The Sky (Celestial Sphere)

Slides:



Advertisements
Similar presentations
The Sun in the Sky And how it changes in the course of the year.
Advertisements

Geology/Physics 360 Astronomy Chapter 1: The Celestial Sphere.
Celestial Coordinates
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.
ASTR 2310 Chapter 1: Early Astronomy Celestial Sphere Coordinates Motions Time  Solar/Sidereal Time  Calendars Figures used in this presentation are.
Physics 101 Astronomy Dr. Brian Davies Office: 532 Currens Hall, Office Hours: M Tu W F 11-noon
The Earth Rotates.
The Sky From Earth. Let’s Step Outside Where are the stars? What direction are we facing?
Constellations. Celestial Sphere Our Point of View.
An Earth Day Sidereal Day: 23 hr 56 min 4 sec Motion relative to background stars Mean Solar Day: 24 hours The average time between meridian crossings.
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Motion in the Sky. Discussion How do we estimate how far away things are from us in everyday life?
Grab your text book Chapter 1 Astronomy Today 7th Edition
Goal: To understand how objects move in the night sky over any time span, and what we can discover from that. Objectives: 1)To be familiar with Basic Sky.
Patterns in the Sky (cont)
ASTR211 EXPLORING THE SKY Coordinates and time Prof. John Hearnshaw.
Lecture 3 -- Astronomical Coordinate Systems Constellation of the Day…Aquila Look at constellation maps on course home page.
The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The 88 official constellations cover the celestial sphere.
The Celestial Sphere Lab 2. Celestial sphere Geocentric model zenith - the point on the celestial sphere that is directly over our heads always 90˚ from.
Observational Astrophysics in the visible light Shai Kaspi Technion - March 2015.
Latitude and longitude
Where is it? On the Celestial Sphere. Longitude and Latitude On Earth: Longitude is how far you are, in degrees, East or West of the “Prime Meridian”
Coordinate Systems.
MAPPING!.
Celestial Sphere. Earthly Sphere Latitude measures the number of degrees north or south of the equator. –DeKalb at 41° 55’ N Longitude measures degrees.
A scientific model.  Why do we use the model of the celestial sphere when studying the night sky, even though it does not accurately represent three-dimensional.
First announcement: full moon tonight at 12:18 AM.
Announcements Clear sky patrol has not yet started We will start using PRS units this week, make sure that you have one.
Introduction to Positional Astronomy The Night Sky  Nick Devereux 2006.
Celestial Sphere Facts: It’s an imaginary sphere with earth in the center. It is useful for locating constellations and stars on a star map.
EARTH IN SPACE. A reminder about earth  The earth is almost a sphere  We locate points on the sphere with 3 coordinates – Longitude (180º W º.
Celestial Navigation Celestial Motion 1. General Organization Original “celestial sphere” model devised by the Greeks is still used –Greeks saw the Earth.
1.Stars move from east to west over the course of the night 2.Change slightly from one night to the next 3.However, their relative positions remain.
Universe Tenth Edition Chapter 2 Knowing the Heavens Roger Freedman Robert Geller William Kaufmann III.
1 Quiz Q & A Junior Navigation Chapter 5 Celestial Coordinates.
Constellations come, and climb the heavens, and go, And thou dost see them rise, Star of the Pole! and thou dost see them set, Alone,
Units of scale. Metric System Review Basic Units: Meter (m)- length Kilogram (kg)- mass Second (s)- time.
Chapter 2 Celestial Motions. Fig. 2.1 The Celestial Sphere To understand the idea of the celestial sphere first think of the earth in space. The stars.
AstroLab-2 Locating Stars in the Sky Merav Opher-Fall 2004.
Local and Sky Coordinates
MOTIONS OF SKY. Goals To identify the different parts of the celestial sphere model To understand how to express the location of objects in the sky To.
Our Location on the Earth North South EastWest North South East you are here West.
Chapter 4: Rising & Setting Stars © BRIEF
The equatorial coordinate system a system like latitude and longitude for the celestial sphere.
Motion in the Sky. Discussion What is a year? Discussion What is a day?
Lecture 3 -- Astronomical Coordinate Systems Constellation of the Day…Aquila constellations.
Phases of the Moon Lab The Celestial Sphere Model One way the celestial sphere model is used explains positions in the sky as seen from YOUR position.
The Celestial Sphere (The sphere should really be rotating, not Earth)
The Celestial Sphere Model describing the sky. (Glass bowl over the Earth) Pretend that the stars are attached to it Celestial Meridian: Line North to.
How do we locate objects in the sky? Angular separation: the angle between objects as seen from Earth (Degrees are separated into minutes (60 minutes of.
Goal: To understand the very basics of Astronomy. Objectives: 1)To understand how the night sky is set up 2)To be familiar with some useful Astronomy terms.
Ancient astronomers believed that the stars were attached to a celestial sphere surrounding the Earth.
Sun’s annual motion and the Seasons
The Night Sky…last time, The Horizon System
Rotating Earth Sunlight animations © Swinburne.
Constellation – Sky Familiarization
The HELIOCENTRIC Model
Stargazing Terminology
Horizon Coordinates A: Azimuth. The angle measured beginning at cardinal pt. north eastward along the horizon to the base of the vertical circle of the.
Celestial Motions Chapter 2.
Tilt of the Earth’s Rotational Axis
On the Celestial Sphere
ASTRO UNIT 1 REVIEW.
Celestial Motions Chapter 2.
On the Celestial Sphere
Celestial Sphere Practice Quiz
What is absolute location?
Reading the Celestial sphere
Presentation transcript:

The Sky (Celestial Sphere) Related to Latitude and Longitude

Celestial Equator and Poles Observer at North Pole, diurnal circles parallel to the celestial equator

Observer at the Equator Diurnal circles perpendicular to the celestial equator (poles at the horizon)

The Ecliptic Projection of the Earth’s orbital plane – Shown ~ July 4th

Projection on Sky of Earth’s Orbital Plane Ecliptic – 23.5 degrees from Equator

Ecliptic is a Projection of the Earth’s Orbital Plane RACE car analogy

Diurnal Motion of Sun and Ecliptic - 23.5 to + 23.5 degrees

Celestial Coordinates Right Ascension, Declination and Hour Angle Related to position on the Earth