universe? Other Planetary Systems (Chapter 13) Extrasolar Planets Is our solar system the only collection of planets in the universe? Based on Chapter 13 No subsequent chapters depend on the material in this lecture

More information

A Comparison of Radio and Optical Astrometric Reduction Algorithms

A Comparison of Radio and Optical Astrometric Reduction Algorithms A Comparison of Radio and Optical Astrometric Reduction Algorithms G. H. Kaplan U.S. Naval Observatory ghk@newcomb.usno.navy.mil Abstract This paper examines the correspondence between two approaches to

More information

Lecture 25: The Outer Planets

Lecture 25: The Outer Planets Lecture 25: The Outer Planets Neptune Uranus Pluto/Charon Uranus and three moons Neptune and two moons 1 The Outer Planets Uranus Discovered by William Herschel in 1781, who realized that this extended

More information

Solar vs. Lunar Tides

Solar vs. Lunar Tides 1 2 3 4 Solar vs. Lunar Tides In the force equations M is the mass of the tide-causing object, r is the separation between the two objects. dr is the size of the object on which the tides are being raised.

More information

1. The Moon appears larger when it rises than when it is high in the sky because

1. The Moon appears larger when it rises than when it is high in the sky because 2-1 Copyright 2016 All rights reserved. No reproduction or distribution without the prior written consent of 1. The Moon appears larger when it rises than when it is high in the sky because A. you are

More information

Useful Formulas and Values

Useful Formulas and Values Name Test 1 Planetary and Stellar Astronomy 2017 (Last, First) The exam has 20 multiple choice questions (3 points each) and 8 short answer questions (5 points each). This is a closed-book, closed-notes

More information

Label next 2 pages in ISN Gas Giants. Make sure the following assignments are turned in:

Label next 2 pages in ISN Gas Giants. Make sure the following assignments are turned in: Do Now: Label next 2 pages in ISN Gas Giants Make sure the following assignments are turned in: A3K Article Analysis Small Group Test Corrections Form (if applicable) Astronomical Bodies in The Solar System

More information

Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations.

Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations. Chapter 1: Discovering the Night Sky Constellations: Recognizable patterns of the brighter stars that have been derived from ancient legends. Different cultures have associated the patterns with their

More information

a. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU

a. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU 1 AST104 Sp04: WELCOME TO EXAM 1 Multiple Choice Questions: Mark the best answer choice. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1. A galaxy

More information

Science Revision Paper- Final Exam May-June Write the scientific terms for the following statements/definitions: Part A

Science Revision Paper- Final Exam May-June Write the scientific terms for the following statements/definitions: Part A Name Grade 4 Date : Science Revision Paper- Final Exam May-June 2018 Write the scientific terms for the following statements/definitions: Part A 1. An imaginary line that goes through an object s center:

More information

Guiding Questions. Discovering the Night Sky. iclicker Qustion

Guiding Questions. Discovering the Night Sky. iclicker Qustion Guiding Questions Discovering the Night Sky 1 1. What methods do scientists use to expand our understanding of the universe? 2. What makes up our solar system? 3. What are the stars? Do they last forever?

More information

Astronomy 1 Winter Lecture 15; February

Astronomy 1 Winter Lecture 15; February Astronomy 1 Winter 2011 Lecture 15; February 9 2011 Previously on Astro-1 Mercury, Venus, Mars (and Earth) Size and composition Crusts and cores Volcanism and internal activity Stargazing Events Santa

More information

Ay 1 Lecture 2. Starting the Exploration

Ay 1 Lecture 2. Starting the Exploration Ay 1 Lecture 2 Starting the Exploration 2.1 Distances and Scales Some Commonly Used Units Distance: Astronomical unit: the distance from the Earth to the Sun, 1 au = 1.496 10 13 cm ~ 1.5 10 13 cm Light

More information

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley ASTR 200 : Lecture 6 Introduction to the Solar System 1 2004 Pearson Education Inc., publishing as Addison-Wesley ANNOUNCEMENTS Keep up with reading! Always posted on course web site. Reading material

More information

The Mass of Jupiter Student Guide

The Mass of Jupiter Student Guide The Mass of Jupiter Student Guide Introduction: In this lab, you will use astronomical observations of Jupiter and its satellites to measure the mass of Jupiter. We will use the program Stellarium to simulate

More information

Astronomy 103: First Exam

Astronomy 103: First Exam Name: Astronomy 103: First Exam Stephen Lepp October 27, 2010 Each question is worth 2 points. Write your name on this exam and on the scantron. 1 Short Answer A. What is the largest of the terrestrial

More information

MS-ESS1-1 Earth's Place in the Universe

MS-ESS1-1 Earth's Place in the Universe MS-ESS1-1 Earth's Place in the Universe Students who demonstrate understanding can: MS-ESS1-1. Develop and use a model of the Earth-sun-moon system to describe the cyclic patterns of lunar phases, eclipses

More information