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Ion Thruster - Propellant
Xenon is the preferred choice because it is heavy (momentum), inert (won't corrode), and easy to store
Ion Thruster - Specific Impulse ($I_{sp}$)
The "fuel economy" of a rocket
Ion Thruster - Why use them?
Ideal for long-duration missions requiring massive velocity changes ($\Delta v$) where chemical fuel would be too heavy
Ion Thruster - Thrust Level
Very low (comparable to the weight of a piece of paper)
Sample Collection - Microgravity Difficulty
Applying any force (drilling/scooping) creates an equal and opposite reaction that pushes the spacecraft away
Sample Collection - Regolith Behavior
In a vacuum, asteroid dust can behave like a fluid or stick to surfaces due to static electricity
Sample Collection - Signal Latency
Real-time control is impossible due to light-speed delay
RTG (Radioisotope Thermoelectric Generator)
Power source for deep space missions (Voyager, Cassini, New Horizons) that converts heat from decaying Plutonium-238 into electricity via the Seebeck Effect
Gravity Assist (Slingshot)
Using a planet’s orbital momentum to accelerate or decelerate a spacecraft without using fuel
Lagrange Point 2 (L2)
A gravitational "parking spot" 1
5 million km from Earth where JWST stays, keeping the Sun, Earth, and Moon all on one side
Interferometry
The technique of combining signals from multiple telescopes (like ALMA) to act as one giant "virtual" telescope
The "Vault" Concept
Used by Juno
White Ceramic Fiber
Thermal insulation used by BepiColombo to survive the 450°C heat at Mercury
Mission Specifics: BepiColomboBepiColombo - Lead Agencies
Joint mission between ESA (Europe) and JAXA (Japan)
BepiColombo - MPO (Mercury Planetary Orbiter)
The European component focused on mapping the surface and internal composition
BepiColombo - MMO (Mercury Magnetospheric Orbiter)
The Japanese component (Mio) focused on Mercury’s magnetic field
BepiColombo - MOSIF
The sunshield that protects the MMO during the long cruise to Mercury
BepiColombo - Why Mercury is hard
The Sun’s gravity pulls the craft in
Mission Specifics: Galileo & JunoGalileo - Major Discovery
Found strong evidence of a subsurface saltwater ocean on the moon Europa
Galileo - Failure
The High-Gain Antenna (HGA) failed to unfurl
Galileo - Atmospheric Probe
First mission to drop a probe directly into a gas giant's atmosphere
Juno - Primary Goal
To understand Jupiter's origin and evolution by mapping its gravity and magnetic fields
Juno - Core Discovery
Revealed Jupiter has a "dilute" or "fuzzy" core rather than a solid rocky one
Juno - MWR (Microwave Radiometer)
An instrument that "sees" through Jupiter's clouds to measure water and ammonia
Juno - Orbit Type
Polar orbit
Mission Specifics: Cassini & VoyagerCassini - Huygens Probe
An ESA-built probe that landed on Titan, revealing methane lakes and a thick atmosphere
Cassini - Enceladus Discovery
Discovered water-ice plumes erupting from "tiger stripes" at the south pole, indicating a subsurface ocean
Cassini - VIMS
Visual and Infrared Mapping Spectrometer used to map the chemical composition of Saturn's moons
Cassini - Grand Finale
The end-of-mission maneuver where Cassini dove between Saturn and its rings before burning up in the atmosphere
Voyager 2 - Unique Achievement
The only spacecraft to have visited all four outer giant planets (Jupiter, Saturn, Uranus, Neptune)
Voyager 2 - Triton Discovery
Discovered active geysers on Neptune’s moon Triton
Voyager 2 - Interstellar Space
The region it entered where the Sun’s solar wind is replaced by the wind of the galaxy
Mission Specifics: New Horizons & DawnNew Horizons - Pluto Discovery
Found "Sputnik Planitia," a giant heart-shaped glacier of nitrogen ice
New Horizons - LORRI
Long Range Reconnaissance Imager
New Horizons - Power Source
A single RTG, because at Pluto (30+ AU), sunlight is 1000x dimmer than on Earth
Dawn - Main Targets
The "protoplanets" Vesta (rocky) and Ceres (icy/water-rich)
Dawn - Ceres Discovery
Found "faculae" (bright salt spots) in Occator Crater, suggesting recent brine activity
Dawn - Engineering First
The first spacecraft to orbit two different extraterrestrial targets
Mission Specifics: LRO, Hayabusa, Deep ImpactLRO - LOLA
Lunar Orbiter Laser Altimeter
LRO - PSRs
Permanently Shadowed Regions
LRO - LAMP
Lyman-Alpha Mapping Project
Hayabusa - Target
The near-Earth asteroid Itokawa
Hayabusa - Sampler Mechanism
Fired a tantalum bullet into the surface to kick up dust into a collection horn
Deep Impact - Smart Impactor
A 370kg copper slug used to crash into Comet Tempel 1
Deep Impact - Why Copper?
Copper is "spectrally clean"—it doesn't have absorption lines that interfere with the comet's chemistry data
Deep Impact - Discovery
Proved comets are "fluffy" (mostly empty space) rather than solid ice
Mission Specifics: ALMA, Hubble, JWSTALMA - Location
Chajnantor Plateau in the Atacama Desert, Chile, at 5,000 meters altitude
ALMA - Why Altitude?
Millimeter waves are absorbed by water vapor
ALMA - Science Goal
Observing the "Cold Universe," specifically the gas disks where planets are born
Hubble - COSTAR
The corrective optics "glasses" installed by astronauts to fix Hubble’s blurry mirror (spherical aberration)
Hubble - WFC3
Wide Field Camera 3
JWST - Golden Mirrors
Gold is used because it has 99% reflectivity for infrared light
JWST - Sunshield Material
Five layers of Kapton, each the size of a tennis court
JWST - MIRI (Mid-Infrared Instrument)
Needs an extra "cryocooler" to stay at 7 Kelvin to detect faint heat signals
JWST - Main Science Goal
To see "First Light"—the very first stars and galaxies formed after the Big Bang