Space P

Tu Dresden

Tu Dresden


H. D.
Diese Karteikarten bieten einen umfassenden Überblick über die Technologien und Prinzipien der Raumfahrttechnik auf Universitätsniveau. Sie behandeln Themen wie Brennstoffzellen, Halbleiter, thermoelektrische Generatoren, Strahlung und Kernreaktionen, wobei der Fokus auf der Energieerzeugung und -umwandlung liegt. Besonders relevant sind die Anwendungen in Raumfahrtsystemen, wie die Nutzung von Radioisotopen-Thermoelektrischen Generatoren (RTGs) und die Abschirmung von Strahlung. Diese Karteikarten sind ideal für Studierende und Forscher, die sich mit den technischen Aspekten der Raumfahrt und Energieversorgung in extremen Umgebungen beschäftigen.
Flashcards
115
Students
2
Language
German
Category
Technology
Level
University
Created / Updated
13.02.2021 / 04.03.2021

Flashcards

Power distribution unit

Power regulation & distribution function

Regulate the bus voltage to the required voltage level

- Regulate the power output (voltage and current) from solar cells and energy storage systems

- Regulate the voltages during charging of energy storage systems

Provide direct current (DC)or alternating current (AC)

pro cons DC / AC

DC

Low power demands

Low transmission distances

 

AC

High power demands

High transmission distances

 

Batteries, fuel cells, solar cellsproduce direct current(DC)

Power conditioning & control - 2 types

PPT - explanation

When a load is directly connected to the solar panel, the operating point of the panel will rarely be at peak power. The impedance seen by the panel determines the operating point of the solar panel. Thus by varying the impedance seen by the panel, the operating point can be moved towards peak power point. Since panels are DC devices, DC-DC converters must be utilized to transform the impedance of one circuit (source) to the other circuit (load). Changing the duty ratio of the DC-DC converter results in an impedance change as seen by the panel. At a particular impedance (i.e. duty ratio) the operating point will be at the peak power transfer point. The I-V curve of the panel can vary considerably with variation in atmospheric conditions such as irradiance and temperature. Therefore, it is not feasible to fix the duty ratio with such dynamically changing operating conditions.

Full energy source overview

ISS m2 of solar and power

3000 m² - 250 kW

photo efficiency lab vs final

which photocell types are primarily used in space

photo Environmental impacts on maximum power

RTG working principle

RTG:

+ / -

Power <1kW

+

-Independence of power production from S/C orientation

-Independence of the distance to the Sun -> deep space missions are possible

-Suitable for mission with long eclipse period (lunar landers, etc.)

-No storage required for shadow eclipse

 

-

-Adversely effect the radiation environment of the S/C -> RTG needs to be deployed on a boom away from the S/C bus

-Careful handling procedures during S/C integration (radioactive source!)

-Potential of dispersing in the atmosphere in case of launch failure

 

 

“The Safety analysis report prepared for the US energy department came to the conclusion that the risks are extremely small and well understood. It‘s much more likely someone will be injured driving a car to protest a RTG launch than in an RTG dispersion accident.”

working principle nuclear reactors

nuclear reactors + /-

Primary batteries

lithium ion - 100 - 265 Wh /kg

Fuel cells (FC)

Energy storage overview

overview iss

k

Why do low-earth orbit S/C need more total battery capacity, meaning more batteries versus those in geostationary orbit for the same energy to be stored.

whats DOD

DOD - 10 years; 1000 Wh; 60 Wh/kh --> calculate battery mass LEO/ GEO

5 secondary batteries

NiCd

NiH2

LiIon

NiMH

Li-poly

Properties NiCd

-Exhibits memory effect,

-Environmental concerns (Cd)

-Extensively used till mid-1980s

 

28-32 Wh/ kg

properties NiH2

-No memory effect,

-Highly reliable operation

 

35-65 Wh/kg

-Extensively used since mid-1980s

properties LiIon

Very sensitive to over-charge and over discharge, -> Needs complex charge control for high number of single cells

-High self-discharging rate @ high temperatures

-Energy density degradation over time independent on use

-Often over 50% degradation after 150 cycles at temperatures <-5°

 

-mission @ low cycle life-temperature problems-small satellites, short mission time

 

70 - 150 Wh

Li-poly

- Performance temperature dependent

-Under evaluation (ESA, ESTEC)

100-200 Wh

Regenerative fuel cell (R-FC)

R-SOFC: Regenerative Solid Oxide Fuel Cell fuel cells (R-FC)

Reversible fuel cell reaction, one unit

generating electricity in fuel cell mode (producing H2O or CO2)

separating water in H2/O2in electrolyze mode -> energy storage!

or: separating Carbon dioxide in CO/O2 -> energy storage & O2production

Tethers for energy storage & propulsion

Flywheels

Flywheels

energy storage final selection properties

low mass, high cycle life, capable of being integrated, autonomy, peak power, capable of discontinuous charging, volume

nuclear vs solar

Mission duration vs. power level

Short term missions:

   -Primary batteries -Fuel cells

Long term missions:

   -Solar photovoltaic systems combined with secondary (rechargeable) batteries for energy storage

Outer-/inner planets:

   -e.g. Radioisotope Thermoelectric Generator (RTG)

Very high power demand

   Nuclear reactor -Solar-dynamic generator (heat?)

 

Hauptaufgabendes EPS

AllgemeineAnforderungenan die Energiequelle

befestigung von solarezellen

1) Körperfestes Solarpanel

2) Drehbar gelagertes Solarpanelàα-/ β -Drehung

3) externe Flächen der Satellitenstruktur (“Body / Panel mounted”)

Abschätzung: Spannungsebene

Nukleonteilchen + ablürzungen

Proton Z - m_z

Neutron N - m_n

 

sum m_Z + sum m_n > m (z, n)

-> dE

wann ist eher kernzerfall?

wenn mehr protononen da sind

 

Auch: kerne sind stabiler wenn mehr neutronen als protonen da sind  (große kernzahlen -> vorher linear)

x achse neutronen

z achse protonen

-> rot stabiler

 

 

Stabil? mangel an neutronen / überschuss an neutronen?

Heliumkern?

2 protonen

2 neutronen

Aufbau RTG

gefahr bei zerfall entsteht gas -> steiogender druck -> muss für die ganze laufzeit ausgelegt sein

Wann nutzt man RTGs

Study