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Transcript of Field Astronomy
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MODULE IIIFIELD ASTRONOMY
ByAbdul MujeebAsst ProfessorDept Civil EngineeringKVGCE
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THE CELESTIAL SPHERE
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To observe the positions
/direction and movement
of the celestial bodies, an
imaginary sphere of
infinite radius is
conceptualized having its
centre at the centre of the
earth.
The stars are studded
over the inner surface of
the sphere and the earth
is represented as a point
at the centre.
The important terms and
definitions are as follows:6
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Point of view of the observer
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(11) Latitude• It is the angular distance of any place on
the earths surface north or south of
equator and measured on the meridian of
the place.
• Marked as +, - or N or S
• Defined as angle between zenith and
celestial equator.
• It varies from zero degree to 90° N and 0°
to 90° S.30
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(12) Co-latitude• It angular distance from zenith to the pole.
• It is complement of latitude and equal to
(90-ɵ).
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(13) Longitude• It is the angle between fixed reference
meridian (prime meridian) and meridian of
the place.
• Universally adopted meridian- Greenwich.
• Varies between 0° to 180°.
• Represented as Φ° east or west of
Greenwich.
•
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(14) Altitude (α)• Altitude of celestial or heavenly bodies is
its angular distance above the horizon,
measured on the vertical circle passing
through the body.
(15) Co-altitude or zenith distance
(z)• It is angular distance of heavenly body
from zenith.
• It is complement of altitude i.e z=(90-α)35
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(16) Azimuth(A)• It is the angle between observers meridian
and vertical circle passing through that body.36
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(17) Declination (δ)• It is the angular distance from plane of
equator measured along the stars meridian
called declination circle
• Varies from 0° to 90° and marked as + or
– according to north or south.
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(18) Co-declination or Polar
distance.• It is angular distance of heavenly body
from nearer pole.
• Compliment of declination i.e p=(90°- δ)
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(19) Hour Circle.• Are great circles passing through north and
south celestial poles. Ex: Declination circle
of heavenly body39
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(20) Hour angle.• Angle between observers meridian ad
declination circle passing through the
body.
(21) Right Ascension (R.A)• It is equatorial angular distance measured
eastward from the first point of aries to
hour circle passing through heavenly body.
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(22) Equinoctial points• The points of intersection of the ecliptic with
the equator are known as equinoctial points.
Declination os sun is zero at this point
• Vernal Equinox or First point of Aries is the
point in which sun’s declination changes
from south to north. Marks arrival of spring.
• Autumnal Equinox or first point of Libra is
point in which sun’s declination changes
from north to south, marks arrival of autumn.
They are six months apart in time. 41
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(23) Ecliptic• The great circle along which the sun
appears to move round the earth in a year
is called the ecliptic.
• The plane of ecliptic is inclined to plane of
equator at angle about 23° 27ꞌ.
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(24) Solastices• Are the points at which
north and south
declination of the sun is
maximum.• Point at which north
declination is maximum
- summer solastice
• Point at which south
declination is maximum
- winter solastice. 44
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THE CELESTIAL CO-ORDINATE
SYSTEM
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• The position of heavenly body can be
specified by 2 spherical co-ordinates, i.e by
two angular distance measured along arcs
of two great circles which cut each other at
right angles.
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• In practical astronomy celestial body can
be specified by following system of
co-ordinates.
1. Horizon system
2. Independent equatorial system
3. Dependent equatorial system
4. The celestial latitude and longitude system
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1. Horizon system (Altitude and Azimuth
system)
• Dependent on position of observer
• Horizon is plane of reference & co-
ordinates of heavenly body are azimuth and
altitude
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• M is the heavenly body in eastern part of
Celestial sphere, Z-zenith & P- celestial pole
• Pass a vertical circle through M to intersect
Mꞌ.
• First co-ordinate of M is azimuth- angle
between observers meridian and vertical circle.
•
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• It can be either angular distance along
horizon measured from meridian to foot of
vertical circle.
• It is also equal to zenith distance between
meridian and vertical circle through M.
• Another co-ordinate of M is altitude (α)-
angular distance above horizon on vertical
through the body.
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2. Independent Equatorial system (The
declination and Right Ascension system)
• Independent on position of observer.
• Great circle of references are equatorial
circle and declination circle.
• First co-ordinate of body is right ascension-
angular distance along equator from first
point of aries towards east to declination
circle passing through the body.
• It is also angle measured at eastward
celestial pole hour circle through RA and
declination circle through M.
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• RA is measured in direction to opposite to
motion of heavenly body, measured in
degrees, minutes and seconds on in terms of
time.
• Another co-ordinate system is declination- it
is angular distance of body from equator
measured along arc of declination circle.
• Declination is positive if body is north and
negative if body is south of equator.
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3. Dependent Equatorial system (The
declination and Hour angle system)
• One co-ordinate is independent and other
co-ordinate is dependent on position of
observer.
• Great circle of references are horizon and
declination circle.
• First co-ordinate of M is hour angle-
angular distance along arc of horizon
measured from observers meridian to
declination circle. 55
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• It is also measured as angle subtended at
pole between observers meridian and
declination circle.
• Hour angle is measured from south towards
east up to declination circle. Varies from 0°
to 360°.
• Other co-ordinate is declination.
• In Fig SMꞌ is hour angle M1M is
declination.
• Mꞌ and M1 are projections of M on horizon
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4. Celestial latitude and longitude system
• Prime plane of reference- ecliptic and
secondary plane- great circle passing through
first point of aries and perpendicular to plane
of ecliptic.
• Two co-ordinates are (i) Celestial latitude
(ii) Celestial longitude
• Celestial latitude is arc of great circle
perpendicular to ecliptic. May be +ve or –ve
• Celestial longitude is arc of ecliptic
intercepted between great circle first point of
aries and celestial latitude
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• It is measured eastwards from 0° to 360°.
• M1M is celestial latitude and M1 is celestial
longitude for heavenly body
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Comparison of systems.
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Horizon system Independent
Equatorial
system
Dependent
Equatorial
system
Celestial latitude
and longitude
system
Coordinate
dependency
Depends on
position of
observer
Both coordinates
does not depends
on position of
observer
One coordinate
depends and
another does
not depends on
position of
observer
Does not depends
on position of
observer
Reference
plane
Altitude and
azimuth
Declination and
right ascension
Declination and
hour angle
Celestial latitude
and longitude
Great circle Horizon Equatorial circle
and declination
circle.
Horizon and
declination
circle.
Ecliptic and great
circle passing
through first point
of aries
Example:
Position of
star
Altitude-45º
Azimuth-140º
Declination-70º
Right ascension-
4h
Declination- 70º
Hour angle-50º
Celestial lat-40º
Celestial long-170º
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Example for Horizon system
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Example for latitude and longitude system
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Example for Independent Equatorial system
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Spherical trigonometry and spherical
triangle
• It is triangle which is formed upon surface
of the sphere by intersection of three arcs of
great circle.
• Angles formed by arcs at vertices of
triangle- spherical angles
• In Fig AB, BC and CA are 3 angles of great
circles and intersect each other at A, B & C.
• Angles at A, B, C are denoted by sides
opposite to them (a, b & c) 74
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• The sides of spherical triangle are
proportional to the angle subtended by them
at centre of sphere and are expressed in
angular measure.
• Sine b means sine of angle subtended at
centre of arc AC.
• A spherical angle is angle between 2 great
circles and is defined by plane angle between
tangents to their circles at point of
intersection.
• Angle A is angle between A1AA2 between
tangents AA1 and AA2
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Formulae in spherical trigonometry
For computation purpose
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Napier’s rule
• Relationship of right angled triangle are
obtained from Napier’s rule.
• In Fig ABC is spherical right angled triangle.
• Napier defines circular part as follows.
• These parts arranged around circle in order as
they are in triangle
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• Starting with side a, orders are b,90°-A,
90°-c, 90°-B.
• If any part is considered as ‘middle part’,
adjacent 2 parts are ‘adjacent parts’ and
remaining 2 sides are ‘opposite parts’.
• From Napier rule
sine of middle part=product of tangents of
adjacent parts
sine of middle part= product of cosines of
opposite parts
sin b= tan a tan (90°-A)
sin b= (cos 90°-A) cos (90°-c)82
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Astronomical Triangle
• Astronomical triangle is obtained by joining
pole, zenith and any star M on the sphere by
arcs of great circle.
• From this triangle, relation existing amongst
spherical co-ordinates may be obtained.
Let
α-altitude of celestial body (M)
δ-declination of celestial body (M)
ɵ- latitude of observer83
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ZP= co-latitude of observer
PM= co-declination or polar distance of
M=(90-δ)=p
ZM= zenith distance = co-altitude of body=
(90- α)=z
The angle at Z=MZP= The azimuth(A) of body
The angle at P=ZPM=The hour angle(H)of body
The angle at M=ZMP= parallactic angle
If three sides MZ, ZP and PM are known angle
A and H can be computed from formulae of
spherical trignometry85
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Important Questions
1. Introduction and purpose of field
astronomy
2. Definitions
3. The Celestial co-ordinate system
4. Comparison of system
5. Spherical triangle and properties
6. Napier's rule
7. Astronomical triangle
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THANK YOU