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1. Space Environment
Lecture 4 β Effects on spacecraft
Atomic Oxygen & atmospheric drag
Professor Hugh Lewis
SESA3038 Space Environment
2. Overview of lecture 4
β’ In this lecture we will complete our high-level look at the key
characteristics of the space environment and their effects on spacecraft,
with a focus here on:
β Atomic Oxygen and how it can affect the drag coefficient
β Thus playing a role in the drag force experienced by spacecraft (and
recalling SESA2024 Astronautics, the rate at which spacecraft orbits
will decay)
β The importance of Atomic Oxygen is such that we will see it again when
we look at the geospace climate, where it plays a crucial role in global
geospace climate change
Space Environment β Environmental effects
3. Environmental effects
β’ High vacuum
β’ Solar radiation
β’ Particle radiation
β’ Atomic Oxygen
Space Environment β Environmental effects
4. Atomic Oxygen reaction & erosion Space Environment β Environmental effects
β’ Can affect spacecraft drag indirectly by affecting material properties:
Reminder: principal effects of drag upon the orbit are to reduce its size and to
circularise it (both semi-major axis, a, and eccentricity, e, decrease)
Original orbit
Successive orbits
Earthβs
atmosphere
5. Drag force (an aside) Space Environment β Environmental effects
β’ Drag force acting is:
β Where: ππ = atmospheric density
ππππ = velocity relative to atmosphere
ππ = reference area (area perpendicular to ππππ)
πΆπΆπ·π· = drag coefficient
β Value of πΆπΆπ·π· ~ 2 to 4 depending on gas-surface interaction (this is what
Atomic Oxygen changes)
ππ =
1
2
πππππΆπΆπ·π·ππ
ππ
2
βοΏ½
ππππ
6. Drag force (an aside) Space Environment β Environmental effects
β’ For LEO spacecraft, particles are:
β’ Incident at ππππ β 7 km/s
β’ Accommodated for a short interval (this is where Atomic Oxygen plays a role)
β’ Re-emitted at thermal velocity πππ‘π‘π‘ β 2 km/s
β’ Estimate of value of πΆπΆπ·π·:
β’ Assume ππ
ππ β« Vπ‘π‘π‘~0
β’ Let ππ be velocity of particles relative to spacecraft (ππ = βππππ)
7. Drag force (an aside) Space Environment β Environmental effects
β’ Estimate of value of πΆπΆπ·π·:
β’ The incident momentum per unit of time on
surface S is:
β’ The reflected momentum is: ππππππππππππ = 0
β’ Therefore the force on surface S is the change
of momentum in unit time:
ππππππππππ = ππ ππππ ππ = ππππ2
πποΏ½
ππ
π π = β ππππ = ππππππππππ β ππππππππππππ = ππππππππππ
S
8. Drag force (an aside) Space Environment β Environmental effects
β’ Estimate of value of πΆπΆπ·π·:
β’ Therefore the force on surface S is the change
of momentum in unit time:
β’ And:
β’ Hence:
π π = β ππππ = ππππππππππ β ππππππππππππ = ππππππππππ
= ππππ2
πποΏ½
ππ
S
π π β‘ ππ =
1
2
ππππ
ππ
2
πππΆπΆπ·π· βοΏ½
ππππ
ππππ2
πποΏ½
ππ = ππ =
1
2
ππππ2
πππΆπΆπ·π·
οΏ½
ππ
9. Drag force (an aside) Space Environment β Environmental effects
β’ Estimate of value of πΆπΆπ·π·:
β’ Hence:
β’ Recall that this is if particles βstickβ to the
spacecraft surface (Vπ‘π‘π‘~0)
S
ππππ2
πποΏ½
ππ = ππ =
1
2
ππππ2
πππΆπΆπ·π·
οΏ½
ππ
πΆπΆπ·π· = 2
10. Drag force (an aside) Space Environment β Environmental effects
β’ Estimate of value of πΆπΆπ·π·:
β’ Assume particles are specularly reflected Vπ‘π‘π‘ = βππ
ππ
β’ Again, let ππ be velocity of particles relative to spacecraft (ππ = βππππ)
β’ The reflected momentum is now: ππππππππππππ = βππππ = βππππ2
πποΏ½
ππ
β’ The force on surface S (the change of momentum in unit time) is now:
π π = β ππππ = ππππππππππ β ππππππππππππ
= ππππ2
πποΏ½
ππ β βππππ2
ππ οΏ½
ππ
= 2ππππ2
πποΏ½
ππ
S
11. Drag force (an aside) Space Environment β Environmental effects
β’ Estimate of value of πΆπΆπ·π·:
β’ Hence:
β’ Recall that this is if particles do not βstickβ to the spacecraft surface at all
(Vπ‘π‘π‘ = βππ
ππ)
β’ The βstickinessβ of the spacecraft surface is characterised using an
accommodation coefficient that depends on the material properties
β’ Atomic Oxygen changes the material properties
S
2ππππ2
πποΏ½
ππ = ππ =
1
2
ππππ2
πππΆπΆπ·π·
οΏ½
ππ
πΆπΆπ·π· = 4
12. Atomic Oxygen erosion Space Environment β Environmental effects
β’ Some materials are unacceptable for long-duration use in LEO
spacecraft. Selection of protective mechanism based on:
β’ Resistant to AO attack
β’ Thin, light weight and adhere strongly to base material
β’ Free from defects, pores and scratches
β’ Non-contaminating
β’ Should not alter basic properties of the base material
β’ Should withstand ground handling, manufacturing loads and orbit loads
β’ Stable in LEO space environment:
β Particulate radiation
β UV radiation
β Micrometeoroids and orbital debris
β Thermal cycling
β Charging
13. Recap of lectures 2 to 4
β’ In these lectures we took a high-level look at the key characteristics of the
space environment and their effects on spacecraft:
β High vacuum
β Solar radiation
β Particle radiation
β Atomic Oxygen, including how it affects the drag coefficient
β The drag coefficient is partly determined by the spacecraft materials,
Atomic Oxygen changes the properties of these materials, thereby
affecting, indirectly, the drag coefficient
β We will see Atomic Oxygen again when we discuss the geospace climate,
where it plays a crucial role in global geospace climate change
β’ In our next lectures we will look at the effects of the space environment on
humans
Space Environment β Environmental effects
14. Activity
β’ A reminder that you can read the βSpacecraft
Environment and its effect on designβ chapter
in Fortescue, Stark & Swinerd:
β’ Read this chapter (pages 11-47) to support your
learning of this topic (and those to come)
β’ Access to the e-book is available via the Library
website:
https://onlinelibrary.wiley.com/doi/book/10.1002/9
781119971009
Space Environment β Environmental effects