Presentation on theme: "Comet Machholz passes the Pleiades. Comet Machholz C/2004 Q2 Discovered byDonald Machholz, Jr. on August 27, 2004 Period of about 120,000 years Just up."— Presentation transcript:
Which stars are circumpolar? The altitude of the North Celestial Pole is equal to our latitude, about 43 degrees. Only those stars within 43 degrees of the NCP are seen as circumpolar at our location So stars with a declination greater than 90 - 43 = 47 degrees are circumpolar for us
Which of the following stars are circumpolar as seen from a latitude of 60 degrees north? –Polaris declination = 89 degrees –Sirius declination = -17 degrees –Vega declination = 39 degrees
Some stars never rise above our horizon A star directly overhead has a declination equal to your latitude. A star that just manages to appear above your southern horizon will be 90 degrees further south. A star with a declination below -47 degrees will never rise above our horizon
Rules For an observer at latitude x north –Circumpolar: stars of dec > 90-x –Never seen: stars of dec < -(90 –x) –All of the stars with inbetween declinations are sometimes above our horizon and sometimes below it
If you are at the North Pole Which stars are circumpolar? Which stars would you never see?
If you are at the equator Which stars are circumpolar? Which stars do you never see?
Local Skies Lines of constant declination cross the sky at different altitudes, depending on your location on Earth. –declination line = your latitude goes through your zenith –the altitude of the N or S celestial pole = your latitude
Celestial Coordinates lines of Right Ascension & Declination lines of constant R.A. continually move in the sky as Earth rotates Movie. Click to play.
Huygens probe landed on Saturn’s moon Titan First data expected later today if all goes well
Solar vs. Sidereal Day Sidereal day – time it takes a star at the meridian to return to the meridian. –23 hours 56 min 4 sec Solar day – time it takes the Sun at meridian (noon) to return to the meridian. –noon to noon or 24 hours Why the 4-minute difference? –as it rotates, the Earth also orbits the Sun –Earth must rotate an extra degree (4 min) each day… – for any observer on Earth to be at noon again
What is the LST? LST = local sidereal time LST = 0 when the Vernal equinox is transiting the meridian LST = 0 at local midnight at the autumnal equinox –LST is 2 hours later at midnight for every month that goes by since the autumnal equinox
What is the LST at local midnight tonight? LST = 0 + 2 X (3.7 months) = 7.4 hours 7.4 hours = 7 hours 24 min At midnight eastern standard time LST = 7 h 24 m – 37 minutes = 6 h 47 min A star with right ascension 6h 47 min would be on the meridian at that time
What is the LST at 8pm? LST = 6 h 47 min – 4 = 2h 47 min
Annual Motion of the Sun The R.A. of the Sun… –increases about 2 hours per month The Declination of the Sun… –varies between –23º and +23º
Review questions (open notes) 1. At local midnight on April 1, 2005, what will be the approximate LST? 2. You are on a ship at latitude 10 degrees north. a. Stars of what declination are circumpolar for you? b. Stars of what declination never rise above your horizon? 3. At the summer solstice, around June 21, what is the declination of the sun? 4. At the summer solstice what is the altitude of the sun at local noon as seen from East Lansing (latitude about 43 degrees)?