Mindmap
P7: Naked Eye Astronomy

Mind map: Naked eye astronomy
Inhalt der Mindmap
P7: Naked Eye Astronomy
The Earth Rotates on its axis
- It does this West to East once in just under 24 hours
- This causes the stars to appear to move East to West in the same amount of time
- The sun, planets and moon also appear to move east to west across the sky, however the time they take to do this depends on their individual orbits
- The sun appears to travel across the sky once every 24 hrs
- A sidereal day is the time it takes for the earth to rotate 360 degrees on its axis
- A solar day is the time from noon one day, to noon the next (i.e. 24 hrs)
- The earth orbits the sun as well as rotating on its axis
- It is this that makes the sidereal day 4 minutes shorter that a solar day
- Different stars can be seen at different times of the year, depending on the position of the earth in the suns orbit
- The earth orbits the sun as well as rotating on its axis
- It does this West to East once in just under 24 hours
The Position of Astronomical Objects
- The position of astronomical objects can be measured in terms of angles as seen from the earth.
- Angles of "Declination" and "Right Ascension" describe the positions of stars in relation to a fixed point on the equator
- Declination is measured south and north of the Equator
- A star with Positive declination will be visible form the northern hemisphere
- A star with Negative Declination will be visible from the southern hemisphere
- Right ascension is measured around the celestial equator
- Declination is measured south and north of the Equator
- Angles of "Declination" and "Right Ascension" describe the positions of stars in relation to a fixed point on the equator
- Planets can be seen from earth with the naked eye, they look similar to stars but change their positions in a complicated pattern
- When compared to backgrounds of fixed stars, planets appear ti move with a retrograde motion
- This is because the earths smaller orbit causes it to overtake each of the outer planets at different times of the year.
- This causes these planets to slow down against the star background and go into reverse
- Retrograde motion- The apparent backwards motion of planets from west to east due to the combined motion of earth and the planets
- This is because the earths smaller orbit causes it to overtake each of the outer planets at different times of the year.
- When compared to backgrounds of fixed stars, planets appear ti move with a retrograde motion
- The position of astronomical objects can be measured in terms of angles as seen from the earth.
The Moon
- Whilst the Earth is rotating on its axis, the moon is orbiting the Earth in the same direction
- Due to this, the moon appears to be moving East to West across the sky in a little over 24 hours, faster than the earth
- The Lunar Cycle describes the moons appearance during its 28 day orbit
- The moons shape during its orbit is due to the part of the moon that is visible to the earth
- We are able to see the moon because of the suns light reflecting off it
- The side facing away from the sun appears dark
- The side facing towards the sun appears light
- We are able to see the moon because of the suns light reflecting off it
- The moons shape during its orbit is due to the part of the moon that is visible to the earth
- Whilst the Earth is rotating on its axis, the moon is orbiting the Earth in the same direction
Eclipses
- Solar Eclipse
- This occurs when the moon passes between the earth and the sun
- This results in the moon casting a shadow on the earth
- Total Solar Eclipse
- Occurs when the moon is directly in front of the sun and completely obscures the earths view of the sun
- This occurs when the moon passes between the earth and the sun
- Lunar Eclipse
- Occurs when the earth is between the sun and the moon
- Results in the Earth casting a shadow on the moon
- Occurs when the earth is between the sun and the moon
- Lunar eclipses don't occur every month because the moon orbits the earth at a 5 degree angle to that of the earths orbit of the sun
- An eclipse can only occur when the moon passes through the ecliptic ( the apparent path the sunlight traces out along the sky)
- There are between 2 and 5 solar eclipses ever year
- A total eclipse will only occur roughly ever 18 months
- An eclipse can only occur when the moon passes through the ecliptic ( the apparent path the sunlight traces out along the sky)
- Solar Eclipse
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- Physics (P7) Mindmap am P7: Naked Eye Astronomy, erstellt von jamiemcparlin am 08/05/2013.
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