2. Colorado Space Grant Consortium Gateway To Space ASEN / ASTR 2500 Class #15 Gateway To Space ASEN / ASTR 2500 Class #15

3. Colorado Space Grant Consortium Gateway To Space ASEN 1400 / ASTR 2500 Class #19 Gateway To Space ASEN 1400 / ASTR 2500 Class #19 T-32

4. -Announcements -Mid Semester Team Evaluations - Orbits and Mission Design – Part I -Launch is in 32 days Today:

5. 4 Announcements… Grades - Don’t panic Spider? DD Rev A/B Comments -Mission sections should read like a science paper - Cooler test should be fully functional + Dry Ice Bombs - Mission Statements + RFP - Requirement Section – Team #1 - Testing Section – Team #4 - Hardware Section – Team #6

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18. 17 Mid Semester Team Evaluations… - Due at the start of class on Thursday - Team of six has 1200 points 200 Total = 1200 points

19. 18 Mid Semester Team Evaluations… - Say not everyone is pulling their weight 200 350 50 150 300 Total = 1200 points

20. 19 Mid Semester Team Evaluations… - I take everyone’s scores and do the math, taking into account how self scoring compares to team score for you 200 35075 150 250 350 200 300 150 300 350 400 350 300 25 50 400 150 200 150 200

21. Colorado Space Grant Consortium Thursday… Orbits and Mission Design – PART II Mid Semester Team Evaluations due in class 30 days to launch Thursday… Orbits and Mission Design – PART II Mid Semester Team Evaluations due in class 30 days to launch

22. Colorado Space Grant Consortium Next Tuesday… Guest Lecture on ADCS Next Tuesday… Guest Lecture on ADCS

23. Colorado Space Grant Consortium Orbits and Mission Design – Part 1 ASEN 1400 / ASTR 2500 Class #19 Orbits and Mission Design – Part 1 ASEN 1400 / ASTR 2500 Class #19

24. Orbits: A Brief Historical Look

25. Earth, the Moon, Mars, and the Stars Beyond A Brief Discussion on Mission Design

26. Questions: How fast can you throw a snowball? - A baseball? - A shot put? - A Subway sandwich out a moving car? Could you throw any of these in to an orbit? - How fast would it have to be going?

27. Universal Gravitation, Applied: What is an orbit?

28. Questions: Let’s figure it out… v is velocity G is Universal Gravitational Constant M is mass of planet or satellite R is radius of planet of satellite

29. Universal Gravitation, Applied: When in space why do you float? i.e. Weightlessness

30. Orbit History: 1665 A.D. Isaac Newton At 23, plague while at Cambridge Went to be one with nature He studied gravity Discovered “Newton’s Laws of Motion” 1666, he understood planetary motion Did zip for 20 years until Edmund Halley

31. Newton’s Laws: 1st Law..... Body at rest stays at rest, a body in motion stay in motion 2nd Law.... F = m * a 3rd Law... For every action, there is an equal and opposite reaction

32. Newton’s Laws: Newton Continued... 1687, Principia Published Law of Universal Gravitation (Attraction)

33. Newton’s Laws: Newton Continued... 1687, Principia Published Law of Universal Gravitation (Attraction)

34. Universal Gravitation, Applied: When in space why do you float? i.e. Weightlessness

35. Questions: Let’s figure it out… v is velocity G is Universal Gravitational Constant M is mass of planet or satellite R is radius of planet of satellite

36. Atmosphere: How about throwing something into orbit on the moon? golf ball

37. Atmosphere: Let’s figure it out… v is velocity G is Universal Gravitational Constant M is mass of planet or satellite R is radius of planet of satellite

38. Orbits: A Brief Historical Look Arthur C. Clarke Discovered This Orbit

39. Ancient Orbit History: “ORBIT” from Latin word “orbita” orbitus = circular; orbis = orb 1800 B.C. Stonehenge - Study of the vernal equinox

40. 1500 B.C.: Egyptians and Babylonians Written evidence of stellar observations Solar Calendar of 365 days Time divided into 60 even units

41. Aristotle Said earth is center of the universe Dominated scientific thought for 1800 years 350 B.C.: Greek Thoughts

42. Start of the Heliocentric Model: 1543 A.D. Nicholas Copernicus Said Sun-centered rotations Measurements crude but thinking shifts Didn’t release findings until the end of his life

43. Orbit History : 1580 A.D. Tycho Brahe Accurate measurements of planets (Mars) as a function of time Even though telescope had not been invented

44. Orbit History : 1610 A.D. Galileo Galilei Good friends with Copernicus Observations with TELESCOPE reinforced Discovered Venus has phases

45. Orbit History: 1600 A.D. Johannes Kepler Used Tycho’s careful Mars observations to smash Aristotle theories Presented 3 laws of planetary motion Basis of understanding of spacecraft motion However, “Why was not understood” Calculus?

46. 45 One Minute Report… - Gottfried Leibniz Isaac Newton

47. Orbit History: Kepler’s 3 Laws of Planetary Motion: 1.All planets move in elliptical orbits, sun at one focus

48. Orbit History: Kepler’s 3 Laws of Planetary Motion: 1.All planets move in elliptical orbits, sun at one focus

49. Orbit History: Kepler’s 3 Laws of Planetary Motion: 2.A line joining any planet to the sun, sweeps out equal areas in equal times

50. Orbit History: Kepler’s 3 Laws of Planetary Motion: 2.A line joining any planet to the sun, sweeps out equal areas in equal times

51. Orbit History: Kepler’s 3 Laws of Planetary Motion: 3.The square of the period of any planet about the sun is proportional to the cube of the of the planet’s mean distance from the sun. If you can observe the period of rotation, you can determine the distance PlanetP (yr)a (AU)T2T2 R3R3 Mercury0.240.390.06 Venus0.620.720.390.37 Earth1.00 Mars1.881.523.533.51 Jupiter11.95.20142141 Saturn29.59.54870868 T 2 = R 3

52. Types of Orbits: Orbits are conic sections: Circle Ellipse Parabola Hyperbola From Kepler’s Law, the central body is at a focus of the conic section

53. Kepler: Kepler’s Laws...Orbits described by conic sections Velocity of an orbit described by following equation For a circle (a=r): For a ellipse (a>0): For a parabola (a=  ):

54. Questions: Let’s figure it out… v is velocity G is Universal Gravitational Constant M is mass of planet or satellite R is radius of planet of satellite

55. Earth, the Moon, Mars, and the Stars Beyond A Brief Discussion on Mission Design

56. Orbit Introduction: What is an orbit? - The path of a satellite around the Earth (or any central body) What shape is it? - Orbits are conic sections - Circles, Ellipses, Parabolas, Hyperbolas How are orbits described? - Position and Velocity at any one time - Keplerian Elements (from Kepler’s Laws)

57. Orbit Definition: Velocity & Position - Given position and velocity of a satellite at time t, you can calculate the position and velocity at any other time

58. Orbit Definition: Keplerian Elements - Semi major axis (a) - Size - Eccentricity (e) - Shape

59. Orbit Definition: Keplerian Elements - Inclination (i) - Angle to the Equator

60. Orbit Definition:

61. Keplerian Elements - Right Ascension of Ascending Node (RAAN, Ω) - Rotation about the Earth’s Spin Axis

62. Orbit Definition: Keplerian Elements - Argument of Perigee (ω) - Rotation of the conic section in the plane

63. Orbit Definition: Keplerian Elements - True Anomaly (θ) - Defines the position of a body in orbit - Angle between the Position Vector and the vector to Perigee - Elliptical only

64. Orbital Elements: Used to determine a satellite’s location in orbit:

65. Types of Orbits:

67. Types of Orbits (cont.) Geosynchronous/Geostationary (equator)

68. Types of Orbits (cont.) Critical Inclination

69. Types of Orbits (cont.) Repeating Ground Trace

70. Polar/ Sun Synchronous Types of Orbits (cont.)

71. Molniya