GELE Geodesy — Figure of the Earth and the Reference EllipsoidRevision Notes
Condensed revision notes for Figure of the Earth and the Reference Ellipsoid, built for the final weeks before the GELE 2026. These are the distilled key points you need when there is no time left for full study notes — just the concepts, formulas, and traps Professional Regulation Commission (PRC) — Board of Geodetic Engineering tests.
Exam context
On the GELE 2026, the Geodesy subtest carries a "Core" weight in Professional Regulation Commission (PRC) — Board of Geodetic Engineering's pattern. Figure of the Earth and the Reference Ellipsoid lands at position 1st out of 6 in the standard review order. Target score is 70% weighted average, no sub-test below 50%, and roughly a meaningful share of items come from Geodesy on a typical GELE paper.
Figure of the Earth and the Reference Ellipsoid - Revision Notes
Geodesy is the science of determining the size, shape, and gravitational field of the Earth, and locating points precisely on its surface. Because the Earth is not a perfect sphere — it bulges at the equator and is flattened at the poles — geodetic computations model it as an oblate ellipsoid of revolution. In the Philippine context, the PRS92 (Philippine Reference System of 1992) adopts the WGS84 ellipsoid as its reference surface. Every geodetic task — from PPCS/UTM coordinate computation to cadastral surveys under PD 1529 and CA 141 — ultimately depends on the ellipsoid parameters and the radii of curvature derived from them. This chapter covers those foundational relationships that are consistently tested in the PRC Geodetic Engineer Licensure Examination.
Sections
Exam Tips
- Remember: Geoid = physical gravity surface ≈ mean sea level; Ellipsoid = mathematical model for computation.
- RA 8560 = PRS92 law; PD 1529 = Property Registration Decree; CA 141 = Public Land Act — know which law governs which survey activity.
- The formula H = h − N appears frequently: H is orthometric height (from leveling), h is GNSS ellipsoidal height, N is the geoid undulation.
- In the Philippines, geoid undulations (N) typically range from about +5 m to +20 m above the WGS84 ellipsoid.
Key Points
- The Earth is an oblate spheroid (ellipsoid of revolution): flattened at the poles, bulging at the equator.
- A sphere is only a first approximation; the equatorial radius exceeds the polar radius by about 21 km.
- The geoid is the equipotential surface of Earth's gravity that coincides with mean sea level — it is irregular and cannot be used directly for computation.
- The reference ellipsoid is a mathematically smooth surface that closely approximates the geoid; all geodetic coordinates (φ, λ, h) are referenced to it.
- The separation between the geoid and the ellipsoid at any point is the geoid undulation N (also called geoid height).
- PRS92 uses the WGS84 ellipsoid with its origin at the Earth's center of mass (geocentric datum), replacing the old Luzon Datum (Clarke 1866 ellipsoid).
- RA 8560 (Philippine Geodetic Reference System Act of 1998) mandates the use of PRS92 for all geodetic surveys in the Philippines.
Definitions
Term
Geoid
Definition
The equipotential gravity surface that best fits global mean sea level; irregular and undulating.
Importance
It defines orthometric (spirit-leveled) heights H; H = h − N where h is ellipsoidal height and N is geoid undulation.
Term
Reference Ellipsoid
Definition
A mathematically defined oblate ellipsoid of revolution used as the computational surface for geodetic coordinates.
Importance
All latitude, longitude, and ellipsoidal height values are referenced to this surface.
Term
Geoid Undulation (N)
Definition
The vertical distance from the ellipsoid surface to the geoid, positive upward.
Importance
Converts GNSS ellipsoidal heights to orthometric heights: H = h − N.
Term
PRS92
Definition
Philippine Reference System of 1992; the official horizontal and vertical datum of the Philippines using the WGS84 ellipsoid.
Importance
Mandated by RA 8560; basis for all PPCS/UTM coordinates used in cadastral and engineering surveys.
Term
Oblate Ellipsoid of Revolution
Definition
A three-dimensional shape formed by rotating an ellipse about its shorter (minor) axis; a ≥ b.
Importance
The standard mathematical model for the Earth in geodesy.
Section Title
1. The Shape of the Earth — From Sphere to Ellipsoid
Common Mistakes
- Confusing the geoid with the ellipsoid — they are different surfaces; the geoid is physical, the ellipsoid is mathematical.
- Using 'elevation' and 'ellipsoidal height' interchangeably — elevations (orthometric heights) are referenced to the geoid, not the ellipsoid.
- Thinking PRS92 uses the Clarke 1866 ellipsoid — that was the old Luzon Datum; PRS92 uses WGS84.
- Assuming the Earth is a perfect sphere in computation problems — always use ellipsoidal formulas unless explicitly told to approximate.
Formulas
Example
WGS84: f = (6 378 137 − 6 356 752.31) / 6 378 137 = 21 384.69 / 6 378 137 = 0.003352811 = 1/298.257
Formula
f = (a − b) / a
Variables
f = flattening (dimensionless); a = semi-major axis (m); b = semi-minor axis (m)
Application
Compute flattening from the two axes, or recover b if f and a are given.
Example
WGS84: b = 6 378 137 × (1 − 0.003352811) = 6 378 137 × 0.996647189 = 6 356 752.31 m
Formula
b = a(1 − f)
Variables
b = semi-minor axis (m); a = semi-major axis (m); f = flattening
Application
Compute the polar radius from a and f.
Example
WGS84: e² = 2(0.003352811) − (0.003352811)² = 0.006705622 − 0.000011241 = 0.006694380
Formula
e² = (a² − b²) / a² = 2f − f²
Variables
e² = first eccentricity squared (dimensionless); a, b = semi-axes; f = flattening
Application
Fundamental quantity in all radius-of-curvature formulas. Use either form depending on given data.
Example
WGS84: e'² = 0.006694380 / (1 − 0.006694380) = 0.006694380 / 0.993305620 = 0.006739497
Formula
e'² = (a² − b²) / b² = e² / (1 − e²)
Variables
e'² = second eccentricity squared (dimensionless)
Application
Used in some geodetic series expansions and in expressing the meridian radius M in alternate form.
Example
Clarke 1866: e² = 1 − (6 356 583.8 / 6 378 206.4)² = 1 − (0.996615)² = 1 − 0.993241 = 0.006768658
Formula
e² = 1 − (b/a)²
Variables
Alternative derivation of first eccentricity squared from the ratio of axes.
Application
Useful when both a and b are given directly.
Exam Tips
- Memorize WGS84: a = 6 378 137 m, 1/f = 298.257223563, e² = 0.00669438.
- Quick check: e² ≈ 2f (since f² is negligible), so e² ≈ 2/298.257 ≈ 0.00671 — a useful sanity check.
- If only a and b are given, use e² = 1 − (b/a)² to avoid computing f as an intermediate step.
- Board exams sometimes use the Clarke 1866 ellipsoid — know its a and b values.
Key Points
- An ellipsoid is fully defined by two parameters; the standard pair is the semi-major axis a and the flattening f.
- Semi-major axis a = equatorial radius (longest); semi-minor axis b = polar radius (shortest).
- WGS84 defining parameters: a = 6 378 137 m (exact), f = 1/298.257223563.
- All other ellipsoid quantities are derived from a and f.
- The first eccentricity squared e² and the second eccentricity squared e'² are the most frequently used derived quantities.
- Flattening f ≈ 1/298, meaning the Earth is only about 0.335% flatter than a sphere — very nearly spherical.
- The Clarke 1866 ellipsoid (used by the old Luzon Datum) has a = 6 378 206.4 m, b = 6 356 583.8 m — still tested in board exams as a comparison reference.
Definitions
Term
Semi-major axis (a)
Definition
The equatorial radius of the reference ellipsoid; the longest semi-axis.
Importance
One of the two defining parameters of any ellipsoid. WGS84: a = 6 378 137 m.
Term
Semi-minor axis (b)
Definition
The polar radius of the reference ellipsoid; derived from a and f.
Importance
WGS84: b = 6 356 752.3142 m. Appears in eccentricity formulas.
Term
Flattening (f)
Definition
The ratio (a − b)/a expressing the degree of polar flattening of the ellipsoid.
Importance
WGS84: 1/f = 298.257223563. Small but critical — never confuse f ≈ 0.00335 with 1/f ≈ 298.
Term
First Eccentricity Squared (e²)
Definition
e² = (a² − b²)/a² = 2f − f²; measures how much the ellipse deviates from a circle.
Importance
Appears in every radius-of-curvature formula. WGS84: e² = 0.00669438.
Term
Second Eccentricity Squared (e'²)
Definition
e'² = (a² − b²)/b²; an alternative eccentricity measure referenced to the minor axis.
Importance
WGS84: e'² = 0.00673950. Used in some alternative forms of geodetic formulas.
Section Title
2. Ellipsoid Parameters and Their Relationships
Common Mistakes
- Using f instead of 1/f — the flattening f ≈ 0.00335, not 298. In problems stating '1/f = 298.257', you must compute f = 1/298.257 first.
- Computing e instead of e² — all curvature formulas use e² directly; avoid the extra square-root step.
- Using e'² where e² is required (or vice versa) in curvature formulas — identify the formula form first.
- Rounding a and b too early — always carry at least 4–6 significant figures in intermediate steps to avoid accumulated error.
Formulas
Example
WGS84, φ = 14°N (approximate center of the Philippines): sin²14° = 0.058615; 1 − e²sin²φ = 1 − 0.006694×0.058615 = 0.999608; N = 6 378 137 / √0.999608 = 6 378 137 / 0.999804 = 6 379 387 m
Formula
N = a / √(1 − e² sin²φ)
Variables
N = prime vertical radius of curvature (m); a = semi-major axis (m); e² = first eccentricity squared; φ = geodetic latitude
Application
East–west (prime vertical) radius of curvature; used in computing meridian arc, UTM scale factors, and normal section azimuths.
Example
WGS84, φ = 14°N: (1 − e²sin²φ)^(3/2) = (0.999608)^1.5 = 0.999412; M = 6 378 137(1 − 0.006694) / 0.999412 = 6 378 137 × 0.993306 / 0.999412 = 6 335 678 m
Formula
M = a(1 − e²) / (1 − e² sin²φ)^(3/2)
Variables
M = meridian radius of curvature (m); a = semi-major axis; e² = first eccentricity squared; φ = geodetic latitude
Application
North–south (meridian) radius of curvature; used in computing the length of a degree of latitude and in traverse reductions.
Example
WGS84, φ = 14°N: R = √(6 335 678 × 6 379 387) = √(40 414 744 × 10⁶) = 6 357 505 m
Formula
R = √(MN)
Variables
R = Gaussian mean radius of curvature (m); M = meridian radius; N = prime vertical radius
Application
Used as the radius of an osculating sphere for local geodetic approximations and for computing spherical excess.
Example
WGS84, φ = 14°N: Ra = 2(6 335 678)(6 379 387) / (6 335 678 + 6 379 387) = 2(40 414 744×10⁶) / 12 715 065 = 6 357 500 m (very close to R)
Formula
Ra = (2MN) / (M + N)
Variables
Ra = arithmetic mean radius (m); alternative to Gaussian mean
Application
Sometimes used as an alternative mean radius for area computations on a local sphere.
Example
WGS84, φ = 14°N: Rφ = 6 379 387 × cos14° = 6 379 387 × 0.97030 = 6 190 430 m
Formula
Rφ = N cos φ
Variables
Rφ = radius of the parallel circle at latitude φ (m); N = prime vertical radius; φ = geodetic latitude
Application
Length of a degree of longitude at latitude φ; used in computing east–west distances on the ellipsoid.
Exam Tips
- At φ = 0° (equator): N = a = 6 378 137 m; M = a(1−e²) = 6 335 439 m — memorize these equatorial values.
- At φ = 90° (poles): N = M = a²/b = 6 399 594 m — the polar radius of curvature.
- N > M at all latitudes (except poles); at mid-latitudes the difference is about 40–50 km.
- For the Philippines (φ ≈ 6°–20°N), M ≈ 6 334 000–6 337 000 m and N ≈ 6 378 500–6 380 000 m.
- Board exam problems often give φ and ask for N, M, or R — practice the substitution systematically.
Key Points
- Unlike a sphere, an ellipsoid has different curvatures in different directions at any given surface point.
- The two principal radii of curvature at any point are: M (meridian, north–south) and N (prime vertical, east–west).
- Both M and N are functions of the geodetic latitude φ and the ellipsoid parameters a and e².
- N ≥ M at all latitudes; they are equal only at the poles.
- At the equator (φ = 0°): N = a and M = a(1 − e²); at the poles (φ = 90°): N = M = a²/b = a/√(1−e²).
- The Gaussian mean radius R = √(MN) is used for converting small ellipsoidal areas to a sphere and in local geodetic approximations.
- For arc-to-chord corrections and scale factor computations in PPCS/UTM, M and N are used directly.
Definitions
Term
Prime Vertical Radius (N)
Definition
The radius of curvature of the ellipsoid in the east–west (prime vertical) direction at geodetic latitude φ.
Importance
Always ≥ a(1−e²); used in GNSS positioning, UTM grid computations, and normal section calculations.
Term
Meridian Radius (M)
Definition
The radius of curvature of the ellipsoid in the north–south (meridian) direction at geodetic latitude φ.
Importance
Used to compute the arc length of a meridian; M < N at all latitudes except the poles.
Term
Gaussian Mean Radius (R)
Definition
R = √(MN); the geometric mean of the two principal radii; the radius of the osculating sphere.
Importance
Used in spherical excess formulas: ε = Area / R²; and in converting ellipsoidal triangles to spherical triangles.
Term
Radius of Parallel (Rφ)
Definition
The radius of the small circle at latitude φ, equal to N cosφ.
Importance
Used to compute the length of one degree of longitude at a given latitude.
Section Title
3. Radii of Curvature of the Reference Ellipsoid
Common Mistakes
- Swapping M and N — N is the prime vertical (E–W) radius; M is the meridian (N–S) radius. The mnemonic: 'N for Normal (prime vertical Normal section)'.
- Using degrees without converting to radians in sin functions — always set your calculator to DEGREE mode when computing sinφ.
- Forgetting to raise the denominator to the 3/2 power for M but only to the 1/2 power for N.
- Assuming M = N = a (sphere approximation) without checking whether the problem allows it.
- Not squaring the sine: the formula uses sin²φ, not sinφ.
Formulas
Example
Answer: b = 6 356 752.31 m; e² = 0.006694381 ✓
Formula
PROBLEM 1 — Find b and e² for WGS84
Variables
Given: a = 6 378 137 m, f = 1/298.257223563
Application
Step 1: f = 1/298.257223563 = 0.003352811. Step 2: b = a(1−f) = 6 378 137 × 0.996647189 = 6 356 752.31 m. Step 3: e² = 2f − f² = 2(0.003352811) − (0.003352811)² = 0.006705622 − 0.000011241 = 0.006694381.
Example
Answer: N = 6 388 838 m ✓ (matches reference solution)
Formula
PROBLEM 2 — Find N at φ = 45°N (WGS84)
Variables
Given: a = 6 378 137 m, e² = 0.006694381, φ = 45°
Application
Step 1: sin²45° = (0.707107)² = 0.500000. Step 2: e²sin²φ = 0.006694381 × 0.500000 = 0.003347190. Step 3: 1 − e²sin²φ = 0.996652810. Step 4: √0.996652810 = 0.998325. Step 5: N = 6 378 137 / 0.998325 = 6 388 838 m.
Example
Answer: M ≈ 6 351 355 m
Formula
PROBLEM 3 — Find M at φ = 30°N (WGS84)
Variables
Given: a = 6 378 137 m, e² = 0.006694381, φ = 30°
Application
Step 1: sin²30° = 0.250000. Step 2: e²sin²φ = 0.006694381 × 0.250 = 0.001673595. Step 3: W = 1 − 0.001673595 = 0.998326405. Step 4: W^(3/2) = (0.998326)^1.5 = 0.997490. Step 5: a(1−e²) = 6 378 137 × 0.993305619 = 6 335 439 m. Step 6: M = 6 335 439 / 0.997490 = 6 351 355 m.
Example
Answer: f = 0.003390 (1/f ≈ 294.98); e² = 0.006768658
Formula
PROBLEM 4 — Find f and e² for Clarke 1866 (a = 6 378 206.4 m, b = 6 356 583.8 m)
Variables
Given: a = 6 378 206.4 m, b = 6 356 583.8 m
Application
Step 1: f = (a−b)/a = (6 378 206.4 − 6 356 583.8) / 6 378 206.4 = 21 622.6 / 6 378 206.4 = 0.003390076. Step 2: 1/f = 294.978. Step 3: e² = 1 − (b/a)² = 1 − (6 356 583.8/6 378 206.4)² = 1 − (0.996609)² = 1 − 0.993230 = 0.006768658.
Example
Answer: R ≈ 6 359 264 m at φ = 14°N
Formula
PROBLEM 5 — Find R = √(MN) at φ = 14°N (WGS84) — Philippine-centric
Variables
Given: a = 6 378 137 m, e² = 0.006694381, φ = 14°
Application
Step 1: sin²14° = (0.241922)² = 0.058526. Step 2: e²sin²φ = 0.006694 × 0.058526 = 0.000392. Step 3: W = 1 − 0.000392 = 0.999608. Step 4: N = 6 378 137/√0.999608 = 6 378 137/0.999804 = 6 379 387 m. Step 5: W^(3/2) = 0.999412. Step 6: M = 6 335 439/0.999412 = 6 339 162 m. Step 7: R = √(6 339 162 × 6 379 387) = √(40 441 ×10⁶) = 6 359 264 m.
Exam Tips
- Systematic approach: (1) Compute sin²φ → (2) Compute W = 1−e²sin²φ → (3) Compute N = a/√W → (4) Compute M = a(1−e²)/W^(3/2) → (5) Compute R = √(MN).
- For multiple-choice questions, use the value of N to quickly eliminate wrong answers: N is always between 6 378 137 m (equator) and 6 399 594 m (pole).
- If asked for 'radius of curvature in the prime vertical,' that is N — always.
- Always double-check your φ is in degrees and your calculator is in DEGREE mode before evaluating sin φ.
Key Points
- Always identify: what is given (a, b, f, e², φ), what is asked (N, M, R, f, e², b).
- Write the formula, substitute values carefully, and compute step-by-step.
- Keep at least 4 decimal places in intermediate steps.
- Verify your answer using a quick-check: N should be close to 6 378 000–6 380 000 m for Philippine latitudes.
Section Title
4. Worked Board-Style Problems
Common Mistakes
- Forgetting to compute W = 1 − e²sin²φ before computing N and M separately.
- Using the wrong exponent: N uses W^(1/2); M uses W^(3/2).
- Computing (1 − e²sin²φ)^(3/2) by cubing the square root twice — use the direct exponent: W^(3/2) = W × √W.
- Mixing up which formula applies to which direction (M = N–S; N = E–W).
Formulas
Example
φ = 10°N on WGS84: N = 6 378 137/√(1 − 0.00669438 sin²10°) = 6 378 137/√(0.999798) = 6 378 781 m
Formula
WGS84: a = 6 378 137 m; 1/f = 298.257223563; e² = 0.00669438; b = 6 356 752.31 m
Variables
Defining constants for the World Geodetic System 1984
Application
Use for all current PRC board exam computations unless specifically stated otherwise.
Example
Molodensky-Badekas or Helmert 7-parameter transforms are used when converting between Luzon Datum and PRS92.
Formula
Clarke 1866: a = 6 378 206.4 m; b = 6 356 583.8 m; f = 1/294.978; e² = 0.006768658
Variables
Parameters of the Clarke 1866 ellipsoid (Old Luzon Datum)
Application
Used in problems involving transformation from Old Luzon Datum to PRS92 or in historical survey contexts.
Exam Tips
- When the problem says 'Philippine Reference System' or 'PRS92,' always use WGS84 parameters.
- RA 8560 amended RA 4374 — know both; RA 8560 is the current controlling law for geodetic engineering practice.
- PD 1529 governs title registration; CA 141 governs public land; both require geodetic surveys tied to official control.
- PPCS/UTM: the Philippines spans Zones I (116.5°–121°E) to V (125°–127.5°E) — Zone III (121°–123°E) covers most of Luzon.
Key Points
- Know both ellipsoids: WGS84 is current (PRS92); Clarke 1866 is historic (Old Luzon Datum) — both appear in board exams.
- The primary ellipsoid for all current Philippine geodetic work is WGS84 under PRS92 (RA 8560).
- All PPCS/UTM grid coordinates in the Philippines are projected from the WGS84/PRS92 ellipsoid.
- For cadastral and titling purposes under PD 1529 and CA 141, geodetic control points are tied to PRS92.
- RA 4374 (Geodetic Engineering Act, as amended by RA 8560) governs the practice of geodetic engineering in the Philippines.
Definitions
Term
RA 8560 (Geodetic Engineering Act)
Definition
Philippine law that amended RA 4374 to define the practice of geodetic engineering, establish PRS92, and require use of WGS84.
Importance
Legal basis for PRS92; all geodetic surveys must comply.
Term
PD 1529 (Property Registration Decree)
Definition
Presidential Decree governing the registration of land titles in the Philippines.
Importance
Cadastral surveys under PD 1529 use geodetic coordinates tied to PRS92.
Term
CA 141 (Public Land Act)
Definition
Commonwealth Act governing the classification and disposition of public lands.
Importance
Public land surveys (cadastral surveys) are conducted under CA 141 and require geodetic control referenced to PRS92.
Term
PPCS/UTM
Definition
Philippine Plane Coordinate System using the Universal Transverse Mercator projection on the WGS84 ellipsoid.
Importance
Provides (x, y) grid coordinates for engineering and cadastral applications; φ and λ from ellipsoid are projected to PPCS.
Section Title
5. Summary of Key Ellipsoid Parameters — WGS84 vs. Clarke 1866
Common Mistakes
- Applying Clarke 1866 parameters in a problem that specifies WGS84/PRS92.
- Ignoring the legal framework — exam questions sometimes ask about which law mandates a particular datum or survey requirement.
- Forgetting that PPCS Zone I–V cover the Philippines from Mindanao to Batanes — zone selection depends on longitude bands.
Connections
- Chapter link → PPCS/UTM Projection: The scale factor k₀ and the central meridian arc length in UTM are computed using M and N from this chapter. Every PPCS coordinate in the Philippines depends on WGS84 ellipsoid parameters.
- Chapter link → Geodetic Datums and Transformations: Converting between Old Luzon Datum (Clarke 1866) and PRS92 (WGS84) requires knowing both sets of ellipsoid parameters and applying 7-parameter Helmert transformations.
- Chapter link → Geodetic Leveling and Heights: The relationship H = h − N (orthometric height = ellipsoidal height − geoid undulation) connects the ellipsoid (this chapter) to the geoid and spirit leveling.
- Chapter link → Geodetic Surveying / Traverse Reduction: Reducing ground distances to the ellipsoid requires N and M at the midpoint latitude of each survey line.
- Chapter link → Spherical Trigonometry and Geodetic Problems: The direct and inverse geodetic problems (Vincenty, Bowring) use M and N throughout their iterative computations.
- Chapter link → GNSS/GPS Positioning: WGS84 is the native ellipsoid of GPS/GNSS receivers. Converting GNSS output (φ, λ, h) to PPCS (N, E) requires full knowledge of WGS84 ellipsoid parameters.
- Legal connection → PD 1529 and CA 141: Cadastral surveys submitted to DENR-LMB and ROD must reference PRS92 control; the ellipsoid parameters here underpin those control networks.
- Chapter link → Gravity and the Geoid: The theoretical gravity formula γ at the ellipsoid surface uses a, b, f, and e² — connecting this chapter to physical geodesy.
- Chapter link → Map Projections (Conformal): The Mercator and Lambert conformal conic projections also require ellipsoid eccentricity e for their scale factor formulas.
- Conceptual connection → Earth's Dimensions: The values of a and b here explain why 1 degree of latitude is longer near the poles (~111.7 km) than near the equator (~110.6 km) — because M increases with latitude.
Exam Strategy
For the PRC Geodetic Engineer board examination on this topic: (1) MEMORIZE the four key WGS84 constants: a = 6 378 137 m, 1/f = 298.257223563, e² = 0.00669438, b = 6 356 752.31 m — write them at the top of your scratch paper immediately. (2) MASTER the two curvature formulas: N = a/√W and M = a(1−e²)/W^(3/2) where W = 1 − e²sin²φ; practice computing W first, then N, then M sequentially. (3) For the distinction between M and N, use the mnemonic: 'N is Normal to the meridian — it points East–West; M is Meridian — it runs North–South.' (4) WATCH YOUR CALCULATOR: always verify it is in DEGREE mode before computing sinφ. (5) KNOW THE LAWS: RA 8560 → PRS92/WGS84; PD 1529 → land title registration; CA 141 → public lands; RA 4374 → original geodetic engineering law. (6) On multiple-choice problems, use boundary checks: at φ = 0°, N = 6 378 137 m and M = 6 335 439 m; at φ = 90°, N = M = 6 399 594 m — answers outside this range are wrong. (7) Practice the full problem sequence: given (a, f or b) → compute e² → substitute φ → compute W → compute N and M → compute R if needed. (8) Time management: these computation problems typically take 3–5 minutes each; if stuck, skip and return — the formulas are deterministic and you can verify by substituting back.
Quick Review Questions
What are the two defining parameters of a reference ellipsoid?
All other ellipsoid quantities — b, e², e'², and the radii of curvature — are derived from these two parameters. WGS84 uses a = 6 378 137 m and f = 1/298.257223563 as its defining constants.
Give the WGS84 values of: (a) semi-major axis a, (b) inverse flattening 1/f, and (c) first eccentricity squared e².
These are the fundamental WGS84 constants used in every modern geodetic computation in the Philippines under PRS92.
Compute the semi-minor axis b of WGS84 given a = 6 378 137 m and f = 1/298.257223563.
First compute f = 1/298.257223563 = 0.003352811, then b = a(1−f). The polar radius is about 21 km shorter than the equatorial radius.
What is the prime vertical radius of curvature N at the equator (φ = 0°) for WGS84?
At φ = 0°, sin²φ = 0, so the denominator √(1−e²sin²φ) = 1, giving N = a. This is a useful boundary check.
What is the meridian radius M at the equator (φ = 0°) for WGS84?
At φ = 0°, the denominator (1−e²sin²φ)^(3/2) = 1, so M = a(1−e²). Note M < N at the equator — the meridian is more curved (shorter radius) than the prime vertical.
Which radius of curvature is greater at any given latitude: M or N?
The prime vertical radius N has a denominator to the 1/2 power while M has the same denominator to the 3/2 power, and a(1−e²) < a. Hence M < N for all 0° ≤ φ < 90°.
What does the formula e² = 2f − f² represent, and why is f² negligible?
Because f is so small (≈1/298), the f² term contributes less than 0.2% to e², making e² ≈ 2f a useful approximation for quick checks.
What is the Gaussian mean radius R and when is it used?
For the Philippines at φ ≈ 14°N, R ≈ 6 359 000 m. The spherical excess of a geodetic triangle is ε = Area/R² (in radians).
What Philippine law mandates the use of PRS92 (based on WGS84) for all geodetic surveys?
RA 8560 established PRS92 as the official horizontal datum of the Philippines, replacing the old Luzon Datum (Clarke 1866 ellipsoid). All cadastral and engineering geodetic surveys must reference PRS92.
For the Clarke 1866 ellipsoid (a = 6 378 206.4 m, b = 6 356 583.8 m), compute the flattening f and e².
Clarke 1866 has slightly different parameters from WGS84. Its 1/f ≈ 295 vs WGS84's 1/f ≈ 298. This difference matters in datum transformation computations.
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