Homework #1 has been posted

Slides:



Advertisements
Similar presentations
Locating Positions on Earth
Advertisements

any object in space outside of Earth's atmosphere
Apparent/Actual Motions Summary
The Earth Rotates.
The night sky? With the naked eye, we can see more than 2000 stars as well as the Milky Way. Remind students that we often use the term “constellation”
Latitude & Longitude.
Locating Positions on Earth
Latitude & Longitude.
Today’s Lecture How to find astronomical objects
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,
Motion in the Sky. Discussion How do we estimate how far away things are from us in everyday life?
LATITUDE AND LONGITUDE
ASTR211 EXPLORING THE SKY Coordinates and time Prof. John Hearnshaw.
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.
Groups of dark brown streaks have been photographed by the Mars Reconnaissance Orbiter on melting pinkish sand dunes covered with light frost. Dark sand.
Venus goes through phases. Just like our Moon, Venus can appear as full as a disk or as a thin as a crescent. Venus, frequently the brightest object in.
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. Scientists have established a coordinate system using circular lines to pinpoint any place on the Earth. The first Coordinate.
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 1.
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.
Our Place in the Cosmos and Introduction to Astrophysics Lecture 3 Patterns in the Sky - The Earth’s Rotation.
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.
Finding locations on the Earth. Latitude (parallels) imaginary lines drawn around the earth parallel to the equator definition – the distance north or.
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.
 Celestial Sphere: an imaginary sphere on which all the celestial objects would appear  Celestial object: any object in the sky that genuinely appears.
At the scale of the Milky Way Galaxy, distances are described in terms of Light-years, which is the distance light travels in one year.
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.
 Distance measure in degrees- from 0 o to 90 o North or South of the equator  Equator- primary reference point  Lines are called parallels- form complete.
GE 109 LECTURE 2 ENGR. MARVIN JAY T. SERRANO LECTURER.
Sky Motions  Diurnal Motion Annual Motion. DIURNAL MOTION o Daily East / West motion of the sky Due to the Earth’s rotation (15°/hour) [360°/24 hours.
AstroLab-2 Locating Stars in the Sky Merav Opher-Fall 2004.
Constellations pg. 65. Constellation section of the sky with a recognizable star pattern. 88 listed 48 from Ptolemy.
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.
Chapter 4: Rising & Setting Stars © BRIEF
What is apparent motion? Important to understand what we see and what is actually happening. Apparent motion is what we see from Earth Actual motion is.
Research Experiences for Undergraduates (REU)
Using the Globe.
Chapter 3 Objectives Distinguish between latitude and longitude.
Locating Positions on Earth
Navigating the Night Sky
Constellations pg. 71.
Constellation – Sky Familiarization
1.5. Describing the Position of Objects in Space
The Celestial Sphere From our perspective on Earth the stars appear embedded on a distant 2-dimensional surface – the Celestial Sphere.
November 8,2010 Celestial Motions.
Latitude and Longitude
Latitude and Longitude
HEMISPHERES, LATITUDE & LONGITUDE
Finding Your Way Around the Night Sky
Stargazing Terminology
Local and Sky Coordinates
Latitude and Longitude
Definitions Latitude – Distance north or south from the equator measured in degrees Longitude – Distance east or west of the Prime Meridian measured in.
Celestial Motions Chapter 2.
12/29/2018 The Sky.
HEMISPHERES, LATITUDE & LONGITUDE
Astronomy Picture of the Day
ASTRO UNIT 1 REVIEW.
Homework #1 has been posted
Celestial Motions Chapter 2.
Celestial Sphere Practice Quiz
LATITUDE AND LONGITUDE
What is the Relationship Between Latitude and Polaris?
Presentation transcript:

Homework #1 has been posted It is due by Friday, Jan. 28, 4 p.m. Answers can be submitted at any time

Phobos: Largest of two Martian moons, is expected to break up and crash into Mars within the next 105 years. Russian Phobos-Grunt robotic spacecraft is scheduled to launch toward Phobos later this year and return surface samples in 2014.

Understanding motions in the sky

Celestial Sphere Large imaginary spherical surface centered on the Earth. Stars and other celestial objects “fixed” on its surface. Conceptual Model, not a physical model

The North Celestial Pole (NCP) and the South Celestial Pole (SCP) are located at the intersection of the earth’s rotation axis with the celestial sphere. The Celestial Equator is the extension of the Earth’s equator onto the celestial sphere.

The celestial sphere is “fixed” in space. We view it in the context of the local sky

Cardinal directions – NSEW Zenith – point directly overhead Nadir - point directly opposite zenith Horizon – half way between zenith and nadir Meridian – line from north point on horizon, through zenith, to south point on horizon (divides sky into eastern and western halves)

Local sky positions remain fixed: horizon, zenith, cardinal locations, meridian, are always in same location. An object’s altitude is the angle between its direction and the horizon

As you move around on the Earth, the portion of the celestial sphere visible in your local sky changes.

At what location on the Earth will the North Celestial Pole appear directly overhead?

Where on Earth is the Celestial Equator directly overhead?

How much of the Celestial Sphere can you see at any given time?

Half of the sky is always visible above the horizon.

Moving north or south on the Earth (changing your latitude), leads to viewing a different portion of the celestial sphere.

The Earth rotates west to east . This causes the (fixed) celestial sphere to appear to rotate east to west The apparent motion of the stars is referred to as “diurnal motion”.

If you are located in the northern hemisphere, what is the point in the sky around which objects on the Celestial Sphere appear to rotate over the course of a day? Do they appear to rotate clockwise or counter-clockwise?

The star named “Polaris” is very near the North Celestial Pole (within one degree). It is also referred to as the “North Star”.

It is helpful to think of the local sky with the zenith towards the top

Half of the Celestial Sphere is visible in the local sky, the other half is below the horizon. Rotation of the Earth causes the portion of the celestial sphere visible in the local sky to change with time.

The apparent motion of the stars due to the Earth’s rotation is referred to as “diurnal motion”.

No matter where you are on Earth, the Celestial Equator ALWAYS intersects the East and West points on the horizon.

In general, most stars rise in the eastern half of the sky (i.e., east of the meridian) increase their altitude (angular distance from the horizon) until they cross the meridian set in the western half of the sky (i.e., west of the meridian).

Some stars, called “circumpolar stars”, are always above the horizon.

Half of the celestial sphere is always visible above the horizon. As you move around on the Earth, the portion of the celestial sphere visible in your local sky changes. Half of the celestial sphere is always visible above the horizon. Moving north or south (changing your latitude), leads to viewing a different portion of the celestial sphere.

How does the altitude of the North Celestial Pole change with the latitude of an observer?

Location: Fairbanks, AL (Figures from Nick Strobel’s “AstronomyNotes” website - www.astronomynotes.com)

Location: Seattle, WA

Location: Los Angeles

Location: Equator

IMPORTANT POINTS!! 1. The altitude of the celestial pole is equal to the latitude of the observer 2. The Celestial Equator ALWAYS intersects the East and West points on the horizon.

What is the “Meridian”? The longitude passing through Greenwich England The point directly over an observer’s head A great circle half way between the observer’s zenith and nadir An imaginary line in the sky that passes from the north point on horizon, through the zenith, to the south point on horizon

What is the “Meridian”? The longitude passing through Greenwich England The point directly over an observer’s head A great circle half way between the observer’s zenith and nadir An imaginary line in the sky that passes from the north point on horizon, through the zenith, to the south point on horizon

ConceptTest You are in Bloomington and observe a star rising directly to the east. When this star reaches its highest point above the horizon, where will it be? (a) high in the northern sky (b) high in the eastern sky (c) high in the southern sky (d) high in the western sky (e) at the zenith

ConceptTest You are in Bloomington and observe a star rising directly to the east. When this star reaches its highest point above the horizon, where will it be? (a) high in the northern sky (b) high in the eastern sky (c) high in the southern sky (d) high in the western sky (e) at the zenith

ConceptTest Where are circumpolar stars at their lowest point in the sky? In the western sky In the eastern sky In the southern sky On the meridian

ConceptTest Where are circumpolar stars at their lowest point in the sky? In the western sky In the eastern sky In the southern sky On the meridian

In Bloomington, where is the North Celestial Pole? On the Celestial Equator On the meridian at an altitude of approximately 40 degrees. Near the zenith At the north point on the horizon

In Bloomington, where is the North Celestial Pole? On the Celestial Equator On the meridian at an altitude of approximately 40 degrees. Near the zenith At the north point on the horizon

You are in Bloomington and observe a star rising directly to the east You are in Bloomington and observe a star rising directly to the east. Where does this star lie on the Celestial Sphere?

ConceptTest As you move from the Earth's equator toward the North Pole, the number of circumpolar stars: increases decreases stays the same

ConceptTest As you move from the Earth's equator toward the North Pole, the number of circumpolar stars: increases b. decreases c. stays the same