The Big Dipper: various views and epochs The Celestial Sphere
• The stars appear to be fixed to the surface of a celestial sphere • The Earth rotates eastward – the stars appear to move east to west with diurnal motion of the sky • The celestial sphere contains all of the visible Universe • Half of the celestial sphere is visible from any location, but different halves for different locations and times of the day • The local horizon depends on latitude and time of day – stars not visible unless sun is below local horizon Long time exposure view to the north above new Gemini Long exposure looking south telescope, Mauna Kea, from Mt. Kilimanjaro, Africa – Hawaii – 19.50 N 30 S Motion of the Stars
North pole 51 ½ N latitude
Equator Three Views from a Mid-Northern Latitude
Constellations help chart motion of stars
Can you predict the angle that the paths Note make with the circumpolar horizon? stars and constellations – always above the horizon Constellations
Use planetarium software or web resources (www.heavens-above.com) to see sky motions Constellations Useful for keeping track of time, location, seasons – used by navigators for centuries
Sagittarius and Scorpius
Constellations have been associated with great heroes, creatures, gods in all ancient civilizations – modern usage is Greek names translated into Latin. Perseus and Andromeda
Ancient sky charts had poorly defined constellation boundaries.
from 1837
Modern convention has well-defined boundaries – celestial sphere divided into 88 constellations. Star Names
Most star names come from Arabic Star Names Since only 24 brightest stars in each constellation can be denoted by Greek letters…
Most stars numbered in catalogs, e.g., Henry Draper catalog
HD 100546, in constellation Musca, south celestial sphere. APOD 2001 May 2.
Swirling spiral- shaped disk Æ ongoing planet formation? The Yearly Motion of the Sun
Summer solstice – approx. June 21. Winter solstice – approx. Dec. 21.
0 Sun appears 23.50 above celestial Sun appears 23.5 below celestial equator. equator.
Summer in the Northern hemisphere, Winter in the Northern hemisphere, winter in Southern hemisphere. summer in Southern hemisphere. The Cause of Seasons Equal incoming energy spread over differing areas.
Can this explain the weather on June 21, Dec 21? The Yearly Motion of the Sun
The Sun completes a 3600 motion on the celestial sphere due to Earth-Sun orbit, but this path (the ecliptic) is offset from the celestial equator by 23.50.
What does the daily motion of the Sun look like at different times of year, from different locations on Earth? The Daily Motion of the Sun Like the stars, the Sun undergoes a diurnal motion due to the Earth’s rotation. This is independent of the slow yearly movement across the CS.
The daily paths of the Sun at latitude 400N. Notice the person’s shadows.
The summer (winter) Sun is above the horizon for more than (less than) 12 hours. The summer Sun stands higher in the sky at mid-day. However, note that it remains below the zenith at all times.
On equinoxes, the Sun moves along the celestial equator, from east to west – 12 hours each of daylight and night. Motion of the Planets
Mercury and Venus are often visible just after sunset in the western sky or just before sunrise in the eastern sky.
The other planets may be seen in the eastern sky at sunset and the western sky at sunrise.
Mercury and Venus are the only planets that are always within a fixed angular distance from the Sun. Why?