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The sun Due to the earth’s tilt and its orbit around the sun, the declination of the sun changes with time of year 23.45 o at summer solstice (21 June)

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Presentation on theme: "The sun Due to the earth’s tilt and its orbit around the sun, the declination of the sun changes with time of year 23.45 o at summer solstice (21 June)"— Presentation transcript:

1 The sun Due to the earth’s tilt and its orbit around the sun, the declination of the sun changes with time of year o at summer solstice (21 June) 0 o at vernal and autumnal equniox (21 Mar, Sept) o at winter solstice (21 Dec) The sun looks like a “star” that changes declination, but also moves through the background of fixed stars over the course of the year.

2 In a given day To a good approximation: –The sun moves like a star with A fixed declination A fixed Sidereal Hour Angle Over the course of a year To a good approximation: –The sun moves against the background of fixed stars Declination changes like a sinusoid SHA changes by approx. 1 o per day

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4 Declination as a function of date o o Summer Solstice Winter Solstice

5 Due South Latitude = 90 o +Decl-Meridian height Meridian height Meridian height is related to latitude and declination

6 Calculating declination on a “desert island” d = declination Day = number of days after 21 March What if you don’t have a calculator or a table of sines or MS Exel?

7 Rule of 12ths: changes are 1:2:3:3:2:1 for sine curves Graphically – draw approximation to sine curve and interpolate visually

8 Radius=23.45 Draw a circle, and measure angles (Burch) Could approximate angle as days after 21 March

9 Something you won’t remember on a desert island: This varies from the other formula by as much as 2 degrees Blame: orbital parameters of the earth, leap year differences, eccentricity of orbit…..buyer beware!!

10 SourceDeclination (degrees) Length of day (hours) Simple form Complex form Random website NOAA online Another NOAA Who are you going to trust? - Declination for Oct. 16 th from various sources NB – if you tried to estimate latitude from length of day, you would see variations of 360 nautical miles!! Also- changes most rapidly this time of year.

11 The sun moves across the sky at 15 o per hour With a compass can be used to tell local time With a shadow stick can be used to find due South (shortest shadow) or latitude

12 Watch method for finding South Not talked about much because we all have digital watches these days. Point the hour hand at the sun. Due south is halfway between the hour hand and 12 on the watch NB works only when the sun is below 45 o in the horizon. –When sun is high, lines of azimuth converge - inaccurate See tables in Gatty’s book for more accurate numbers using a compass

13 Shadow stick method

14 Precision of altitude measurements These are limited by 1.) height of sun and 2.) measuring instrument With hands – only if very low in the sky (arctic) can one get a degree or so. With shadow stick – depends on the geometry – maybe 1 o With quadrant – maybe 1 o Warning – do not look directly at noon-day sun – use smoked glass etc With sextant – maybe 2-4 ’

15 Steve Callahan – from Adrift

16 Example: Shadow stick work compared with GPS on trip from Orlando to PA

17 θ Due East Summer Solstice rises N of E Winter Solstice rises S of E The sun will look like a star that has a declination that varies with time of year – hence rising/setting azimuth changes Rising and setting angles are (90 o -Latitude) at the equinox At any latitude – the maximum rising/setting angle north or south of due east/wests called the sun’s amplitude Equinox, rises due east

18 Viking sun compass Found in Greenland by the archeologist C. L. Vebæk Indicates 32 compass points. Hole in the center is where the gnomon (or pointer for Sun-shadow) goes. Markings on surface are Interpreted as guides for sunrise and sunset angles.

19 Interpretation of the scratches are hyperbolae that give the position of the gnomon’s shadow at different times of the day

20 From the azimuth/declination/latitude formula, you can get the amplitude for any latitude (use R z formula from last week) Note: it goes offscale at 66 o N or S, at the artic circle

21 Terminator of earth – sunset in the summer over Europe and Africa Direction of sunset is perpendicular to terminator

22 you dec Terminator day night Length of day = 24*d/360 o d Side view Top view Length of day from latitude and declination

23 Example: Boston – constant lat, different dates

24 16-Oct-2008, Decl. of sun = o hours of daylight

25 Time Need a watch – typical wristwatches are pretty accurate –Can calibrate – NIST time service: –http://tf.nist.gov/service/its.htmhttp://tf.nist.gov/service/its.htm –Keep track of gain/loss –Precision of a few seconds possible (less than a nautical mile) Limiting factors become accuracy of sightings

26 1 o of Latitude = 0.04 hours = 2.4 min. Close up of daylight on Oct. 16 near latitude of Boston

27 Comments on latitude from length of day Angular diameter of the sun is 32.5 ’ (2 minutes) At horizon, must factor in refraction effects Works best around the solstices Almost impossible to use around equinox –Daylight the same at all latitudes Accuracy of declination, other factors Distortion of sunset from refraction

28 Comparison – naïve approach (mine) to NOAA calculation at solstice and Oct 16th Oct 16 th – 1 o = 2.4 minutes of daylight Solstice – 1 o = 15 minutes of daylight Oct 16 th – 1 o error in declination Solstice – no error in declination Oct 16 th – 28 minutes difference in daylight Solstice – 8.4 minutes difference in daylight Oct 16 th – difference in latitude = 6 o Solstice – difference in latitude = 0.56 o Huge difference!!

29 Special considerations for areas near the North or South Pole

30 Midnight above the arctic circle – perfect for determining latitude from horizon grazing!!

31 Mean Solar Time The common meaning of “time” (how we set our watches) is mean solar time. Places the highest point of the sun in the sky (solar meridian) roughly at noon. –Achieved by shifting time zones for every 15 o of longitude Greenwich Mean Time (GMT) is used as prime meridian Variations caused by –Axial tilt of earth –Eccentricity of earth’s orbit (speeds up and slows down) –Position within time zone –Leap year effects – one year is not precisely days (minor for the primitive navigator) –Tidal forces from moon slows down the earth’s rotation ever so slightly (VERY minor)

32 Time zones are approx. 15 o wide in longitude centered on local noon (modulo political boundaries)

33 Equation of time describes deviations of the sun’s true position at noon from mean solar time (negative means the sun is late relative to mean solar time)

34 Memorization trick for E.o.T. – 14 minutes late on Feb. 14 th (Valentines day), 4 days early three months later (May 15 th ), 16 minutes early on Halloween, 6 minutes late 3 months earlier (June 26 th ) Approximate this – 2 weeks either side of points are flat, use trapezoids to connect

35 Longitude from local noon Variation of height of sun at meridian crossing is very slow – not accurate Mid-point between a time of sunrise and sunset is most accurate With a watch – measure identical height above horizon at sunrise and sunset using hands or kamal for accuracy

36 The kamal – used by ancient Arab sea traders Based on same principle as use of hands to measure angles Knotted string allows for range of angles Board at end is calibrated in degrees Hold knot in teeth and read off elevation from horizon

37 Local Area Noon Correction from equation of time Then – knowing watch time zone (from GMT) – caclulate time difference from of LAN from GMT, and convert to degrees from prime meridian Accuracy of sighting of sunrise and sunset with a kamal should be fairly accurate – much better than 1 degree. Fraction of the sun’s diameter (10 ’ = 10 nautical miles)

38 The analema A simultaneous plot of solar declination and time of the sun (relative to mean solar time) produces a figure 8 called an analema A photo of the sun at the same time every day for a year

39 An “analemmatic” sundial corrects for the equation of time – with different locations of the gnomon (shadow stick) depending on date.

40 Incoming Scattered light is polarized at 90 o scattering Why the sky is blue and polarized? The light reaching your eyes from the sky is the result of a single scatter off of air molecules. This scattering is called “Rayleigh scattering”. It is larger at higher Frequencies (shorter wavelengths) – so blue scatters best. Also, light is polarized when scattered at 90 o

41 At sunset, light has all the blue scattered out of it, and is red.

42 Polarization of the sky depends on the location of the sun Sun at zenithSun at horizon

43 Photo of the sky with a polarization filter Polarization filter

44 The Viking sun stone From Harafns Saga: “the weather was thick and stormy…The king looked about and saw no blue sky…then the king took out the sunstone and held it up, and then he saw where the Sun beamed from the stone.” Modern speculation is that the sun stone was Icelandic spar (calcite) that was used to get polarization information from the sky for the direction of the sun.

45 Calcite is “birefringent” – meaning that two different polarization states of light have two different refractive indices

46 Speculation on the sun stone The sun was often low on the horizon during the voyaging season A lot of fog also was low in the sky and could obscure the sun Sky polarization would be observable overhead, and could have been used Large sources of calcite on east coast of Iceland.

47 The moon Although the moon can be used for celestial navigation, it can’t really be used for “primitive” navigation, except for rough direction finding (i.e. not latitude and longitude – need sextant, clock and tables) Tidal forces from the earth slowed down the moon’s rotation until it shows the same face to us. The moon moves to the east in rotation by 12 o per day (half a degree per hour). Moves west like the sun, at 15 o per hour The lit side of the moon always faces the sun –Full moon rises opposite the setting sun around the time of the equinox –Website for moon phases: –http://tycho.usno.navy.mil/vphase.html

48 Due South Direction of sun 14.5 o per hour Horns of moon point south B Bright face of moon always faces the sun – phase of the moon tells you the angle to the sun

49 Oct. 14Oct. 15Oct. 16Oct. 17Oct. 18Oct. 19Oct. 20 Oct. 28Oct. 29Oct. 30Oct. 31Nov 1Nov. 2Nov. 3 Oct. 21Oct. 22Oct. 23Oct. 24Oct. 25Oct. 26Oct. 27 Nov. 4Nov. 5Nov. 6Nov. 7Nov. 8Nov. 9Nov. 10 Moon opposite Sun 180 o to 270 o 270 o to 0 o 0 o to 90 o 90 o to 180 o New Moon


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