





Study with the several resources on Docsity
Earn points by helping other students or get them with a premium plan
Prepare for your exams
Study with the several resources on Docsity
Earn points to download
Earn points by helping other students or get them with a premium plan
Community
Ask the community for help and clear up your study doubts
Discover the best universities in your country according to Docsity users
Free resources
Download our free guides on studying techniques, anxiety management strategies, and thesis advice from Docsity tutors
Material Type: Notes; Professor: Cash; Class: Elementary Astronomy; Subject: Physical Science; University: South Carolina State University; Term: Summer 2004;
Typology: Study notes
1 / 9
This page cannot be seen from the preview
Don't miss anything!
(^) In this section:In this section: (^) What do we see from Earth?What do we see from Earth? (^) How do objects in the sky move daily?How do objects in the sky move daily? (^) How do objects in the sky move yearly?How do objects in the sky move yearly? (^) How do things change at other locations?How do things change at other locations?
(^) For objects such as the Sun and stars, weFor objects such as the Sun and stars, we cannot directly perceive their distance cannot directly perceive their distance (^) Historically the sky was perceived as aHistorically the sky was perceived as a sphere with little lights on it sphere with little lights on it (^) We still use the same vocabularyWe still use the same vocabulary
(^) Horizon – the horizontal circle separatingHorizon – the horizontal circle separating the sky from the ground the sky from the ground (^) Zenith – the point straight overheadZenith – the point straight overhead (^) Meridian – line from North to southMeridian – line from North to south through zenith through zenith
(^) Just like the curved surface of the earthJust like the curved surface of the earth has a coordinate system … has a coordinate system … (^) So does the sky, 2 systems in factSo does the sky, 2 systems in fact (^) Altitude and AzimuthAltitude and Azimuth (^) Right Ascension and DeclinationRight Ascension and Declination (^) These will be studied in the planetariumThese will be studied in the planetarium
(^) Altitude – how far above the horizonAltitude – how far above the horizon (^) 0 on horizon0 on horizon (^) 90 at zenith90 at zenith (^) Azimuth – how far around horizonAzimuth – how far around horizon (^) 0 at north0 at north (^) 90 at east, 180 at south, 270 at west90 at east, 180 at south, 270 at west
(^) Project Earth’s coordinates out into spaceProject Earth’s coordinates out into space (^) EquatorEquator (^) →→ Celestial equatorCelestial equator (^) PolesPoles →→ Celestial polesCelestial poles (^) LongitudeLongitude →→Right AscensionRight Ascension (^) LatitudeLatitude →→DeclinationDeclination
(^) Depends on location, we will look at SouthDepends on location, we will look at South Carolina first (SC)Carolina first (SC) (^) Latitude ~35 NLatitude ~35 N
(^) Stars rise SEStars rise SE (^) Have low altitude atHave low altitude at the meridian the meridian (^) Set in SWSet in SW
(^) Stars rise alongStars rise along eastern horizoneastern horizon (^) Move up in at anMove up in at an angle towards theangle towards the southsouth
(^) Move down towardsMove down towards the western horizon the western horizon an angle from the an angle from the south south
(^) Some star rise is NESome star rise is NE and set in NWand set in NW (^) Others circle aroundOthers circle around the north celestialthe north celestial pole (circumpolar)pole (circumpolar)
(^) The path of stars are different in differentThe path of stars are different in different locationslocations (^) We will look atWe will look at (^) Equator – latitude 0Equator – latitude 0 (^) South Africa – latitude ~40SSouth Africa – latitude ~40S (^) Alaska – latitude ~60NAlaska – latitude ~60N (^) North Pole – latitude ~90NNorth Pole – latitude ~90N
(^) Stars move from east to west moreStars move from east to west more directly overhead directly overhead (^) (instead of arcs towards the southern horizon)(instead of arcs towards the southern horizon) (^) There are no circumpolar starsThere are no circumpolar stars (^) Celestial poles are on the horizonCelestial poles are on the horizon
(^) North celestial pole at zenith (overhead)North celestial pole at zenith (overhead) (^) Stars are all circumpolar and move aroundStars are all circumpolar and move around at constant altitudes at constant altitudes
(^) Rises in SERises in SE (^) Reaches low altitude at noonReaches low altitude at noon (^) Sets in SWSets in SW (^) Night longer than dayNight longer than day
(^) Rises in ERises in E (^) Reaches mid altitude at noonReaches mid altitude at noon (^) Sets in WSets in W (^) Day and night equalDay and night equal
(^) Rises in NERises in NE (^) Reaches high altitude at noonReaches high altitude at noon (^) Sets in NWSets in NW (^) Day longer than nightDay longer than night
(^) Rises in ERises in E (^) Reaches mid altitude at noonReaches mid altitude at noon (^) Sets in WSets in W (^) Day and night equalDay and night equal
(^) Sun always moves more overheadSun always moves more overhead
(^) My diagramMy diagram
(^) In March, ecliptic on celestial equatorIn March, ecliptic on celestial equator (^) In June, ecliptic north of celestial equatorIn June, ecliptic north of celestial equator (^) In Sep, ecliptic on celestial equatorIn Sep, ecliptic on celestial equator (^) In Dec, ecliptic south of celestial equatorIn Dec, ecliptic south of celestial equator