On the Celestial Sphere

Slides:



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

Chapter S1 Celestial Timekeeping and Navigation
Chapter S1 Celestial Timekeeping and Navigation
Apparent/Actual Motions Summary
Announcements Homework Set 1 is due today
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Observing Astronomy 315 Professor Lee Carkner Lecture 3.
The Earth Rotates.
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.
Latitude and Longitude
Latitude & Longitude.
Motions of the Celestial Sphere. Constellations Sky looks like a dome with the star painted on the inside. 88 constellations such as Ursa Major, Orion,
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.
Patterns in the Sky (cont)
Introduction To Astronomy Lesson 1
Introduction to Astronomy.  Observations lead to theories and laws  Laws are concise statements that summaries a large number of observations.  Theories.
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.
Lines of Latitude and Longitude
Observational Astrophysics in the visible light Shai Kaspi Technion - March 2015.
Latitude and longitude
Terrestrial Coordinates (useful for specifying locations on the surface of the Earth) Longitude - Longitude -- East/West Coordinate -- 0  at the Prime.
Latitude and Longitude Notes
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”
MAPPING!.
Latitude, Longitude, and Time September, 2011 Coordinate System A system used for determining the coordinates of a point. Coordinates = Numbers Latitude.
Celestial Sphere. Earthly Sphere Latitude measures the number of degrees north or south of the equator. –DeKalb at 41° 55’ N Longitude measures degrees.
Chapter 1 Predicting the Motions of the Stars, Sun, and Moon.
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.
1 Lines in the Sky In order to use the sky to measure time you need to measure the location of objects in the sky. We will look at two methods of measuring.
Navigation Unit 1-Planet Earth. What is Navigation?  The science of locating a position on earth.
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.
Announcements Homework Set 1 is due today Homework set 2: Chapter 2 # 46, 50, 52, 53 & 54 + Determine the number of kilometers in 1° of longitude at the.
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.
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,
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
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 Model describing the sky. (Glass bowl over the Earth) Pretend that the stars are attached to it Celestial Meridian: Line North to.
Chapter S1 Celestial Timekeeping and Navigation
Ancient astronomers believed that the stars were attached to a celestial sphere surrounding the Earth.
Latitude and Longitude
Introduction To Astronomy & Celestial Coordinates
Latitude and Longitude
Latitude and Longitude
Finding Your Way Around the Night Sky
Local and Sky Coordinates
Latitude and Longitude
Latitude and Longitude
Celestial Motions Chapter 2.
Latitude and Longitude
To Do Today: Students will be able to…
12/29/2018 The Sky.
Latitude and Longitude Notes
Latitude and Longitude
The Sky (Celestial Sphere)
Finding Locations on Earth: Latitude and Longitude
Celestial Motions Chapter 2.
On the Celestial Sphere
Latitude and Longitude
Celestial Sphere Practice Quiz
Latitude and Longitude
Reading the Celestial sphere
Presentation transcript:

On the Celestial Sphere 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” which goes from the North Pole through Greenwich England and on to the South Pole. Latitude is how far you are, in degrees, north or south of the Equator which is 0°. The North Pole is 90° North.

Right Ascension (RA) On the Celestial sphere: Right Ascension is like Longitude. The Right Ascension of an object is how far east an object is from a line that runs from celestial pole to the other through the vernal equinox. Unlike longitude Right Ascension is measured in Hours, Minutes and Seconds. 24 hours is once around.

Declination (Dec) Declination is how far an object is north or south of the celestial equator in degrees. It is just like latitude in everyway. The Equator is 0° Declination, The celestial poles are at 90° North and South Declination (or +90° and -90°) The Tropic of Cancer is a declination line along about 23°27’ North. The Tropic of Capricorn is

The Location of Celestial Objects All Celestial objects can be located: In the sky at a given time with Altitude and Azimuth But that changes due to the motion of the celestial sphere. On the Celestial Sphere with Right Ascension and Declination. The RA and Dec of almost all celestial objects stay the same. Except… The Objects in the Solar System

The Motions of the Sun, Moon and Planets Ancients noticed that the Sun, Moon, Planets (and the other objects in the solar system) move across the celestial sphere. “Planet” means wanderer in Greek. So…their Right Ascension and Declination are always changing. They move on paths that are close to, and intersect the ecliptic They also move with the Celestial Sphere

Circumpolar Stars Stars that are no more than a location’s latitude from the Celestial Pole will never set when viewed from that location. These are “circumpolar” stars. For Example from Culver City stars within 34° of the North Celestial Pole never set thus The Big Dipper a circumpolar