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CELESTIAL SPHERE

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Page 1: Celestial Sphere SK

CELESTIAL SPHERE

Page 2: Celestial Sphere SK

There are many celestial bodies on the sky…

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We can see celestial bodies (stars, planets etc.) on many

parts of the sky but…

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How to orient the position of star?

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We can spot positions on the Earth with Geographic

coordinates.

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Equator, Poles & Other Latitudes

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Prime Meridian & Other Longitudes

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We imagine the Cosmic Sky that

looks like Sphere.

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Celestial Sphere is a sphere that

extends Global sphere

to the Sky faraway.

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A person being at each position on the Earth can see half of celestial sphere.

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Horizon divides the Celestial sphere to 2 Hemispheres (Overhorizontal &

Undererhorizontal).

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Astronomers crated many systems of

coordinates for spotting position

on the sky.

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There are 4 coordinating

systems that be popular in using

!

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HORIZONTAL COORDINATE SYSTEM

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“Azimuth” & “Altitude”

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You must know about directional point.

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North point is a point on horizon that point to Geographic North Pole.

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A point on horizon that is opposite to North point is South point.

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West point is to the left and East point is to the right hand of

North point.

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Azimuth is the angular distance along horizon from north eastward to

position of object.

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360 degrees for azimuth

angle.

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Altitude is the angular distance from horizon to object, measured along a

vertical circle.

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90 degrees for altitude from

horizon.

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There are 90 degrees of altitude at

Zenith (overhead

point).

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Zenith distance is the angular distance from

zenith to object,

measured along a vertical

circle.

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Altitude + Zenith distance = 90

degrees.

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Astrolabe

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Simple astrolabe

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How to use simple astrolabe to spot the object in horizontal

coordinate .

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Simple astrolabe and direction plate

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Altitude & Azimuth measurement by hand

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Hand signs for altitude & azimuth measurement

(1 – 20 degrees)

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Altitude measurement for 35 degrees.

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Vertical circle & Meridian

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Vertical circle is a circle which pass zenith.

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Meridian is a circle which pass zenith,

north and south point.

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Problems in using Horizontal Coordinates

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Different place…Different horizon

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Different time…Different celestial

hemisphere

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So…there are other coordinate systems for

unity of spotting.

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EQUATORIAL COORDINATE

SYSTEM

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“Right Ascension” & “Declination”

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“Celestial equator” & “Celestial pole”

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“Earth’s axis of rotation”

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N“Right hand rule” & “Planet’s rotation”

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Rotation of each planets. (Earth, Uranus & Venus)

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Apparent motion of the sky is opposite way to Earth’s rotation.

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At “Equator”

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All stars rise from the east and set to the

west.

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At “Mid-North latitude”

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Some stars are circumpolar,

some stars can rise and set.

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At “North Pole”

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All stars that can be seen

are “circumpolar

stars”.

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Zenith distance of celestial equator equals “latitude of observer” and “altitude to celestial pole”.

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“Declination”

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Declination is the angular distance measured north and south of celestial

equator.

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Celestial equator has a declination of 0 degree. North celestial pole has +90

degree & South has -90 degree.

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Declination at zenith equals to Latitude at observer.

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Lowest declination that be circumpolar declination = 90 – latitude of observer

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“Ecliptic plane” & “Ecliptic line”

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Ecliptic plane is a plane of the Earth’s orbit around the Sun.

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Ecliptic line is the apparent path of the Sun on celestial sphere.

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Ecliptic line angles to Celestial equator ~23 degrees and half.

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Ecliptic line crosses Celestial equator at “Vernal Equinox” and “Autumnal

Equinox”

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“Right Ascension”

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Right ascension is the angular distance measured eastward along

celestial equator.

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Right ascension is measured in hour minute & second with 24 hours

equivalent to a full circle.

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0 hour of right ascension begins at “Vernal equinox” point lined from North to South.

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Star map in 0 hr – 12 hr in R.A.

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Stars map in 12 hr – 24(0) hr in R.A.

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Each right ascension can rise from the East and set to the West when the Earth rotates.

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So…Each right ascension can reach to highest point at meridian line.

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Position of the Sun in Equatorial Coordinate System

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The Sun changes position in equatorial coordinate system in each day during

a year .

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The Sun is on Dec. 0 at Equinox day. Vernal is on 0 hr and Autumnal is on

12 hr right ascension.

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The Sun is on +23.5 Dec. and 6hr R.A. at Summer solstice day.

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The Sun is on -23.5 Dec. and 18 hr R.A. at Summer solstice day.

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Ecliptic line on Equatorial Coordinate

system

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The Sun rises from the east point and sets to the west point at Equinox

day.

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Path of the Sun in Equinox day

observing in each latitude.

Equator

Pole

Mid latitude