Parker Solar Probe
PARKER SOLAR
TOUCHING THE SUN
Braving the Heat
Launched in 2018, the Parker Solar Probe travels through the Sun's outer atmosphere (Corona) to study solar wind and high-energy particles.
Fastest human-made object.
Temperature of the heat shield.
Thermal Sync
Carbon Mapping. Monitoring the TPS (Thermal Protection System) to track the 1,370°C solar interface.
- 🛡️ Shield: 4.5-Inch Carbon Composite.
- 🔥 External: 2,500°F Solar Flux Sync.
- ❄️ Internal: 30°C Payload Buffer.
Velocity Sync
Kinetic Mapping. Tracking the Perihelion buffer as the probe reaches 690,000 km/h.
- 🚀 Speed: 191 km/s Orbital Sync.
- ☄️ Gravity: Venus Assist Protocol.
- ⏱️ Record: Fastest Kinetic Buffer.
Plasma Sync
Magnetic Mapping. Monitoring the FIELDS instrument to track solar wind acceleration.
- 🧲 Fields: EMF Induction Sync.
- 🌬️ Wind: Supersonic Ion Protocol.
- 🌀 Corona: Alfvén Surface Buffer.
Proximity Sync
Distance Mapping. Monitoring the solar-approach buffer at 3.8 million miles from the surface.
- ☀️ Distance: 9.86 Solar Radii Sync.
- 🛰️ Orbit: Highly Elliptical Protocol.
- 🌌 Corona: Outer Atmosphere Buffer.
Power Sync
Solar Mapping. Managing the retractable solar arrays and autonomous cooling buffer.
- 🔋 Array: Shadow-Retraction Sync.
- 💧 Cooling: Deionized Water Protocol.
- 🧠 Logic: Self-Correction Buffer.
Paper
PARKER SOLAR UPLINK ☀️
Objective: 10-Item Coronal Physics Calibration.
Sources
THERMAL PROTECTION (TPS)
An 8-foot-wide, 4.5-inch-thick carbon-carbon composite shield. It protects the craft from temperatures reaching nearly **1,370°C** while keeping the instruments at a cool **29°C**.
SHIELD SPECSRECORD VELOCITY
Using Venus gravity assists, Parker reaches speeds up to **692,000 km/h** (430,000 mph). This is fast enough to travel from Tokyo to New York in under a minute.
MISSION LOGALFVÉN SURFACE
The probe's mission is to locate where solar winds transition from sub-Alfvénic to super-Alfvénic, helping solve the mystery of why the corona is hotter than the surface.
CORONA DATA