Newton’s Universal Law of Gravitation and planetary orbits
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Newton’s Universal Law of Gravitation and planetary orbits. Announcements. The first homework due Thursday (at the start of class). The next assignment will be posted on the website on Thursday Weekly preceptor-led study group Every Monday 10:30AM-12:00Noon Mission update volunteers?.

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Newton’s Universal Law of Gravitation and planetary orbits

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Newton s universal law of gravitation and planetary orbits

Newton’s Universal Law of Gravitation and planetary orbits

Gravity (cont.) / Night Sky / Seasons

1/23/07


Announcements

Announcements

  • The first homework due Thursday (at the start of class).

    • The next assignment will be posted on the website on Thursday

  • Weekly preceptor-led study group

    • Every Monday 10:30AM-12:00Noon

  • Mission update volunteers?

Gravity (cont.) / Night Sky / Seasons

1/23/07


Newton s universal law of gravitation and planetary orbits

Tonight's Public-Lecture Series: Dr. Martin TomaskoMission to the Surface of Saturn’s Moon Titan(7:30 PM, 308 of Kuiper – this room)

Gravity (cont.) / Night Sky / Seasons

1/23/07


Stereo first light image of comet mcnaught

STEREO “first light” image of Comet McNaught

Gravity (cont.) / Night Sky / Seasons

1/23/07


Today s topics

Today’s Topics

  • Gravity continued

    • Newton’s Universal law of Gravitation

    • orbits

  • Diurnal and seasonal variations

    • The motion of stars and planets in the sky

    • What is the reason for the seasons?

Gravity (cont.) / Night Sky / Seasons

1/23/07


Newton s law of universal gravitation

Newton’s Law of Universal Gravitation

  • Gravitation force between two bodies

•G = Gravitational Constant = 6.67x10-11 N • m2 / kg2

• m1 and m2 = the masses of the two objects

• r = the distance between the two (more precisely,

the distance between the two centers)

Gravity (cont.) / Night Sky / Seasons

1/23/07


Example 1

Example #1

  • A boy with a mass of 25 kg experiences how much less of a gravitational force by the Earth than a man with a mass of 100 kg?

  • (possibly) Useful info

    MEarth = 5.97x1024 kg

    REarth = 6378 km

Gravity (cont.) / Night Sky / Seasons

1/23/07


Example 2

Example #2

  • Suppose that Earth were at 10 AU. How much less of a gravitational force from the Sun would it experience?

  • Note 1AU = 1.5x108 km

    MSun = 2x1030 kg

Gravity (cont.) / Night Sky / Seasons

1/23/07


Example 3

Example #3

  • How much would a man weight on Mars if he weighs 200 pounds on Earth?

    Useful info:

    The mass of Mars = 10 times less than Earth

    The radius of Mars = ½ times smaller than Earth

Gravity (cont.) / Night Sky / Seasons

1/23/07


Orbits

Orbits

  • The law of universal gravitation accounts for planets not falling into the Sun nor the Moon crashing into the Earth

  • Paths A, B, and C do not have enough horizontal velocity to escape Earth’s surface whereas Paths D, E, and F do.

  • Path E is where the horizontal velocity is exactly what is needed so its orbit matches the circular curve of the Earth

Gravity (cont.) / Night Sky / Seasons

1/23/07


Physics of spaceflight weightlessness

Physics of spaceflight: Weightlessness

  • Astronauts are actually still falling

    • they are falling with the spacecraft

  • They sometimes train for missions in large airplanes.

Gravity (cont.) / Night Sky / Seasons

1/23/07


New subject the night sky

New Subject: The Night Sky

  • The night sky changes in a number of ways

    • Diurnal variations

    • Seasonal variations

    • Pole-star wander

  • These variations can be understood in terms of the combined effects of the spinning of the Earth on its axis, the orbit of Earth about the Sun, and the precession of Earth’s spin axis.

Gravity (cont.) / Night Sky / Seasons

1/23/07


Diurnal motion

Diurnal motion

  • “Diurnal” means having a period of 1 day.

  • Stars appear to rise in the east, slowly rotate about the earth and set in the west.

  • This diurnal or daily motion of the stars is caused by the ~24-hour rotation of the Earth on its axis.

Gravity (cont.) / Night Sky / Seasons

1/23/07


Diurnal motion1

Diurnal Motion

Gravity (cont.) / Night Sky / Seasons

1/23/07


Diurnal motion2

Diurnal Motion

Gravity (cont.) / Night Sky / Seasons

1/23/07


Seasonal variations in the night sky

Seasonal variations in the night sky

  • The stars also appear to slowly shift in position throughout the year

  • This is due to the orbit of the Earth around the Sun, relative to the (essentially) fixed stars

  • If you follow a particular star on successive evenings, you will find that it rises approximately 4 minutes earlier each night, or 2 hours earlier each month

Gravity (cont.) / Night Sky / Seasons

1/23/07


Constellations

Constellations

Orion – A Winter/Spring Constellation

Sagittarius – A Summer Constellation

  • Zodiac Constellations are those that the planets and Sun move through

    • Near the ecliptic plane!

    • Leo, Sagittarius, Scorpio, Taurus, etc.

  • The constellation that the Sun is in on your birth date defines which zodiac sign you are

Gravity (cont.) / Night Sky / Seasons

1/23/07


What causes the change of seasons

What causes the change of seasons?

Gravity (cont.) / Night Sky / Seasons

1/23/07


The source of energy that heats earth s surface the sun

The source of energy that heats Earth’s surface – the Sun

Gravity (cont.) / Night Sky / Seasons

1/23/07


Proximity to the sun partly determines the temperature of a planet s surface

The closer a planet is to the Sun, the warmer its surface will be

The received solar energy decreases with the square of the distance to the Sun

If Earth were at 2AU, it would receive 22 = 4 times less solar energy

Proximity to the Sun partly determines the temperature of a planet’s surface

Gravity (cont.) / Night Sky / Seasons

1/23/07


Newton s universal law of gravitation and planetary orbits

These Solar magnetograms show that the size of the Sun as seen from Earth changes depending on where Earth in its orbit

_________________________________________________________

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January, 1989

July, 1989

The Earth is closer to the Sun in January

Gravity (cont.) / Night Sky / Seasons

1/23/07


Newton s universal law of gravitation and planetary orbits

  • Recall that Earth’s orbits is very nearly circular

    • The Earth’s orbital eccentricity = 0.017

      This is too small to effect the seasons

The solar energy at Earth’s orbit at:

Perihelion = 1420 W/m2

Aphelion = 1330 W/m2

This is not enough of a difference to lead to a change in seasons

Gravity (cont.) / Night Sky / Seasons

1/23/07


The seasons are caused by the tilt of earth s axis of rotation

The seasons are caused by the tilt of Earth’s axis of rotation

  • The Earth’s axis of rotation is not perpendicular to the plane of the Earth’s orbit

  • It is tilted about 23½° away from the perpendicular

  • The Earth maintains this tilt as it orbits the Sun, with the Earth’s north pole pointing toward the north celestial pole

Gravity (cont.) / Night Sky / Seasons

1/23/07


Newton s universal law of gravitation and planetary orbits

Gravity (cont.) / Night Sky / Seasons

1/23/07


Newton s universal law of gravitation and planetary orbits

Gravity (cont.) / Night Sky / Seasons

1/23/07


Newton s universal law of gravitation and planetary orbits

  • In Tucson, when the Sun at its highest point in the sky on Dec 21 (the winter solstice) is at an angle of 35 degrees above the horizon

    • Solar flux absorbed by Earth per square meter = 450 W/m2

  • In Tucson, when the Sun at its highest point in the sky on June 21 (the summer solstice) is at an angle of 82 above the horizon

    • Solar flux absorbed by Earth per square meter = 1350 W/m2

  • Thus, by far, the angle of incidence is the most important factor in leading to a change in seasons on Earth

Gravity (cont.) / Night Sky / Seasons

1/23/07


Newton s universal law of gravitation and planetary orbits

  • Reading Assignment:

    • Please read the textbook discussions of the following topics (this is in Chapter 2) as they will not be covered in lectures

      • Celestial Coordinates

        • Right Asscension

        • Declination

      • Zenith and Meridian

      • Solstices and Equinoxes

Stonehenge, England

Sun Dagger, Chaco, NM

Gravity (cont.) / Night Sky / Seasons

1/23/07


Reading for next class

Reading for next class

  • Chapter 3

    • pp. 42-55

  • Also, re-read section 4-2 and box 4-2 (pages 65-69).

Gravity (cont.) / Night Sky / Seasons

1/23/07


Additional slides

Additional slides

Gravity (cont.) / Night Sky / Seasons

1/23/07


Precession

Precession

  • The Earth precesses as it rotates on its axis, much like a top

  • Has a period of about 19,000 years

  • Causes the “pole” star to change

Gravity (cont.) / Night Sky / Seasons

1/23/07


What is the north star

What is the North Star?

  • Polaris -- for now, but it wont be forever!

  • Vega will be the pole star in about 14,000 years

Gravity (cont.) / Night Sky / Seasons

1/23/07


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