Physics 55 Friday, September 16, 2005 1.Celestial navigation, phases of planets and moons, retrograde motion 2.Will then turn to Kepler’s empirical laws.

Slides:



Advertisements
Similar presentations
Knowing the Heavens Chapter Two.
Advertisements

The Sun in the Sky And how it changes in the course of the year.
Physics 55 Monday, September 12, The celestial sphere, the ecliptic. 2.Solar versus sidereal days; synodic versus sidereal months. 3.Celestial coordinates:
Chapter S1 Celestial Timekeeping and Navigation
Chapter S1 Celestial Timekeeping and Navigation
Prof. D.C. Richardson Sections
The Earth’s Movement.
PHYS 1025 – Introductory Astronomy Lecture 2, Either Semester
A100 Oct. 13 Keeping Time READ Essay 2 – Keeping Time in the text, pp
Climate and Latitude Sun’s rays spread over large area = cooler
Prof. John Hearnshaw ASTR211: COORDINATES AND TIME Coordinates and time Sections 9 – 17.
Apparent/Actual Motions Summary
Celestial Sphere Stars seem to be on the inner surface of a sphere surrounding the Earth.
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Observing Astronomy 315 Professor Lee Carkner Lecture 3.
Prologue Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2003.
The Earth Rotates.
Astronomy 104 Lunar Phases AndEclipses January 24, 2007.
Astronomy 1010 Planetary Astronomy Fall_2014 Day-9.
August 29, 2011: 10am Class On-line Quiz #1 on d2l: Please complete before class on Friday, Sept. 2 HW 2 on line (d2l and boojum): Create a Constellation.
Earth as a Planet Earth’s position in space Shape & Size of Earth
Knowing the Heavens Chapter Two. Naked-eye astronomy had an important place in ancient civilizations Positional astronomy –the study of the positions.
The Night Sky. Diurnal (daily) motion of the stars Like the Sun, the stars generally rise in the east and set in the west. This daily motion of the.
The Celestial Sphere The 88 official constellations cover the celestial sphere. If you do not have a model of the celestial sphere to bring to class, you.
Unit 8 Study Guide Notes Earth, Moon, and Sun.
Constellations A constellation is a region of the sky.
Introduction to Astronomy.  Observations lead to theories and laws  Laws are concise statements that summaries a large number of observations.  Theories.
Groups of dark brown streaks have been photographed by the Mars Reconnaissance Orbiter on melting pinkish sand dunes covered with light frost. Dark sand.
The Sun-Earth-Moon System (Chapter 3). Student Learning Objectives Associate cycles in the sky with time Describe why Earth has seasons Determine the.
Equinoxes and Solstices When the ecliptic and celestial equator intersect, day and night are each 12 hours long: the equinox. When the Sun reaches its.
The Seasons There would be no seasons if the Earth were not tilted on it’s axis!  Nick Devereux 2006.
Astronomical Coordinates Summary
NATS From the Cosmos to Earth A model of the celestial sphere shows the patterns of the stars, the borders of the 88 official constellations, the.
Knowing The Heavens Hawaii: latitude 20 deg Washington D.C.: latitude 38 deg.
Solar Motion. Label front flap MOTIONS OF THE EARTH -DAY & NIGHT.
Earth’s Rotation and Revolution
Last time: 2.1. Patterns in The Sky: Stars and constellations, TODAY: celestial coordinates 2.2 Seasons,…Precession 2.2 (cont.) The Moon and Eclipses.
Coordinate Systems.
Chapter 1 Predicting the Motions of the Stars, Sun, and Moon.
Earth in Space. All planets REVOLVE around the sun. Revolution is the movement of one object around another. One revolution equals the time it takes to.
Astronomy The study of the moon, stars, and other objects in space Study the movements of the sun, and moon as they appear to travel across the sky Will.
Announcements Clear sky patrol has not yet started We will start using PRS units this week, make sure that you have one.
Mastering Astronomy.
Physics 55 Friday, September 16, Finish Chapters 2 and S1 2.Celestial coordinates: RA and dec.
Earth, Sun, Moon and the Seasons Topic 4 and 6 Discussion Question Review Question.
What causes the Seasons?. The Earth’s orbit Seasons do NOT arise from the distance the Earth is from the Sun but rather as a result of the Earth’s annual.
Quiz #1 Review Thursday, 15 September 2011 I list here the main topics and the main points for each topic. Study also the indicated lecture notes.
Astronomy: Apparent Motions Making sense of celestial observations.
AstroLab-2 Locating Stars in the Sky Merav Opher-Fall 2004.
Knowing the Heavens Chapter Two. Naked-eye astronomy had an important place in ancient civilizations Positional astronomy –the study of the positions.
The Sun’s Path. Summer Solstice (approximately June 20-21) North Pole: The North Pole (90 degrees north latitude) receives 24 hours of daylight, as it.
PSCI 1414 GENERAL ASTRONOMY LECTURE 6: THE REASON FOR SEASONS ALEXANDER C. SPAHN.
© 2010 Pearson Education, Inc. Chapter 2 Discovering the Universe for Yourself.
Chapter 4: Rising & Setting Stars © BRIEF
Astronomy vs. Astrology Astronomy: Astronomy: The scientific study of matter in outer space, especially the positions, dimensions, distribution, motion,
Motion in the Sky. Discussion What is a year? Discussion What is a day?
Motion of the Moon. Review Question Describe the path the Sun will take across the sky on the day of the autumnal equinox as viewed from the Earth’s equator.
Chapter S1 Celestial Timekeeping and Navigation
Did you get the Key Ideas from the Seasonal Stars Lecture Tutorial?
Ancient astronomers believed that the stars were attached to a celestial sphere surrounding the Earth.
Sun’s annual motion and the Seasons
Good Morning!!! TEST DAY.
Finding Your Way Around the Night Sky
The Seasons.
Science Vocab 2 Week 1-2.
ASTRO UNIT 1 REVIEW.
Space motion.
Earth, Moon, and Sun.
Presentation transcript:

Physics 55 Friday, September 16, Celestial navigation, phases of planets and moons, retrograde motion 2.Will then turn to Kepler’s empirical laws of motion. 3.Newton’s laws of motion, connections to conservation laws. 4.The universal law of gravitation. 5.Application of gravity to the discovery of dark matter. 6.Tides, tidal forces, and the Roche limit.

Announcements 1.Professor Ronen Plesser will teach in my place this Friday. It will be a regular lecture, I am postponing his guest lecture on string theory until later in the course. 2.New assignment available on Wednesday. 3.Important dates: –Quiz 3 on Friday, Sept 30, –Midterm exam on Friday, October 7.Note: Fall break begins the evening of Oct. 7. –Final exam on Thursday, Dec. 15, 2-5 pm.

Path of Sun in Local Sky If dec of object > 0, will rise north of east, set north of west. If dec of object = 0, will rise exactly in east, set exactly in west. If dec of object < 0, will rise south of east, set south of west. Picture on left helps to explain why summer months are warmer than winter months: Sun stays longer in the sky.

Fall Equinox Comments: 1.This Wed, September 21, Sun will have RA ~12 h, dec ~0 o. Sun’s dec will remain negative until about March Since Sun lies on celestial equator this day, path of Sun during day traces out the celestial equator in your local. 3.Until spring equinox, Sun will now rise south of due east, set south of due west. How much to the south is hard to calculate, beyond the level of this course. 4.Sun will start spending shorter amount of time in sky, hence shorter days, cooler weather. 5.Sidereal time about equal to solar time on the day of the fall equinox since spring equinox will be on your meridian at about midnight, which is place of 0 RA.

PRS Question The city of Mumbai (formerly Bombay) in India has latitude 19 o N. On how many days of the year is the Sun at zenith at midday in Mumbai? 1.Zero. 2.One. 3.Two. 4.More than two. 5.I don’t know how to solve this.

Local Sky at Equator No circumpolar stars All stars eventually visible

Local Sky Near Durham

Celestial Navigation at Night: Latitude from Star’s Meridian Crossing Vega has dec=38 o 44’. If you measure altitude at meridian crossing of 78 o 44’S, latitude = 50 o N. What does one 1 o error mean in terms of distance?

Celestial Navigation During Day: Latitude from Sun’s Meridian Crossing We measure altitude of Sun’s meridian crossing to be 70 o N on spring equinox March 21 when Sun’s dec is 0 o. So latitude is 20 o S and we are in the southern hemisphere. Generally, you need a table or computer to know Sun’s dec on any given day.

Longitude From Universal Time Clock Need to compare location of star in sky now with time when star appears in same location in sky at some other known longitude such as Greenwich, England. Difference in time in hours times 360 o /24 hr = 15 o /hr gives you your longitude in degrees from Greenwich. Use Universal Time (UT) clock which records mean solar time with noon coinciding with noon in Greenwich, England. UT also known as “Zulu time” and “universal coordinated time”. Recommended book: “Longitude” by Dava Sobel.

Celestial Navigation Problem During a boat trip, you make the following observations: 1.It is the day of the summer solstice, June The Sun is on your meridian at altitude 66½ o in the North 3.Your universal time (UT) clock reads 06:00. What is your longitude and latitude? About where are you?

Question About Seasons Most important point: most planets have nearly circular orbits (why?!) so seasons are not due to variation in distance of Earth to Sun but because of tilt of planet’s axis. See 20-min online video “A Private Universe” at Think: How do lengths of day and night, and lengths of seasons, and properties of celestial sphere depend on the tilt of the Earth’s axis? If tilt were zero degrees, would there still be seasons? If tilt were 90 degrees, describe how days, seasons, celestial sphere would differ from present day situation? What about a tilt of 113 degrees from normal to the ecliptic?

Tilt of Axis Causes Earth’s Seasons SkyGazer: select menu Explore, then submenu Seasons of the Earth. Do Astronomy Place tutorial on Seasons.

Moons, Planets Always Half Illuminated

Phases of Moon and Planets

PRS Question Which planet(s) undergoes full (fully illuminated) and new (dark) phases like our Moon? 1.Venus 2.Mars 3.Venus and Mars 4.Neither

Retrograde Motion of Planets Think: If Earth somehow orbited more slowly than Mars around Sun, would retrograde motion still occur? Would an astronaut on Mars see Earth undergoing retrograde motion against the background of stars?