Other Flashcards

1
Q

Where is space?

A

Over 80 km according to US air force, 100 km according to everyone else

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2
Q

Why is SOFIA expensive?

A

Many people needed to operate it, ~400

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3
Q

Phases of a space project

A
  • Scientific idea
  • Scientific objectives
  • Scientific requirements
  • Technical solutions
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4
Q

The Space mission Analysis and Design Process

A

Define objectives
Characterize the mission
Evaluate the mission
Define requirements

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5
Q

Define Objectives

A
  1. Define broad objectives and constraints (broad brush strokes)
  2. Estimate quantative mission needs and requirements
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6
Q

Characterize the mission

A
  1. Define alternate mission concepts (what do you want it to do?)
  2. Define alternate mission architectures (how will it do it?)
  3. Identify system drivers for each (performance and cost drivers, e.g. number of satellites, orbit, size)
  4. Characterize mission concepts/architectures
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7
Q

Evaluate the mission

A
  1. Identify drivin requirements
  2. Evaluate mission utililty
  3. Define mission concecp (baseline)
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8
Q

Define requirements

A
  1. Define system requirements

2. Allocate requirements to system elements

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9
Q

What objects are in LEO?

A

Space shuttle, ISS, HST, Iridium, Remoste sensing, military

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10
Q

Waht objects are in MEO?

A

GPS, Galileo

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11
Q

What objects are in GEO?

A

Meteorology, communication

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12
Q

What do we call the amplitude of RV motion?

A

K

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13
Q

What can we do with the K from RV?

A

K = (2 pi G /P) ^(1/3) m_p sin(i) m_s^(-2/3) *1/(sqrt(1-e^2)) = (2piaM_p sin(i))/((M_p+M_s) P sqrt(1-e^2)

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14
Q

V_rad in terms of K?

A

V_rad = V_0,z + K[cos(theta(t)+omega_op)+e cos(omega_op)]

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15
Q

velocity of the star?

A

v_star = M_p/(m_p+M_s) *v_p

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16
Q

Transit equation

A

Delta F/F = (R_p/R_s)^2

17
Q

Where do error bars on planet measurements mostly come from?

A

Stellar uncertainties

18
Q

Stellar mass-radius relation

A

R=M^(0.8)

19
Q

Conditions for transits:

A

1 Eclipses have flat bottoms, or the planet is fully superimposed on the star
2 There are at least 2 consecutive eclipses to determine period