Schedule of public programs on last page!

Similar documents
Aim: What causes Seasons?

The Observer. Schedule of public programs on last page!

PHYS 155 Introductory Astronomy

Earth s Motions. Rotation -!! Period of Rotation - amount of time to make one complete rotation Example: Earth rotates in hours.

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.

Seasons ASTR 101 2/12/2018

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016

Name Class Date. Chapter 23 Touring Our Solar System Investigation 23

PHYS 160 Astronomy Test #1 Fall 2017 Version B

Reasons for the seasons - Rebecca Kaplan

EXAM #2. ANSWERS ASTR , Spring 2008

KEPLER S LAWS OF PLANETARY MOTION

Intro to Astronomy. Looking at Our Space Neighborhood

1. The bar graph below shows one planetary characteristic, identified as X, plotted for the planets of our solar system.

5 - Seasons. Figure 1 shows two pictures of the Sun taken six months apart with the same camera, at the same time of the day, from the same location.

Unit 6 Lesson 1 How Do the Sun, Earth, and Moon Interact? Copyright Houghton Mifflin Harcourt Publishing Company

Additional Exercises for Chapter 4

Planetary Orbits: Kepler s Laws 1/18/07

PTYS/ASTR 206 Section 2 Spring 2007 Homework #1 (Page 1/4)

Grade 6 Standard 2 Unit Test Astronomy

Directed Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past?

Early history of astronomy. Early history of astronomy. Positions in the sky. Lecture 3: The Sun & Constellations

6 The Orbit of Mercury

Astronomy Section 2 Solar System Test

Learning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ?

Chapter. Origin of Modern Astronomy

Earth Science Unit 6: Astronomy Period: Date: Elliptical Orbits

THE SEASONS PART I: THE EARTH S ORBIT & THE SEASONS

a. exactly 360 b. less than 360 c. more than 360 On Figure 1, draw the Earth the next day and justify your answer above.

Earth Science Lesson Plan Quarter 4, Week 5, Day 1

,.~ Readlng ~ What,~,~~ is a geocentric system? Chapter3 J 73

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

4. What verb is used to describe Earth s

January 2009 Videmus Stellae

Jan. 12th SMAS Meeting PSTCC, Main Campus Hardin Valley Road 7:30 pm, Alexander Bldg, Room 223

Astronomical Events 2019 (edited somewhat) from:

Astronomy 291. Professor Bradley M. Peterson

Astronomy 100 Section 2 MWF Greg Hall. Outline. Total Lunar Eclipse Time Lapse. Homework #1 is due Friday, 11:50 a.m.!!!!!

Astronomy 102/104: Our Solar System MWF 11:15-12:05P, Uris Auditorium Spring 2008 Course Syllabus

June 2016 E-Newsletter of the Sonoma County Astronomical Society

Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1

Astronomy Studio Exercise Geocentric and Heliocentric World Views Guy Worthey

Summer solstice June 21, 2014

Eclipses and Forces. Jan 21, ) Review 2) Eclipses 3) Kepler s Laws 4) Newton s Laws

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

Paper Reference. Paper Reference(s) 1627/01 Edexcel GCSE Astronomy Paper 01. Friday 15 May 2009 Morning Time: 2 hours

The Earth, Moon, and Sky. Lecture 5 1/31/2017

Ch. 22 Origin of Modern Astronomy Pretest

Motion in the Heavens

Contents: -Information/Research Packet. - Jumbled Image packet. - Comic book cover page. -Comic book pages. -Example finished comic

The Revolution of the Moons of Jupiter

Saturn and Planetary Rings 4/5/07

The Sun. - this is the visible surface of the Sun. The gases here are very still hot, but much cooler than inside about 6,000 C.

Early Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle

Astronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric

1 The Solar System. 1.1 a journey into our galaxy

1st Grade. Slide 1 / 90. Slide 2 / 90. Slide 3 / 90. The Sun, Moon, Earth and Stars. Table of Contents The Sun.

Copernican Revolution. ~1500 to ~1700

Earth & Beyond Teacher Newsletter

Eclipses September 12th, 2013

Lecture 4: Kepler and Galileo. Astronomy 111 Wednesday September 6, 2017

C) D) 2. The model below shows the apparent path of the Sun as seen by an observer in New York State on the first day of one of the four seasons.

ASTR 4 Solar System Astronom y

Earth Science, 13e Tarbuck & Lutgens

Key #

Introduction To Modern Astronomy II

18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton.

Orbital Mechanics. CTLA Earth & Environmental Science

Lecture 13. Gravity in the Solar System

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler

Earth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy

Cycles. 1. Explain what the picture to the left shows. 2. Explain what the picture to the right shows. 3. Explain what the picture to the left shows.

Lecture 2 Motions in the Sky September 10, 2018

Midpoints between the Planets and the Gravitational Force at these Midpoints

How can we describe the motion of the sun in the sky? Where is the Sun at noon today? What about the path of the Sun?

12.1. The Night Sky. Earth s Motions

Estimation of the Earth s Unperturbed Perihelion from Times of Solstices and Equinoxes

AS 101: The Solar System (Spring 2017) Course Syllabus

Chapter 14 Satellite Motion

function get_style23731 () { return "none"; } function end23731_ () { document.getelementbyid('elastomer23731').style.display = get_style23731(); }

Simulating the Solar System

Lab 6: The Planets and Kepler

October 19, NOTES Solar System Data Table.notebook. Which page in the ESRT???? million km million. average.

[04] Seasons, Phases, and Eclipses (9/7/17)

Exploring more with seasons Name: Block

DeAnza College Winter First Midterm Exam MAKE ALL MARKS DARK AND COMPLETE.

The Celestial Sphere. GEK1506 Heavenly Mathematics: Cultural Astronomy

What Is the Relationship Between Earth s Tilt and the Seasons?

Name and Student ID Section Day/Time:

Chapter 02 The Rise of Astronomy

Today in Space News: Earth s oldest rock found on the Moon.

Chapter 22 Exam Study Guide

Schedule of public programs on last page!

GRADE 8: Earth and space 1. UNIT 8E.1 8 hours. The Solar System. Resources. About this unit. Previous learning. Expectations

Venus Project Book, the Galileo Project, GEAR

You should have finished reading Chapter 3, and started on chapter 4 for next week.

Astr 1050 Mon. Jan. 31, 2017

SCI-4 Pinchbeck_Seccia_SOLReview_Science4_Quiz4 Exam not valid for Paper Pencil Test Sessions

2. See FIGURE B. In the Renaissance times, he proposed this model of the solar system (name this person).

The Sun s center is much hotter than the surface. The Sun looks large and bright in the sky. Other stars look much smaller.

Transcription:

The Observer February 2016 (#39) Schedule of public programs on last page! CELEBRATE PERIHELION DAY! There are many holidays that people celebrate around the end of December and the beginning of January. There is Christmas and New Year s Day, of course. Then there are other holidays that people like to mark, ranging from Kwanzaa to The Winter Solstice. But of course whether you celebrate any of these depends on factors such as your religion, your culture, and where you live. You might think that The Winter Solstice transcends such factors, but no. The Solstice is not the Winter Solstice in the southern hemisphere. There it is the Summer Solstice. And in tropical regions there is not Winter per se. So The Winter Solstice does not really apply broadly to everyone. Alas, is there no truly universal day that all of humankind can commemorate during The Holidays, one that transcends all differences of religion, culture, and location? Indeed there is! That day is Perihelion Day! Yes, Perihelion Day. What is Perihelion Day? Well, the Earth goes around the sun in an elliptical orbit, not a circular one. In the seventeenth century the German astronomer Johannes Kepler discovered that all orbits are elliptical. When the moon orbits the Earth, for example, the orbit is an ellipse, and the Earth is located at one focus of the ellipse (students www.jefferson.kctcs.edu/observatory

always ask what it at the other focus the answer is nothing ). What is an ellipse? And what is a focus? An ellipse is the oval shape you will get if you drive two nails into a board, tie a length of string to the two nails, and then use a pencil to pull the string tight and trace out a curve on the board. Each nail is a focus of that ellipse. The orbits of the planets are only slightly elliptical. The orbit of Mercury is shown below, at left. Mercury is represented by the grey dot on the orbit. The sun is the yellow dot at one of the two focus points of Mercury s orbit. Mercury has the most elliptical orbit of all the major planets. The orbit of Earth is shown to the right of Mercury. Earth s orbit is almost circular, barely an ellipse at all. Orbit of Mercury Orbit of Earth Diagrams from the Planetary Orbits Simulator of the University of Nebraska-Lincoln (http://astro.unl.edu/naap/pos/animations/kepler.swf) Nonetheless, the fact that Earth s orbit is elliptical means that at some times of the year it is closer to the sun than at other times. The point on the orbit at which Earth is closest to the sun is called the point of perihelion. (The point at which Earth is farthest from the sun is the point of aphelion.) And so that day on which the Earth is at the perihelion point is Perihelion Day! Because the Earth is closer to the sun then, the sun appears its largest in the sky. The effect is not very

Earth at Perihelion Earth at Aphelion The sun as seen from Earth at perihelion and aphelion (image from http://apod.nasa.gov/apod/ap090703.html)

significant, as the photos here show, but nonetheless, the sun does appear larger. Moreover, it appears larger to everyone on Earth, regardless of where they live or what is their culture! Thus Perihelion Day is a true global holiday! (As is its counterpart, Aphelion Day.) Perihelion Day always occurs in the beginning on January. Perihelion Day 2016 was January 2. On that day the Earth reached the perihelion point at 5:49 PM Eastern Standard Time, and it was 91,403,800 miles from the sun. Aphelion will occur on July 4, when Earth will be 94,512,900 miles from the sun about 3.4% more distant. Thus the sun on July 4 will appear about 3.4% smaller in diameter than it did on January 2. Next year, when people wish you a generic Happy Holidays, wish them in return a Merry Perihelion! HUNDREDS TURN OUT TO HEAR ASTRONOMERS TALK AT THE LIBRARY As mentioned in the last issue of the Observer, Civil War General Ormsby Mitchel (portrayed by Frazier History Museum teaching artists Tony Dingman) and Vatican Observatory Director Guy Consolmagno both spoke at the Louisville Free Public Library on Wednesday, December 9, at 7:00 PM. Both astronomers have been noted for their exceptional ability to communicate to the public the science of astronomy, and for this reason have been compared to Carl Sagan. Six hundred people came to the Library for the program. It was a very good night for astronomy in the Louisville region. Video of the entire program, from introductory comments to the last audience member s question, is available on Youtube click here. Photos of the program are on the following pages.

Top Library Director Jim Blanton makes introductory remarks. Bottom Consolmagno and Mitchel (Dingman) during the introductions. Photos courtesy of Lawrence Gettleman.

Mitchel (Dingman) speaks. Mitchel s talk was an edited version of a speech he gave in New York in 1847. Photo courtesy of Lawrence Gettleman.

Top The crowd of six hundred at the Library. Bottom Consolmagno takes a question from an audience member. Photos courtesy of Lawrence Gettleman.

Top Consolmagno answers a question. Bottom Consolmagno and program emcee Chris Graney (who is on the staff of Otter Creek South Harrison Observatory). Photos courtesy of Lawrence Gettleman.

Top Consolmagno and students who wanted pictures. Bottom Consolmagno and Mitchel (Dingman). Photos courtesy of Lawrence Gettleman and Chris Graney.

UNIVERSITY OF LOUISVILLE PUBLIC ASTRONOMY LECTURE SERIES As part of its mission as a Metropolitan Research University and to build on the success of the UofL Bullitt Lecture in Astronomy, members of the UofL department of Physics and Astronomy and visiting lecturers will be holding approximately one evening public lecture on astronomy per month during the next few months. The talks will last no more than one hour, and there will be a chance for questions and to talk with the speaker afterward. This is ideal for students of any age and for members of the general public. Speakers are below come and hear them! Christopher Graney (Jefferson Community & Technical College) Wed, Jan 20, 2016 at 7:30pm, Ekstrom Library, Chao Auditorium, UofL You Would Not Have Stood With Galileo: The surprising (and forgotten) strength of the science against Copernicus in Galileo's time Gerard Williger (UofL) Thu, Feb 11, 2016 at 7:30pm, in Natural Science 112, UofL Proto-Planetary Disks: Where Do Baby Solar Systems Come From? James Lauroesch (UofL) Thu, Mar 10, 2016 at 7:30pm, in Natural Science 112, UofL The Origin of the Elements

2016 Schedule South Harrison Park Observatory Programs Jan 16 7:00pm to 9:00pm Feb 13 7:00pm to 9:00pm Feb 20 7:30pm to 9:30pm March 5 7:30pm to 9:30pm March 12 8:00pm to 10:00pm April 9 8:30pm to 10:30pm April 23 9:00pm to 11:00pm May 7 9:30pm to 11:30pm May 21 11:00am to 1:00pm Daytime June 4 11:00am to 1:00pm Daytime June 18 9:30pm to 11:30pm July 9 9:30pm to 10:00pm NASA Program Enceladus, the water world of Saturn July 23 11:00am to 1:00pm Daytime Aug 6 9:00pm to 11:00pm NASA Program JUNO arrives at Jupiter Aug 20 11:00am to 1:00pm Daytime Sept 10 8:00pm to 10:00pm NASA Program OSIRIS-REX Asteroid Sample Return Sept 24 7:30pm to 9:30pm Oct 8 7:00pm to 9:00pm NASA Program International Observe the Moon Night Oct 22 7:30pm to 9:30pm Nov 5 6:30pm to 8:30pm Nov 19 6:30pm to 8:30pm All programs at South Harrison Park are open rain or shine. Daytime programs allow you to safely view the Sun using solar filters. Nighttime programs allow you to view the Moon, Stars, Planets, and more. The facility is handicapped accessible and we feature a video display system for cloudy days and/or nights. Contacts: Park Astronomer Henry Sipes Cell 270-668-2103 Harrison County Park Office 812-738-8236 Websites: http://www.harrisoncoparks.com/observatory.html http://www.jefferson.kctcs.edu/observatory/