1 / 21

Bit of Administration ….

Bit of Administration …. Lab 2 New observation dates: March 22 - April 5 No need to duplicate observations in hand! New due date: April 9 at my office Homework Reading BSNV pp. 153 - 168 No office hours today Feel free to e-mail for later in week. Astronautics. Interplanetary Travel

ophira
Télécharger la présentation

Bit of Administration ….

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Bit of Administration …. • Lab 2 • New observation dates: March 22 - April 5 • No need to duplicate observations in hand! • New due date: April 9 at my office • Homework • Reading • BSNV pp. 153 - 168 • No office hours today • Feel free to e-mail for later in week

  2. Astronautics • Interplanetary Travel • The Central Concept … • The paths of interplanetary spacecraft are • simply orbits around the Sun … • And the spacecraft obey the same physical laws • as do planets.

  3. Astronautics • Transfer Orbit = Minimum Launch Energy • Launch in the direction of motion of the launch platform. • Arrive at destination at aphelion ( for outer target) or • perihelion (for inner target) of spacecraft orbit. • (Aphelion - point of orbit most distant from Sun • Perihelion - point of orbit closest to Sun)

  4. Transfer Orbit for the Moon

  5. Astronautics • Transfer Orbit = Minimum Launch Energy • Launch in the direction of motion of the launch platform. • Arrive at destination at aphelion ( for outer target) or • perihelion (for inner target) of spacecraft orbit. • (Aphelion - point of orbit most distant from Sun • Perihelion - point of orbit closest to Sun) • Advantages - Fuel efficiency • Disadvantages - Long travel time

  6. Astronautics • Gravity Boosts • Gain in energy due to gravitational “slingshot” around • a more massive body. • Note: More massive body loses energy, but in case of • planet and spacecraft this is not a problem!

  7. Astronautics • Gravity Boosts but Jupiter is moving … In frame of Jupiter In frame of Solar System

  8. Astronautics • Gravity Boosts - NASA missions

  9. The Physics of Light • Light as a Wave = Electromagnetic Radiation • Wavelength (l) has units of length • Frequency (n) - number of crests passing per second • - has units of cycles per second, or Hertz • Speed - for light, c = 3x105 km/sec 3 x 105 km/sec Wavelength

  10. The Physics of Light • Light as a Wave = Electromagnetic Radiation • Wavelength (l) has units of length • Frequency (n) - number of crests per second • Speed - for light, c = 3x105 km/sec Small wavelength Large frequency Large wavelength Small frequency

  11. The Physics of Light • Light as a Wave = Electromagnetic Radiation • Wavelength (l) has units of length • Frequency (n) - number of crests passing per second • - has units of cycles per second, or Hertz • Speed - for light, c = 3x105 km/sec

  12. The Physics of Light • Electromagnetic • Spectrum 1 km = 1000 m 1 m 1 mm = 0.001 m = 10-3 m 1 mm = 10-6 m (“micron”) 1 nm = 10-9 m (nanometer)

  13. - - - - - - - - - - - - - - S S S S S S N N N N N N N N N N N N S S S S S S The Physics of Light • Electromagnetic Radiation • Light acts as an electric force • Light acts as a magnetic force

  14. - - - - - - - - - The Physics of Light • Electromagnetic Radiation Antenna

  15. The Physics of Light • Doppler Shift

  16. The Physics of Light • Doppler Shift • Source moving toward observer or • observer moving toward light source Shorter Wavelength Higher Frequency Blueshift • Light source moving away from observer or • observer moving away from light source Longer Wavelength Lower Frequency Redshift

  17. The Physics of Light • Doppler Shift • Source across observer’s line of sight Same Wavelength as emitted Same Frequency as emitted No Shift

  18. The Physics of Light • Doppler Shift v = velocity of light source or observer (+ => toward each other) l = rest wavelength Dl = change (shift) in wavelength c = 3 x 105 km/sec

More Related