Presentation is loading. Please wait.

Presentation is loading. Please wait.

Chapter 4: Rising & Setting Stars www.boyce-astro.org © BRIEF 20141.

Similar presentations


Presentation on theme: "Chapter 4: Rising & Setting Stars www.boyce-astro.org © BRIEF 20141."— Presentation transcript:

1 Chapter 4: Rising & Setting Stars www.boyce-astro.org © BRIEF 20141

2 2 Rising & Setting Stars Overview: Coordinate Systems Celestial Sphere Local Sky Ecliptic Equatorial Coordinate System 3 Classes of Stars Local Sky Examples Measuring Angles

3 www.boyce-astro.org © BRIEF 20143 Rising & Setting Stars Rising & Stetting Stars: Coordinate systems Observer based – azimuth and altitude Earth based – latitude and longitude Celestial – declination and right ascension (or sidereal hour angle) All three are basically ways of describing locations on a sphere – inherently two dimensional Requires two parameters (e.g. latitude and longitude) What you see in the sky depends on Date of year Time Latitude Longitude Which is how we can use the stars to navigate!!

4 www.boyce-astro.org © BRIEF 20144 Rising & Setting Stars Celestial Sphere: Points on the Sphere North and south celestial poles Celestial equator REMEMBER: These are points /lines on the celestial sphere and NOT on the Earth

5 www.boyce-astro.org © BRIEF 20145 Rising & Setting Stars Your Local Sky: Zenith: Imaginary point directly above your head on the celestial sphere Nadir: Imaginary point directly below your feet Horizon: The apparent line that separates the earth from the sky Meridian: Imaginary great circle passing through the celestial north and south pole and the zenith Transit: When a celestial body crosses the meridian due to the Earth’s rotation

6 www.boyce-astro.org © BRIEF 20146 Rising & Setting Stars Your Local Sky: Horizontal Coordinate System Coordinates are measured with respect to horizon Change with time and depend on observer Azimuth: 0 to 360 degrees around horizon from north towards east 0° = North, 90 ° = East, 180 ° = South, 270 °= West Altitude: 0 to 90 degrees up from horizon 0 ° = Horizon, 90 ° = Zenith DEMO: http://astro.unl.edu/classaction/animations/coordsmotion/altazimuth.htmlhttp://astro.unl.edu/classaction/animations/coordsmotion/altazimuth.html

7 www.boyce-astro.org © BRIEF 20147 Rising & Setting Stars Ecliptic: Ecliptic: The Sun's apparent annual path among the constellations Plane containing the Sun and planets Ecliptic is tilted 23.5° with respect to the Equator

8 www.boyce-astro.org © BRIEF 20148 Rising & Setting Stars Ecliptic:

9 www.boyce-astro.org © BRIEF 20149 Rising & Setting Stars Ecliptic: Cardinal Points Vernal Equinox Sun rises due East and sets due West Length of day = length of night = 12 hours Summer Solstice Sun is highest in the sky Autumnal Equinox Sun rises due East and sets due West Length of day = night = 12 hours Winter Solstice Sun is lowest in the sky This is REVERSED for the Southern Hemisphere

10 www.boyce-astro.org © BRIEF 201410 Rising & Setting Stars Celestial Sphere: Tilted 23 ½ degrees We live on the side of the Earth. Sky appears tilted at an angle equal to our latitude. Stars appear to move in arcs across the sky that are not perpendicular to horizon.

11 www.boyce-astro.org © BRIEF 201411 Rising & Setting Stars Basic Motion of the Celestial Sphere (Demo with TheSky) The sky appears to rotate around NCP. Altitude of NCP from the horizon is always equal to your latitude on Earth's surface Stars move in arcs that parallel the celestial equator Star move across the sky at 15 o per hour (4 minutes per degree) Each day star positions move 1 o west (difference between Sidereal vs. Solar Time) Some stars are “circumpolar” – never set Practical Application with TheSky X

12 www.boyce-astro.org © BRIEF 201412 Rising & Setting Stars Equatorial Coordinate System: Coordinates fixed on the celestial sphere Time and observer independent (unlike Alt/Az) Declination (dec)‏: Analogous to latitude, but on the celestial sphere North-south distance between celestial equator and a location on the celestial sphere. Measured in degrees: +90 ° to 0 ° – north from celestial equator 0 ° to -90 ° – south from celestial equator Right Ascension (RA)‏: Analogous to longitude, but on the celestial sphere Measured in units of time: hours, minutes, seconds (See next slide) 0 h – 24 h from Vernal Equinox towards east Ex. Sirius has RA = 6 h 45 m OR 6:45 Don’t confuse RA with time on your watch! DEMO: http://astro.unl.edu/classaction/animations/coordsmotion/ra decdemo.html http://astro.unl.edu/classaction/animations/coordsmotion/ra decdemo.html

13 www.boyce-astro.org © BRIEF 201413

14 www.boyce-astro.org © BRIEF 201414 Rising & Setting Stars Equatorial Coordinate System: Latitude and longitude vs. Declination and Right Ascension DEMO: http://astro.unl.edu/classaction/animations/coordsmotion/radecdemo.htmlhttp://astro.unl.edu/classaction/animations/coordsmotion/radecdemo.html

15 www.boyce-astro.org © BRIEF 201415 Rising & Setting Stars RA and Dec of the Cardinal Points on the Ecliptic: Vernal Equinox Sun appears on March 21 RA = 0h Dec = 0˚ Summer Solstice Sun appears on June 21 RA = 6h Dec = 23.5˚ Autumnal Equinox Sun appears on Sept. 21 RA = 12h Dec = 0˚ Winter Solstice Sun appears on Dec. 21 RA = 18h Dec = -23.5˚

16 www.boyce-astro.org © BRIEF 201416 Rising & Setting Stars RA and Dec of the Cardinal Points on the Ecliptic: Vernal Equinox – Sun appears on March 21 – RA = 0h Dec = 0˚ Summer Solstice – Sun appears on June 21 – RA = 6h Dec = 23.5˚ Autumnal Equinox – Sun appears on Sept. 21 – RA = 12h Dec = 0˚ Winter Solstice – Sun appears on Dec. 21 – RA = 18h Dec = -23.5˚ Declination 0 h Ecliptic Equator 6 h12 h18 h24 h 23.5° -23.5°

17 www.boyce-astro.org © BRIEF 201417 Rising & Setting Stars Equatorial Coordinate System: Practical Example - Vega Declination tells us that it is 38°44′ north of the celestial equator. We can interpret its right ascension in two ways: As an angle, it means Vega is about 279° east of the vernal equinox As a time, it means Vega crosses the meridian about 18 hours 35 minutes after the spring equinox.

18 www.boyce-astro.org © BRIEF 201418 Rising & Setting Stars Constellations of the Zodiac: The constellations on the celestial sphere through which the ecliptic passes Origin of Astrology (Zodiac Sign)

19 www.boyce-astro.org © BRIEF 201419 Rising & Setting Stars Local Skies: 3 Classes of Stars Circumpolar North Always visible Never Set Rotate Around the NCP Circumpolar South Never visible for northern observers Rising and setting Stars Lie between Circumpolar North & South DEMO: http://astro.unl.edu/classaction/animations/coordsmotion/celhorcomp.htmlhttp://astro.unl.edu/classaction/animations/coordsmotion/celhorcomp.html

20 www.boyce-astro.org © BRIEF 201420 Rising & Setting Stars Local Skies: How to determine your Latitude The altitude of the celestial pole in your sky is equal to your latitude.

21 www.boyce-astro.org © BRIEF 201421 Rising & Setting Stars Local Skies: Equator

22 www.boyce-astro.org © BRIEF 201422 Rising & Setting Stars Local Skies: 30 degrees South Latitude

23 www.boyce-astro.org © BRIEF 201423 Rising & Setting Stars Local Skies: 40 degrees North Latitude

24 www.boyce-astro.org © BRIEF 201424 Rising & Setting Stars Local Skies: North Pole

25 www.boyce-astro.org © BRIEF 201425 Rising & Setting Stars Measuring Angles on the Sky: Full circle = 360º 1º = 60 (arcminutes) 1 = 60  (arcseconds)

26 www.boyce-astro.org © BRIEF 201426 Rising & Setting Stars Measuring Angles on the Sky:

27 www.boyce-astro.org © BRIEF 201427 Rising & Setting Stars Declination Angles: http://astro.unl.edu/classaction/animations/coordsmotion/latsim.html Seasons Simulator: http://astro.unl.edu/classaction/animations/coordsmotion/transitmovie.html Alt/Az Simulator: http://astro.unl.edu/classaction/animations/coordsmotion/altazimuth.html Lat/Long Demonstrator: http://astro.unl.edu/classaction/animations/coordsmotion/longlat.html RA/Dec Demonstrator: http://astro.unl.edu/classaction/animations/coordsmotion/radecdemo.html Sun Motions Simulator: http://astro.unl.edu/classaction/animations/coordsmotion/sunmotionsoverview.html Motions of Sun Simulator: http://astro.unl.edu/classaction/animations/coordsmotion/sunmotions.html Sun Rays Simulator: http://astro.unl.edu/classaction/animations/coordsmotion/sunsrays.html Sun’s Position on Horizon: http://astro.unl.edu/classaction/animations/coordsmotion/horizon.html Season’s Simulator: http://astro.unl.edu/classaction/animations/coordsmotion/eclipticsimulator.html Rotating Sky Coordinate Systems Comparer: http://astro.unl.edu/classaction/animations/coordsmotion/celhorcomp.html

28 www.boyce-astro.org © BRIEF 201428 Rising & Setting Stars Sidereal Time and Hour Angle Demonstrator: http://astro.unl.edu/classaction/animations/200level/siderealTimeAndHourAngleDemo. html http://astro.unl.edu/classaction/animations/200level/siderealTimeAndHourAngleDemo. html Celestial and Horizon Systems Comparison: http://astro.unl.edu/classaction/animations/coordsmotion/celestialhorizon.html Sidereal and Solar Time Simulator: http://astro.unl.edu/classaction/animations/coordsmotion/siderealSolarTime.html

29 www.boyce-astro.org © BRIEF 201429 Rising & Setting Stars Questions?

30 www.boyce-astro.org © BRIEF 201430 Rising & Setting Stars Celestial Sphere: Our lack of depth perception when we look into space creates the illusion that Earth is surrounded by a celestial sphere In reality, stars that appear very close together in our sky may actually lie at very different distances from Earth.

31 www.boyce-astro.org © BRIEF 201431 Rising & Setting Stars Celestial Sphere: Our lack of depth perception when we look into space creates the illusion that Earth is surrounded by a celestial sphere In reality, stars that appear very close together in our sky may actually lie at very different distances from Earth.

32 www.boyce-astro.org © BRIEF 201432 Rising & Setting Stars The Celestial Sphere: Pasachoff_Fig. 4.25 © Cambridge University Press 2013

33 www.boyce-astro.org © BRIEF 201433 Rising & Setting Stars Precession: Precession: rotation of Earth’s axis itself; makes one complete circle in about 26,000 years This is due to the gravitational tug of BOTH the Sun and Moon. Earth’s axis currently points nearly toward the star Polaris. About 12,000 years from now—almost halfway through one cycle of precession—Earth’s axis will point toward a star called Vega, which will then be the “North Star.” Five thousand years ago, the North Star was a star named Thuban in the constellation Draco.


Download ppt "Chapter 4: Rising & Setting Stars www.boyce-astro.org © BRIEF 20141."

Similar presentations


Ads by Google