The Celestial SphereThe Celestial Sphere
Karen Meech Karen Meech
Institute for AstronomyInstitute for Astronomy
TOPS 2003TOPS 2003
Latitude and LongitudeLatitude and Longitude
Latitude (Latitude () meas from ) meas from equatorequator
Longitude (Longitude () point of ) point of reference – Greenwich reference – Greenwich UKUK
Units of measure:Units of measure: Deg, arcmin, arcsecDeg, arcmin, arcsec OO ‘ “ ‘ “
The Horizon SystemThe Horizon System
Altitude (h) – angle Altitude (h) – angle measured from the measured from the horizon to Zenith (Z)horizon to Zenith (Z)
Azimuth – the angle Azimuth – the angle measured from Nmeasured from NE E along horizonalong horizon
Problem as a celestial Problem as a celestial system?system?
Celestial SphereCelestial Sphere
Imaginary sphere Imaginary sphere where stars residewhere stars reside
Extension of Earth’s Extension of Earth’s equator, polesequator, poles
Celestial EquatorCelestial Equator Celestial polesCelestial poles
Zenith & NadirZenith & Nadir
Great CirclesGreat Circles
Circles covering the Circles covering the largest diameter on spherelargest diameter on sphere
NCP altitude = NCP altitude = Celestial MeridianCelestial Meridian – CM – CM
great circle through Z and great circle through Z and NCPNCP
Hour AngleHour Angle – angular – angular distance / time from CMdistance / time from CM HA = 0 on CMHA = 0 on CM ““-” indicates rising-” indicates rising ““+” indicates setting+” indicates setting
Declination & Right AscensionDeclination & Right Ascension DeclinationDeclination = Latitude = Latitude
Celestial Equator Celestial Equator = 0 = 0 Latitude, NCP elevationLatitude, NCP elevation Units: deg, arcmin, ‘’Units: deg, arcmin, ‘’
The The CelestialCelestial MeridianMeridian Great circle going through Great circle going through
zenith & NCPzenith & NCP Right AscensionRight Ascension = =
LongitudeLongitude Units: hh:mm:ssUnits: hh:mm:ss 360360oo = 24 hr (1 hr = 15 = 24 hr (1 hr = 15oo)) Where to start RA?Where to start RA?
The Ecliptic & The Ecliptic & SeasonsSeasons
ObliquityObliquity – tilt of Earth’s orbital axis (23.5 – tilt of Earth’s orbital axis (23.5oo))
EclipticEcliptic – path of the Earth around the sun – path of the Earth around the sun Apparent path of the sun & planets in the skyApparent path of the sun & planets in the sky Traces a great circle on the celestial sphereTraces a great circle on the celestial sphere Intersects at 2 points: Intersects at 2 points: and and ( (vernal & autumnal equinoxvernal & autumnal equinox))
is visible at midnight on CM in Septemberis visible at midnight on CM in September
Right Ascension Right Ascension
Starting PointStarting Point
Longitude system: Longitude system: Prime MeridianPrime Meridian
Two intersections Two intersections between CE & eclipticbetween CE & ecliptic Vernal EquinoxVernal Equinox Autumnal EquinoxAutumnal Equinox
Units of measure:Units of measure: Hours, min, secHours, min, sec Measure Eastward Measure Eastward
from from (RA = 0) (RA = 0) RA increases to ERA increases to E
Time ScalesTime Scales UT/Local – measured from noon to noon UT/Local – measured from noon to noon
(movement of sun)(movement of sun) Earth’s orbital motion Earth’s orbital motion must rotate >360 must rotate >360oo
= 360/365.25 = 0.986= 360/365.25 = 0.986oo
24 : (360+ 24 : (360+ ) = sidereal : 360 ) = sidereal : 360 Sidereal day = 23Sidereal day = 23hh 56 56mm 04 04ss
Start defined when Start defined when is on the celestial meridian is on the celestial meridian
Relation between ST and RARelation between ST and RA
HA = ST – RAHA = ST – RA ST at night = RA of ST at night = RA of
object on CMobject on CM is on the CM at is on the CM at
midnight at midnight at Observing tipObserving tip
RA = 0 on CM in SepRA = 0 on CM in Sep Advances 2 hr / moAdvances 2 hr / mo
Airmass – Coordinate Airmass – Coordinate RelationsRelations
Best observe @ HA = 0Best observe @ HA = 0 Airmass Airmass – amt of atm– amt of atm Extinction = absorption Extinction = absorption
& scattering& scattering = sec(ZD)= sec(ZD) Spherical Trig – law of Spherical Trig – law of
cosinescosines
cos(scos(s11) = cos(s) = cos(s22)cos(s)cos(s33) + sin(s) + sin(s22)sin(s)sin(s33)cos(A)cos(A11))
Effect of AirmassEffect of Airmass
= sec(z) = sin(= sec(z) = sin() sin () sin () + cos() + cos() cos() cos() cos(HA)) cos(HA)
Higher airmass = more extinctionHigher airmass = more extinction Higher airmass = more refractionHigher airmass = more refraction Higher airmass = poorer seeingHigher airmass = poorer seeing
SummarySummary
Coordinates: Coordinates: , , CM – passes thru Z CM – passes thru Z
and NCPand NCP increases to Eincreases to E Altitude of NCP = Altitude of NCP = HA = ST – HA = ST – is on CM at is on CM at Best obs at small HA Best obs at small HA
(small (small ))
The AstrolabeThe Astrolabe
2-D model of csphere2-D model of csphere Greek origins: astron Greek origins: astron
+ lambanien+ lambanien Ancient laptop!Ancient laptop!
Oldest about 900 BC Oldest about 900 BC (Hipparchus)(Hipparchus)
Middle AgesMiddle Ages Arabian astronomersArabian astronomers
Astrolabe FunctionsAstrolabe Functions
View of night skyView of night sky Position of starsPosition of stars Rise/set of sun, starsRise/set of sun, stars Altitude of objectAltitude of object Measure time of yearMeasure time of year Measure time of nightMeasure time of night
Astrolabe ExercisesAstrolabe Exercises
The Sky TonightThe Sky Tonight When an object rises When an object rises
or setsor sets Sunset for 6/20/02Sunset for 6/20/02
RA = 05:58:31RA = 05:58:31 Dec = +23:26:18Dec = +23:26:18 04:56 UT04:56 UT
Determine the time of Determine the time of yearyear
The Astrolabe The Astrolabe timepiecetimepiece