Local Horizon and Sundials
Rosa M. Ros
International Astronomical Union
Technical University of Catalonia, Spain
Goals
The Earth rotates and moves�rotation (day / night)� orbital position (seasons)
Activity 1: Four Earth spheres with �the Sun (a lamp) in the middle.�t�The line from the centre of the Sun to the centre of the Earth makes a 23.5° angle with the ground�(which represents the plane of the Equator).
Summer in the Northern Hemisphere
Winter in the Southern Hemisphere
Winter in the Northern Hemisphere
Summer in the Southern Hemisphere
Activity 2: Parallel Earth � �
� A spotlight illuminates two spheres in the same way and produces the same areas of light and shadow�
Activity 2: Parallel Earth
* Remove the globe from its mounting, take it outside and stand it on a glass
�* Carefully orientate its rotational axis with a compass
�* Turn it so our location is at the top
Activity 2: Parallel Earth
�
Place:
* a doll indicating our position
�* pieces of clay to mark the light / shadow line
(it advances with time)
�* pieces of toothpick to create shadows to study
Activity 2: Parallel Earth
* The North Pole is on the sunny side so it is summer in the Northern Hemisphere (the midnight sun)�� * The South Pole is in shadow and therefore in the Southern Hemisphere it is winter
Activity 2: Parallel Earth
�* The North Pole is within the area at darkness, so it is in the Northern hemisphere's winter.��* South Pole is illuminated and so it is summer in the Southern hemisphere.
Activity 2: Parallel Earth�
When the day / night shadow line passes through both poles, it is the first day of spring or the first day of autumn.
Activity 2: Parallel Earth
North H. summer North H. equinoxes North H. winter
South H. winter South H. equinoxes South H. summer
Rotation and celestial movements of day and night�
when seen
from inside
and outside
Celestial sphere "from outside"
... it seems that everything is understood
… but after class, ... he is disconcerted
All schools have an "Astronomy Laboratory"
Activity 3: We will build a model of the horizon visible from school
Begin by photographing all round your location
Rosa M. Ros
Let’s glue the photos together on a supporting platform
… we must adjust the photographed horizon to align it with the real horizon
Rosa M. Ros
To position the model we can use the compass direction, or better, we can use the projection of the pole above the horizon
Introducing the Earth’s rotation
The altitude of the pole is equal to your latitude
Indicate the apparent path of the sun on the first day of spring or autumn
Movement due to Earth’s rotation: �Note the angle of the Sun’s path
Movement due to Earth’s rotation: �Note the angle of the star trails
Rotational movement in the model
The inclination of the Sun’s apparent path and of the star trails depend on latitude
Solar paths on first day of each season (note the different durations)
Orbital motion leads to the seasonal positions
The Earth’s orbital motion leads to the change of the position of sunsets every day
Winter – Spring or Autumn – Summer
Viewing the �"meridian" in the model
Rosa M. Ros
…around the pole - circles
…near the equator the paths change from concave to convex
…the model is no more than an Equatorial Sundial!
…other sundials can be made from the equatorial one
… the horizontal sundial
…and the vertically oriented E-W sundial
… and with the Sun (or with a flashlight) we observe the model acting like a sundial
The three sundials in the model
Activity 4: Let's see how to build a �very simple “equatorial” sundial!
Activity 4: “equatorial” sundial!
Activity 5: How to Read the Time
Solar Time + Total Adjustment = Wristwatch Time
Total Adjustment =
Activity 5: Read the time, Longitude Adjustment
meridian longitude of your area.
Activity 5: Read the time, �Summer / Winter Adjustment
Activity 5: Read the time, �Equation of Time Adjustment
day | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
1 | +3m 33s | +13m 35s | +12m 22s | +3m 54s | -2m 54s | -2m 12s | +3m 50s | +6m 21s | +0m 2s | -10m 18s | -16m 24s | -11m 1s |
6 | +5m 50s | +14 m 5s | +11m 17s | +2m 27s | -3m 23s | -1m 22s | +4m 45s | +5m 54s | -1m 23s | -11m 51s | -16m 22s | -9m 1s |
11 | +7m 55s | +14m 14s | +10m 3s | +1m 4s | -3m 38s | -0m 23s | +5m 29s | +5m 13s | -3m 21s | -13m 14s | -15m 31s | -6m 49s |
16 | +9m 45s | +14m 4s | +8m 40s | -0m 11s | -3m 40s | +0m 39s | +6m 3s | +4m 17s | -5m 7s | -14m 56s | -15m 15s | -4m 27s |
21 | +11m 18s | +13m 37s | +7m 12s | -1m 17s | -3m 27s | +1m 44s | +6m 24s | +3m 10s | -6m 54s | -15m 21s | -14m 10s | -1m 58s |
26 | +12m 32s | +12m 54s | +5m 42s | -2m 12s | -3m | +2m 49s | +6m 32s | +1m 50s | -8m 38s | -16m 1s | -12m 44s | +0m 31s |
31 | +13m 26s | | +4m 12s | | -2m 21s | | +6m 24s | +0m 21s | | -16m 22s | | +2m 57s |
Activity 5: Reading Time
Example 1: Barcelona (Spain) on May 24th
Adjustment | Comment | Result |
1. Longitude | Barcelona is in the same "standard" zone as Greenwich. Its longitude is 2º 10’ E = 2.17º E = -8.7 m (1° is equivalent to 4 m) | -8.7 m |
2. Summer Time | May has daylight saving of +1 h | + 60 m |
3. Equation of Time | We read the table for May 24th | -3.4 m |
Total | | +47.9 m |
For example at 12h of solar time (noon), our watches indicated
(Solar time) 12h + 47.9 m = 12h 47.9 m (wristwatch time)
Activity 5: Reading Time
Example 2: Tulsa, Oklahoma (USA) November 16th
Adjustment | Comment | Result |
1. Longitude | The standard meridian of Tulsa is 90 ° W. Its longitude is 95º 58’ W = 96 º W, so it is 6° W from the standard meridian (1° is equivalent to 4 m) | +24 m |
2. Winter Time | November 16th does not have daylight saving added | 0 |
3. Equation of Time | We read the table for November 16th | -15.3 m |
Total | | + 8.7 m |
For example at 12h solar time (noon), our watches will indicate
(Solar time) 12h + 8.7 m = 12h 8.7 m (Wristwatch time)
the model serves to orientate us …
… to observe and understand …
Conclusions
Rosa M. Ros
Thank you very much �for your attention! �