Near edge-on view.

Slides:



Advertisements
Similar presentations
Earth in Space 19-1 Astronomy is the study of objects beyond the Earth’s atmosphere. It is one of the oldest sciences, as ancient people studied the heavens.
Advertisements

Unit 9: Earth Cycles Vocabulary.
Observing the Sky The Birth of Astronomy.
Chapter S1 Celestial Timekeeping and Navigation
Chapter S1 Celestial Timekeeping and Navigation
Prof. D.C. Richardson Sections
Seasons Review Earth’s rotation axis is tilted 23.5 degrees; tilt remains the same as it orbits the sun Therefore, different parts of the Earth receive.
The Memphis Astronomical Society Presents A SHORT COURSE in ASTRONOMY
The Sun-Earth-Moon System
27.3 – Sun-Earth-Moon System
Orbit of the Moon around the Sun
A100 Oct. 13 Keeping Time READ Essay 2 – Keeping Time in the text, pp
Climate and Latitude Sun’s rays spread over large area = cooler
Topic 4 Motions of the Earth, Moon, and Sun
Bringing Astronomy Down to Earth What do we know about Earth – Moon – Sun interactions?
Celestial Sphere Stars seem to be on the inner surface of a sphere surrounding the Earth.
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Observing Astronomy 315 Professor Lee Carkner Lecture 3.
The Earth Rotates.
Astronomy 104 Lunar Phases AndEclipses January 24, 2007.
August 29, 2011: 10am Class On-line Quiz #1 on d2l: Please complete before class on Friday, Sept. 2 HW 2 on line (d2l and boojum): Create a Constellation.
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Earth as a Planet Earth’s position in space Shape & Size of Earth
Knowing the Heavens Chapter Two. Naked-eye astronomy had an important place in ancient civilizations Positional astronomy –the study of the positions.
The Night Sky. Diurnal (daily) motion of the stars Like the Sun, the stars generally rise in the east and set in the west. This daily motion of the.
The Celestial Sphere The 88 official constellations cover the celestial sphere. If you do not have a model of the celestial sphere to bring to class, you.
Unit 8 Study Guide Notes Earth, Moon, and Sun.
Motion of the Moon.
Sponge: What two factors cause the seasons on Earth?
Earth Moon and Sun Interactions
Space Cycles Moon Phases Seasons.
Earth Motions and the Heavens
Week 2 Earthly Phenomena: Seasons Lunar Phases Solar and Lunar Eclipses Tides Reading: E2, E3, 5.2 (12 pages)
Earth’s Motions Unit 4.
Seasons and the Angle of Solar Radiation Rotation: the time it takes a planet to rotate (spin) once on its axis. For Earth = 1 day.
Chapter 1: The Cycles of the Sky
CHAPTER 1: Discovering the Night Sky.
Introduction to Astronomy.  Observations lead to theories and laws  Laws are concise statements that summaries a large number of observations.  Theories.
Chapter 2 Discovering the Universe for Yourself
Celestial coordinates
Seasons, Phases of the Moon and Eclipses Chapter 2.2 & 2.3.
Equinoxes and Solstices When the ecliptic and celestial equator intersect, day and night are each 12 hours long: the equinox. When the Sun reaches its.
The Seasons There would be no seasons if the Earth were not tilted on it’s axis!  Nick Devereux 2006.
1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.
Chapter 1 Charting the Heavens.
Last time: 2.1. Patterns in The Sky: Stars and constellations, TODAY: celestial coordinates 2.2 Seasons,…Precession 2.2 (cont.) The Moon and Eclipses.
To an observer on Earth, the bright and dark portions of the moon appear to change shape during each phase. The diagram, however, shows that during each.
Chapter 1 Predicting the Motions of the Stars, Sun, and Moon.
Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as.
Why do we have seasons? Seasons are the result of the tilt of the Earth's axis. Earth’s axis is tilted 23.5°. This tilting is why we have SEASONS like.
Mastering Astronomy.
Revolution/Rotation Day/Night Phases of the Moon Seasons.
The study of the moon, stars, and other objects in space.
Quiz #1 Review Thursday, 15 September 2011 I list here the main topics and the main points for each topic. Study also the indicated lecture notes.
The Sun, The Moon, and Observing the Heavens. 0/0 If you could see stars during the day, the drawing below shows what the sky would look like at noon.
Axis: imaginary line that passes through Earth’s center and the North & South Poles Earth’s axis tilt = 23.5° causes Earth’s seasons causes ‘length’ of.
27.3 – Sun-Earth-Moon System dfrhmBrI.
CHAPTER 1.1 – EARTH IN SPACE. I. HOW EARTH MOVES Definition of Astronomy: The study of the moon, stars, and other objects in space. Definition of Astronomy:
Astronomy vs. Astrology Astronomy: Astronomy: The scientific study of matter in outer space, especially the positions, dimensions, distribution, motion,
Earth and Its Moon. Movement of the Earth in Space A.The Earth’s Rotation: the turning of the Earth on it’s axis. * axis – the imaginary line from the.
Motion of the Moon. Review Question Describe the path the Sun will take across the sky on the day of the autumnal equinox as viewed from the Earth’s equator.
Knowing the Heavens Chapter Two.
Chapter S1 Celestial Timekeeping and Navigation
The Sun-Earth-Moon System
Winter Sky – Facing North
The Sun-Earth-Moon System
Earth in Space.
The Cycles of the Sky.
Seasons & Moon Motion.
The Reasons for Seasons
Presentation transcript:

Near edge-on view

The arctic circle The arctic circle is the northern latitude at which on the summer solstice the Sun never sets and on the winter solstice the Sun never rises above the horizon.

Discussion What is the latitude of the arctic circle?

Discussion The tropics mark the furthest points north and south where the Sun can appear at the zenith. What is the latitude of the tropics?

Discussion How far above the southern horizon is the Sun on the summer solstice as viewed from a latitude of 42 degrees north?

Earth’s rotation

Discussion Why is Kennedy Space Center in Florida and not in Maine?

Centrifugal force This extra velocity at the equator pushes the matter out at the equator.

The Earth is not a perfect sphere The Earth is oblate, it bulges out at its equator. The diameter measured along its equator is 43 km larger than its diameter from the north to the south pole.

Sun and Moon apply a torque

Precession This off axis force, or torque, on the Earth causes Earth’s rotation axis to vary slightly, or precess, over long periods of time. Thus, the celestial poles trace out a circle against the stars over a period 26,000 years.

Precession

Discussion The Great Pyramid at Giza has a tunnel which points toward the north celestial pole. At the time the pyramid was built, around 2600 BCE, toward which star did it point?

Discussion If the position of the north and south celestial poles changes in the sky, what else changes position on the celestial sphere?

Precession of the Equinoxes If the celestial poles change with time, so too must the celestial equator, which is 90 degrees away from the poles. If the celestial equator changes with time, than the intersection of ecliptic and the celestial equator will also change with time.

Age of Aquarius? The “age” is defined by which constellation the Sun is in on the vernal equinox. Currently, it is the age of Pisces.

Discussion Why is the changing of the equinox position important?

Tropical year The length of our calendar year is defined by the time it takes between two vernal equinoxes. This is called the tropical year and is 365 days 5 hours 48 minutes and 46 seconds long.

Sidereal year However, because the equinox positions slowly change, this is not the Earth’s actual orbital period around the Sun. The actual orbital period is called the sidereal year and is 365 days, 6 hours, 9 minutes and 10 seconds, or 20 minutes 24 seconds longer.

What is the difference? If we used the sidereal year for our calendar year the seasons would slowly migrate through the different months over time. Spring would come one day earlier every 70 years.

Leap Years There are 365.242 days per tropical year, or about a quarter of day more than 365. To make everything come out even we therefore add an extra day to our year every four years.

Astronomical coordinates Because of precession and the changing position of the celestial poles and the vernal equinox, celestial coordinates of astronomical objects change from year to year.

Astrology Your astrological sign is the constellation the Sun was in on the day you were born. But, the constellation the Sun is in at any given time of the year changes due to precession. Astrology ignores this change.

TRADITIONAL ASTROLOGICAL DATES ACTUAL ASTRONOMICAL DATES TODAY (c. 2000 C.E.) Constellation Date Span Days Aries 21 Mar - 19 Apr 30 19 Apr - 13 May 25 Taurus 20 Apr - 20 May 31 14 May - 19 Jun 37 Gemini 21 May - 20 Jun 20 Jun - 20 Jul Cancer 21 Jun - 22 Jul 32 21 Jul - 9 Aug 20 Leo 23 Jul - 22 Aug 10 Aug - 15 Sep Virgo 23 Aug - 22 Sep 16 Sep - 30 Oct 45 Libra 23 Sep - 22 Oct 31 Oct - 22 Nov 23 Scorpio 23 Oct - 21 Nov Scorpius 23 Nov - 29 Nov 7   Ophiuchus 30 Nov - 17 Dec 18 Sagittarius 22 Nov - 21 Dec 18 Dec - 18 Jan Capricorn 22 Dec - 19 Jan 29 Capricornus 19 Jan - 15 Feb 28 Aquarius 20 Jan - 18 Feb 16 Feb - 3/11 24-25 Pisces 19 Feb - 20 Mar 30-31 12 Mar - 18 Apr 38

The Moon As we pass through the month, the appearance of the Moon changes each night. We say the Moon goes through a series of phases.

Discussion Many people believe incorrectly that the phases of the Moon are caused by the shadow of the Earth on the Moon. What simple observation of the Moon could you make to prove that they are wrong?

First quarter Moon

The Earth is round The “shadow” on a first or last quarter Moon is a straight line dividing the face of the Moon in half. The Earth is round and will always cause a curved shadow on the Moon. When the shadow of the Earth does fall on the Moon we call this a lunar eclipse.

The real reason The Moon’s phases are actually cause by the changing position of the Moon with respect to the Sun. The side of the Moon facing the Sun is always fully illuminated (except during a lunar eclipse). But because the angle we view the Moon differs from that of the Sun, we see varying degrees of the Moon’s surface facing us illuminated.

New Moon Occurs when the Moon is in the same part of the sky as the Sun. Thus the Moon is up during the day, and the illuminated side of the Moon faces away from the Earth. The Moon is not visible when it is new.

Waxing crescent When less than ½ of the Moon’s face is illuminated. It is the western side of the Moon’s face that is illuminated and the Moon is visible in the sky before Sunset. Waxing means increasing.

First Quarter When exactly ½ of the Moon’s face is illuminated. It is the western side of the Moon’s face that is illuminated and the Moon is up before sunset. Although ½ of the Moon’s face is illuminated it is called a quarter because the Moon is ¼ of the way through it’s cycle and occurs about one week after the new phase. The Moon is 90 degrees away from the Sun in the sky.

Waxing Gibbous When more than ½ of the Moon’s western face is illuminated.

Full Moon when the Moon’s face is fully illuminated. At this time the Moon is directly opposite the Sun. Occurs about 2 weeks after the new phase.

Waning Gibbous when more than ½ of the Moon’s face is illuminated. But now it is the eastern face that is illuminated and waning means decreasing.

Last Quarter when ½ of the Moon’s face is illuminated. Again it is the eastern half that is illuminated and the Moon is visible after sunrise. Occurs about 3 weeks after the new phase.

Waning Crescent When less than ½ of the eastern half of the Moon’s face is illuminated.

Discussion If the Moon is in its full phase on March 21st and the Sun sets at 6:00 P.M. what time does the Moon rise? What time does the Moon reach the meridian? What time does the Moon set?

The full Moon is exactly opposite the Sun or 180 degrees away in the sky. Astronomers would measure this angle in hours and say it is 12 hours from the Sun. If sunset is at 6:00 P.M. the full Moon rises at 6:00 P.M., crosses the meridian at midnight and sets at sunrise at 6:00 A.M., 12 hours different from the Sun.

Discussion If the Moon is in its last quarter phase on March 21st and the Sun sets at 6:00 P.M. what time does the Moon rise? What time does the Moon reach the meridian? What time does the Moon set?

The last quarter Moon is 90 degrees to the west of the Sun in the sky, or 6 hours before the Sun. If sunset is at 6:00 P.M. and rises at 6:00 A.M. (we are at the equinox) the last quarter Moon rises at midnight, crosses the meridian at 6:00 A.M and sets at noon.

Discussion Suppose it is the first day of autumn in the northern hemisphere. What phase is the Moon if the Moon is located at the position of the vernal equinox?

Discussion Suppose it is the first day of autumn in the northern hemisphere. What phase is the Moon if the Moon is located at the position of the vernal equinox? If the Moon is at the position of the vernal equinox it must be 180 degrees from the Sun and therefore full.

Discussion Suppose it is the first day of autumn in the northern hemisphere. What phase is the Moon if the Moon is located at the position of the winter solstice? Explain.

Discussion Suppose it is the first day of autumn in the northern hemisphere. What phase is the Moon if the Moon is located at the position of the summer solstice? Explain.

Discussion Suppose it is the first day of autumn in the northern hemisphere. What phase is the Moon if the Moon is located at the position of the summer solstice? Explain. The Moon is 90 degrees behind the Sun. Because the Sun is moving eastward relative to the stars, the Moon is 90 degrees to the west of the Sun and therefore in last quart phase.

Discussion The Moon goes through its phases in 29.53 days. This is called the synodic month, i.e. the month relative to the Sun. The actual orbital period of the Moon is 27.32 days, the sidereal month. Why is there a difference in the synodic and sidereal months?

In the 27.32 days that the Moon has taken to orbit the Earth the Earth has moved in its orbit relative to the Sun. The Earth moves about 1 degree per day so that after 27 days the Moon needs to move through an extra 27 degrees in the sky to get back to the same position relative to the Sun.

Discussion The Moon always keeps the same side facing the Earth. Does this mean the Moon does not spin on its axis? Explain?

Synchronous Rotation If the Moon did not spin on its axis we would see the Moon’s entire surface over the month. The Moon therefore does rotate but the rotation period is exactly equal to its orbital period and rotates such that we always see the same face. Thus, the Moon’s rotation period is synchronous with its orbital period.