Spacecraft Structure Requirements –Mass, Strength, Stiffness, Cleanliness (Particulate/Magnetic) Constraints –Fields of view (instruments, thrusters, motors)

Slides:



Advertisements
Similar presentations
Distances in the Universe and Space Travel
Advertisements

ACTIVITY ON THE SUN: Prominences Sunspots Solar Flares CME’s – Coronal Mass Ejections Solar Wind Space Weather.
Chapter 2 The Solar System. Solar System Comprised of Sun Inner Terrestrial Planets (Mercury, Venus, Earth, Mars) Main Asteroid Belt Outer Gas Giants.
The second exam is this Thursday. It will cover everything we have covered from since the first exam (until the end of class today). There will be a review.
Space Weather. Coronal loops Intense magnetic field lines trap plasma main_TRACE_loop_arcade_lg.jpg.
Review Vocabulary magnetic field: the portion of space near a magnetic or current-carrying body where magnetic forces can be detected The Sun contains.
Attitude Determination and Control
Danish Space Research Institute Danish Small Satellite Programme FH Space_Environment.ppt Slide # 1 Flemming Hansen MScEE, PhD Technology Manager.
SPACE WEATHER Definition used by the US National Space Weather Plan: Conditions on the Sun and the solar wind, magnetosphere, ionosphere, and thermosphere.
1 L 27 Electricity & Magnetism [5] Magnets –permanent magnets –Electromagnets –The Earth’s magnetic field magnetic forces applications Magnetism.
The sun and our solar system Grade 9 Science Space Part 2.
S/C System Design Overview Robert G. Melton Department of Aerospace Engineering.
What are the four inner planets?. Mercury, Venus, Earth, and Mars.
Stratosphere Troposphere
Student Satellite Project University of Arizona Team Goals Design, Fabricate, and Analyze a Structure that will Support the Payload –Space Allocation of.
Note key, please leave in binder. Our Sun
Spacecraft Instruments. ► Spacecraft instrument selection begins with the mission description and the selected primary and secondary mission objectives.
The Sun and the Heliosphere: some basic concepts…
Our Sun A medium sized star. Our Sun Our sun is a typical medium sized star. A star is a hot ball of plasma that shines because nuclear fusion is taking.
Sponge: List the six layers of the Earth.. Atmosphere A mixture of gases: N 2 78% O 2 21% Ar0.9% CO %
NEEP 541 Radiation Interactions Fall 2003 Jake Blanchard.
Space Environment Neutral Environment Hydrogen
The Sun Internal structure of the Sun Nuclear fusion –Protons, neutrons, electrons, neutrinos –Fusion reactions –Lifetime of the Sun Transport of energy.
Space Weather: What is it? How Will it Affect You? An introduction to Space Weather What is it? Where does it come from? What does it do? Rodney Viereck.
Our second exam is next Tuesday – Nov 1. It will cover everything I have covered in class including material covered today. You will be allowed one 8 ½.
The Sun By: Kristel Curameng and Courtney Lee. The Sun The Sun is the most prominent feature in our solar system. The largest object and contains approximately.
By Miss O..  Remember “ solar ” means “things having to do with the sun (in Latin).
Is There Life Out There? Our Solar System (and beyond) Draw a picture of what you think life would look like on another planet, if it existed. Describe.
Space Radiation and Fox Satellites 2011 Space Symposium AMSAT Fox.
Space Research Institute Graz Austrian Academy of Sciences CERN, Geneve, June 2006 Helmut O. Rucker Exploring the Planets and Moons in our Solar System.
Forces between electric charges in motion.
Sun, Moon, Earth, How do they work together to help life survive? Magnetosphere.
Charged Particle Trajectories in Earth’s Magnetic Field Sarah Arveson.
The Sun. Components of the Sun Core Radiative zone Convective zone Atmosphere –Photosphere –Chromosphere –Corona Solar wind (mass loss)
Solar Wind and Coronal Mass Ejections
The Sun.
Objectives Describe the layers and features of the Sun. Explain the process of energy production in the Sun. Define the three types of spectra. The Sun.
By Elisha. » The Sun » The sun is the star in the centre of the solar system in which the earth orbits around and is about 149,600,000 km away from earth.
GEOL3045: Planetary Geology Lysa Chizmadia The Sun & Ulysses Lysa Chizmadia The Sun & Ulysses.
A Transitional Fossil 375 Ma fish: flat nose, beginnings of limbs “Missing link” between fish and life on land.
THE SUN. The Sun The sun has a diameter of 900,000 miles (>100 Earths could fit across it) >1 million Earths could fit inside it. The sun is composed.
Space Environment September 30,2003 H. Kirkici Istanbul Technical University Lecture-4 Solar Physics it is a star has a radius of about 696,000 km composed.
Space Environment SSE-120 Please type in your questions and raise your hand so we can answer it during class.
AURORAS Aurora borealis (northern lights) Aurora australis (southern lights) Beautiful, dynamic, light displays seen in the night sky in the northern.
Magnetic Earth Chapter 1 Section 3 Pages Objective: Understand the Earth’s magnetic field and Compare magnetic and geographic poles. Compass:
The Sun Distance from Earth: 150 million km OR 93 million miles Size: 1.4 million km in diameter Age: 4.5 billion years old, halfway through its 10 billion.
Cosmic Rays2 The Origin of Cosmic Rays and Geomagnetic Effects.
Topics in Space Weather Earth Atmosphere & Ionosphere
Lesson 2.  At the center of our solar system is the Sun which is a typical medium sized star.  Composed mainly of Hydrogen (73% by mass), 23% helium.
Unit 8 Chapter 29 The Sun. We used to think that our sun was a ball of fire in the sky. Looking at our sun unaided will cause blindness. The Sun’s Energy.
The Gas Giants. Jupiter Exploration of Jupiter Four large moons of Jupiter discovered by Galileo (and now called the Galilean satellites) Great Red Spot.
© 2009 W.W. Norton Earth Liquid water on its surface Oxygen atmosphere Only planet known to support life 4.6 billion years old 71% covered by H 2 O Oblate.
Magnetic Forces. The Force on a Moving Charge in a Magnetic Field Just as current-carrying wires (a stream of moving charges) experience a force in a.
Reading Unit 31, 32, 51. The Sun The Sun is a huge ball of gas at the center of the solar system –1 million Earths would fit inside it! –Releases the.
The Gas Giants. JupiterSaturnUranusNeptune Mass (M Earth ) Distance from Sun (AU) Equatorial Radius (R Earth )
The Solar Wind. The Sun is not a quiet place. Disturbances in the Sun’s magnetic field create Sunspots.
By Martina Stumpp. Overview I.What are Auroras? II.What causes them? III.Auroral Zone IV.Colors V.Auroras on other planets.
The Sun The SUN Chapter 29 Chapter 29.
Sponge: List the six layers of the Earth.
Reading Unit 31, 32, 51.
L 27 Electricity & Magnetism [5]
Earth’s Magnetic Field ~Magnetosphere
Inside Jupiter and Saturn
Chapter 29-2 Solar Activity.
The Sun The interior of the sun has three layers:
Guided Notes about the Sun
L 27 Electricity & Magnetism [5]
The Sun.
Grades 9-12: Introduction
The Space Environments
Presentation transcript:

Spacecraft Structure Requirements –Mass, Strength, Stiffness, Cleanliness (Particulate/Magnetic) Constraints –Fields of view (instruments, thrusters, motors) –Thermal control –Center of mass –Ratio of moments of inertia –Propulsion lever arm –Constraints of launch vehicle shroud –Constraints of sun and earth vector –Component Collocation –Launch Vehicle Environment (loads, shock, acoustics) Steady state Transient –Random Vibration –Acoustic vibration –Testing

Design Approach Accessibility –Test, Repair Harness and Cables –Routing Standard Approaches? –Attempts at “generic” spacecraft have failed Building blocks –Boxes, Truss (tube), Cylinders, X-agons –Materials: Metals, Honeycomb, Composites

Launch Vehicle

Payload Planners Guide

Spacecraft Spacecraft are generally classified by: –Attitude Control System None Gravity Gradient Spinner Despun (Momentum Biased) 3-Axis Stabilized – Mission they are performing Flyby Orbiter Probe Lander Penetrator

None Sputnik 1957

Gravity Gradient LDEF Deployed on orbit on April 7, 1984 by the Shuttle Challenger. Circular orbit Altitude of 275 nautical miles Inclination of 28.4 degrees. Attitude control of the LDEF spacecraft was achieved with gravity gradient and inertial distribution to maintain three-axis stability in orbit.

Spinner SNOE Circular orbit 580 km altitude degrees inclination sun synchronous precession, 26 Feb

Despun (Momentum Biased) OSO-8 Launched on 21 June km circular orbit 33 degree inclination scanning and pointing mode. spin period was 10.7 seconds. rotating cylindrical base section non-spinning upper section

3-Axis Stabilized TERRA (EOS AM) 12/18/1999

3-Axis Stabilized TERRA (EOS AM) Solar Array

Flyby Voyager 1977 Jupiter Saturn Uranus Neptune

Cassini Orbiter

Prob e

Viking Lander

Space Environment and Effects –Earth Planet Mass Iron Core Atmosphere –Sun Mass Solar Activity –Planets Planet environment Proximity to sun

Spacecraft Systems Computers Batteries Propellant Electronics Instruments Windows Mirrors Mechanisms Detectors

Environment and Effects - Earth Radiation Belts Trapped Protons and Electrons Changing Magnetic Field Atmosphere South Atlantic Anomaly Solar Wind Magnetopause Magnetosphere

Environment and Effects - Sun UV Wavelength Solar Wind CMEs - Protons, Neutrons and X rays

Coronal Mass Ejection

Space Environment from the Spacecraft Perspective Thermal: Solar, IR, S/C Dissipatoin Solar UV Charged Particles – Solar Wind, Sun Materials Outgassing and Contamination Magnetics Spacecraft Charging Atomic Oxygen

Thermal Total radiant-heat energy emitted from a surface is proportional to the fourth power of its absolute temperature. E =  T 4 Direct Solar Exposure Eclipse Orbit transition Changing response of spacecraft Temperature of planet body

Solar UV Flux Short wavelength energy Reactions Changes material properties Optical Properties of Surfaces Glass darkens Polymerize hydrocarbons

Outgassing and Contamination Earth vs Space: Pressure, water, oil, unpolymerized materials Fingerprint Total Mass Loss (TML) <1% Collected Volatile Condensible Materials (CVCM) < 0.1%

Effects of Radiation Single Events Upsets Latchup Long term exposure (Total Dose) Electronics Degredation –Threshold Levels and Timing –Semiconductors – Holes

Magnetic 11  Dipole (bar magnet) Rotating magnetic field Magnetometer Fixed and Changing Fields on Instruments Non-magnetic materials Earth Axis

Spacecraft Charging Spacecraft moving through a plasma Plasma density Debye length Field around spacecraft Photo-electric emission –Photons hit surface, release electrons Insulators on spacecraft surfaces –Near earth ~1-2 volts –10 Earth Radii (10R E ) ~10,000 Volts

Atomic Oxygen In low Earth orbits, satellites encounter the very low density residual atmosphere. At orbital altitudes, this is composed primarily of oxygen in an atomic state. A satellite moves through the atomic oxygen (AO) at a velocity of about 7.5 km/sec. Although the density of AO is relatively low, the flux is high (speed x density x surface area). Highly reactive atomic oxygen can produce serious erosion of surfaces through oxidation. Thermal cycling of surfaces, which go in and out of the earth's shadow frequently in this orbit, can remove the oxidized layer from the surface.

Glow Aurora Australis or Southern Lights, in the km altitude region Charged plasma glow around shuttle Excitation of atomic oxygen in the upper atmosphere by the van Allen Radiation Belts

Radiation Environment Radiation Belts around the Earth Electrons Protons Cosmic Rays

Debris and Micrometeorites Humans Damage to Spacecraft and Systems