Astronomy 1 - September 16, 1998
Date: Wednesday - Sept 16, 1998
Topic: Horizon Coordinates and Time
NOTICES
See the notice of the Halifax RASC meeting for Friday (previous lecture notes)
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HOMEWORK- Due next Wednesday (Sept 23)
Chapter #1 Chaisson Problems # (see assignment on ACME)
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EQUIPMENT AND VISUAL AIDES
Plastic Coordinate Sphere
overheads: Monthly movement
Star chart to show ecliptic and equator
Hour Angle and TIME overhead
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LECTURE
-- Star Charts and Constellations
Outlines and labeling of stars
Ancient Arabic etc names
- Bayer letters (greek letters)
- Numbering
- SAO numbers
- HGSC numbers
- HD numbers(Henry Draper Catalog)
Scales of Atlases -
limiting magnitude of stars plotted
eg. Sky Atlas 2000.0 by Wil Tirion (43,000 stars to 8th mag)
Nortons 2000.0 (8700 stars to 6.5 mag)
ECU 1/4 million stars with SAO catalog to 9th mag
16 million start with HGSC (CDROM) to 15th mag
example: (overheads of NGC7331 in Perseus)
-- Horizon System (overhead transparencies)
Horizon related to Earth and Latitude, Longitude
Altitude and Azimuth
Examples: Show change in altitude and Azimuth on ECU
Calculation of Latitude from altitude of NCP
Terms: NCP, Celestial Meridian, Zenith, Zenith Distance
SCP, North Point, South Point, Celestial Equator
-- Declination and Altitude of objects on the Local Meridian
**Diagram to show how to calculate Altitude of Object on local meridian
Example - Trinidad and Shadow of vertical stick
(lat = 10 deg. May 30 solar dec = 21 deg)
Example: Altitude of Fomalhaut (dec = -30)
Vancouver lat = 49 deg
-- Rotation of the Earth and Hour Angle
Longitude and Time of Rise
Star/sun motion
Hour angle (OVER HEAD on rotation)
- Examples: Zenith Angle, Hour Angle etc of SUN
Edmonton June 21, dec = 23, a = 53o, HA = 45o
(draw position - see notes)
- RISE and SET
1- Moon Rise at latitude 45 deg example (notes)
2- Circumpolar stars and altitude versus latitude
Examples ( Victoria, Tucson, Wolfville)
Canopus visibility dec = -53 o
Southern Cross dec = - 63 o
- TIME and HOUR ANGLE: Earth Rotation relative to the SUN
HA = 0 to HA = 0 ----> 24 hours
60 minutes/hour 60 seconds/minute
24 hour = 360 degrees
1 hour = 15 degrees of rotation
1 min time = 15/60 degrees = 1/4 degree
OR 1 degree of Earth rotation = 4 minutes of time
(this is useful to remember)
also 1'arc of Earth rotation = 4 seconds of time
Diagram of Time Zones and Hour Angles
- TIME, TIMEZONES, and LONGITUDE
1. 15 degree wide time zones
2. UT = Universal Time (Time at 0 degree Longitude)
3. Offset of other timezones
Atlantic Time (Longitude = 60W) 4 hours earlier
Eastern Time (Longitude = 75W) 5 hours earlier
etc
(UT = AST + 4 hours)
(AST = UT - 4 hours)
(ADT = atlantic daylight time = AST + 1 hour)
4. Offset of Local Mean Time
- SIDERIAL DAY and SIDERIAL TIME
Diagram of Siderial Rotation
Siderial Day = 4 minutes shorter than Solar Day
360/36.986 x 86400 sec = 86164 sec
shorter by 236 seconds (240 sec = 4 min)
**Diagram of Siderial Time and Celestial Coordinate System
ST = hour angle of Vernal Equinox
RA = right ascension of celestial object
HA = hour angle of Celestial object
[ ST = HA + RA ] reduced to less than 24 hours
If HA = 0 (object on the meridian)
then ST = RA of celestial object on the local celestial meridian
-Example: What is the Siderial Time at the present time?
We need HA and RA of some celestial object
Use the Sun: Time = 5 pm ADT (HA = 4 hours) explain!
RA of the Sun = Sept 16 almost Autumnal Equinox
On Sept 23 RA = 12 hr
1 day ~ 1 degree = 4 min time
12 hr - (23 - 16)x 4 min = 12 hr - 28 min
RA = 11-1/2 hr
ST (now) = 4 + 11.5 = 15.5 hours
- What is the HA of Jupiter (RA = 23.5 hrs)
HA = ST - RA = 15.5 - 23.5 = - 8 hr
8 hours before Jupiter gets on our local celestial meridian
NEXT TIME: Precession of the Equinoxes, Equation of Time and Eclipses