2) Orbital Mechanics & Orbit Types

🌍 Orbit Regimes β€” LEO, MEO, GEO and HEO
EARTH LEO 160–2000 km MEO 2 000–20 000 km GEO 35 786 km HEO (e.g. Molniya) Key trade-offs β€’ LEO β€” low latency (~5–20 ms), small footprint, many sats needed β€’ MEO β€” moderate latency (~50–100 ms), navigation & some voice β€’ GEO β€” ~240 ms latency, single continental coverage, fixed dish β€’ HEO β€” high-latitude coverage, elliptical, slow near apogee Kepler's third law TΒ² = (4π² / ΞΌ) Β· aΒ³ β€” orbital period grows with semi-major axis ΞΌ Earth = 398 600 kmΒ³/sΒ²
β–Ά Play Slideshow (Voice ON)
πŸ“– Theory – 2) Orbital Mechanics & Orbit Types

I. Kepler's Laws
β€’ First law β€” orbits are ellipses with Earth at one focus.
β€’ Second law β€” equal areas in equal times.
β€’ Third law β€” TΒ² ∝ aΒ³.

II. The Six Keplerian Elements
β€’ a β€” semi-major axis.
β€’ e β€” eccentricity.
β€’ i β€” inclination.
β€’ Ξ© β€” RAAN.
β€’ Ο‰ β€” argument of perigee.
β€’ Ξ½ β€” true anomaly.

III. Orbit Regimes
β€’ LEO 160–2000 km β€” 90 min period.
β€’ MEO 2000–20000 km β€” 6–12 h period.
β€’ GEO 35786 km β€” 24 h period.
β€’ HEO β€” elliptical, slow near apogee.

IV. Special Orbits
β€’ Geostationary β€” equatorial, circular, 24 h.
β€’ Sun-synchronous β€” near-polar, constant solar illumination.
β€’ Molniya β€” 12 h HEO, high-latitude coverage.
β€’ Polar β€” 90Β° inclination.

V. Orbital Perturbations
β€’ Earth's oblateness (J2) β€” nodal regression.
β€’ Solar and lunar gravity.
β€’ Atmospheric drag β€” significant in LEO.
β€’ Solar radiation pressure.

VI. Coverage Geometry
β€’ Elevation angle β€” must be above ~5–10Β°.
β€’ Slant range β€” varies with elevation.
β€’ Footprint β€” the area visible to the satellite.
β€’ Eclipse period β€” satellite in Earth's shadow.

πŸ† Level 1

⭐ 0 points

πŸ›°οΈ 0 MCQs
πŸ“ 0 essays πŸ§ͺ 0 labs πŸ… 0 badges

πŸ“ Advanced Essay (AI-Marked)

Question:
Critically analyse orbital mechanics as applied to satellite communication. Discuss Kepler's laws, the six orbital elements, the trade-offs between LEO, MEO, GEO and HEO regimes, and how coverage and latency requirements dictate orbit choice.
πŸ“‹ Rubric: Knowledge (30%) Β· Analysis (30%) Β· Literature (20%) Β· Structure (10%) Β· Originality (10%). 1500–2500 words.

πŸ“ Practice MCQs (15)

Q1: Why is Semi-major axis important?

Q2: What is Polar?

Q3: How does Kepler third law differ from alternatives?

Q4: What is Kepler first law?

Q5: Why is RAAN important?

Q6: What is Molniya?

Q7: Why is Argument of perigee important?

Q8: Explain Sun-synchronous in satellite communication.

Q9: Why is Kepler first law important?

Q10: Why is Sun-synchronous important?

Q11: How does RAAN differ from alternatives?

Q12: How does Sun-synchronous differ from alternatives?

Q13: How does Semi-major axis differ from alternatives?

Q14: What is Inclination?

Q15: How does Geostationary differ from alternatives?

Module score: 0/0