The Equator
The only parallel whose plane passes through Earth's centre, so it satisfies both definitions at once.
- Rhumb line?
- Yes
- Great circle?
- Yes
- Constant track?
- Yes — 090° or 270°
- Shortest route?
- Yes
ATPL General Navigation
Shortest route versus constant bearing
Two important paths can connect positions on Earth. A great-circle route follows the shortest path over the spherical Earth, but its true track usually changes continuously. A rhumb line crosses all meridians at a constant angle, making it easier to steer, but it is normally longer.
By the end of this chapter, you should be able to:
Both routes join the same two positions, yet they take different paths across the sphere. Everything in this chapter builds on the reference lines shown here.
Interactive educational diagram
Hover, tap or tab through a legend item to isolate that element on the globe.
A 48°00′N 060°00′W
B 40°00′N 040°00′E
Both paths join the same two positions. The red arc is a section of a circle whose plane cuts Earth’s centre; the purple path holds one steady angle against every meridian it crosses.
A great circle is formed by the intersection of Earth with a plane that passes through Earth's centre.
Set any two positions, or pick a published city pair, and read the distance, tracks and vertex straight off the spherical calculation.
Interactive educational diagram
Drag any slider, or pick a preset city pair. Distance uses the haversine central angle; tracks use spherical trigonometry.
Preset city pairs
Classic mid-latitude North Atlantic route: the great circle passes well north of the rhumb line.
Central angle from the haversine form, worked in radians:
Δσ = 2 asin( √( sin²(Δφ/2) + cos φ₁ · cos φ₂ · sin²(Δλ/2) ) )
Distance = R · Δσ with R = 3440.065 NM (mean Earth radius)
Distance = 60 × Δσ° (the ATPL rule of thumb)
Initial track, then normalised to 000°–359°:
θ = atan2( sin Δλ · cos φ₂ , cos φ₁ · sin φ₂ − sin φ₁ · cos φ₂ · cos Δλ )
The final track is the reverse initial track plus 180°. Clairaut’s equation gives the vertex:
cos φ_vertex = | sin θ · cos φ₁ |
The aircraft follows one fixed great-circle plane, but the direction of local meridians changes as the aircraft moves across Earth. The angle between the route and local north therefore changes.
Interactive educational diagram
Move the route-progress slider with the pointer or the arrow keys. The aircraft symbol turns to follow the local tangent.
Track comparison
The route is fixed, but the reference direction of local north changes.
Try the same route on another leg
Classic mid-latitude North Atlantic route: the great circle passes well north of the rhumb line.
Local north is drawn at 51.5° N, meridian angle reference 0.0175 radians per degree.
The vertex is the point where a great circle reaches its maximum latitude in one hemisphere.
Interactive educational diagram
Switch between the complete great circle and the segment actually flown to see whether the vertex is crossed.
Preset city pairs
Classic mid-latitude North Atlantic route: the great circle passes well north of the rhumb line.
A rhumb line, or loxodrome, crosses every meridian at the same angle. It therefore maintains a constant true track.
Interactive educational diagram
Each amber wedge measures the angle between the route and local north. Every wedge is the same size — that is what makes this a rhumb line.
Because the angle never changes, a navigator could hold one compass course for the whole leg. Extended indefinitely the track keeps turning across new meridians and winds ever tighter around the pole — approaching it, but never arriving.
Only two families of route satisfy both definitions at once. Everything else is a rhumb line only.
The only parallel whose plane passes through Earth's centre, so it satisfies both definitions at once.
A meridian and its anti-meridian together form a complete great circle, flown on a constant track.
Its plane is parallel to the Equator but does not contain Earth's centre, so it is a small circle.
Any other constant-track route. Extended indefinitely it spirals towards a pole without reaching it.
The same positions as the great-circle tool, now solved with the loxodromic equations.
Interactive educational diagram
Set any departure and destination. The great circle is shown faintly for reference — notice the rhumb line never wanders from its single track.
Preset city pairs
Classic mid-latitude North Atlantic route: the great circle passes well north of the rhumb line.
Worked in radians, with Δλ taken as the shorter difference in longitude:
Δψ = ln[ tan(π/4 + φ₂/2) / tan(π/4 + φ₁/2) ]
q = Δφ / Δψ (q = cos φ₁ when |Δψ| is negligible, e.g. along a parallel)
d = R · √( Δφ² + q²·Δλ² )
θ = atan2( Δλ , Δψ ) , normalised to 000°–359°
The Δψ term is the Mercator latitude difference, which is exactly why a rhumb line plots straight on a Mercator chart.
Change the projection and the two routes swap appearances: the rhumb line becomes straight and the great circle bends towards the nearer pole.
Interactive educational diagram
Toggle each route on and off. The rhumb line is drawn from the same loxodromic equations as the globe view — it plots straight because Mercator preserves angles.
Preset city pairs
Classic mid-latitude North Atlantic route: the great circle passes well north of the rhumb line.
Interactive educational diagram
Both columns use the same departure and destination, so every difference you see comes from the geometry alone.
The rhumb-line route is 118 NM longer, an increase of 3.9%.
Preset city pairs
Classic mid-latitude North Atlantic route: the great circle passes well north of the rhumb line.
Distance difference = rhumb-line distance − great-circle distance
Percentage penalty = [ (rhumb − great circle) / great circle ] × 100
Both distances use the same mean Earth radius, so the comparison is consistent. A percentage is only meaningful alongside the absolute figure: 2% of a 200 NM leg is 4 NM, which no flight plan would notice.
The geometric penalty depends on length, orientation and latitude — and geometry is only one input to a real flight plan.
Short local route
Negligible — well under 1 NM, far inside normal flight-planning tolerance.
Medium continental route
Minor — 8 NM on this leg, rarely a routing driver on its own.
Long intercontinental route
Substantial — 438 NM saved by flying the great circle, which is real fuel and time.
Shortest geometric distance does not automatically mean shortest flight time or lowest fuel burn: wind, airway structure, airspace restrictions and traffic flow all matter.
Read each scenario, reason it through with the steps, then reveal the answer.
Example 1
Two points on the Equator
Is the route along the Equator a great circle, a rhumb line, or both?
Example 2
Along one meridian, 30° N to 60° N
What kind of route is this, and what is the true track?
Example 3
Along latitude 50° N, eastbound
Is this route a great circle, a rhumb line, or both?
Example 4
A long mid-latitude route curving polewards on a Mercator chart
A long route between two mid-latitude points appears curved toward the pole on a Mercator chart. What is it?
Example 5
A route crossing every meridian at the same angle
What is this route called, and is it the shortest path?
Each claim below is one of the classic traps. Open the panel for the correction.
It depends on the projection. On a Mercator chart a straight line is a rhumb line; on a Lambert or polar stereographic chart a straight line is very nearly a great circle.
The track normally changes continuously, because local north changes direction along the route. The Equator and the meridians are the only exceptions.
Only the Equator is. Every other parallel is a small circle, because its plane does not pass through Earth's centre.
The difference may be very small on short routes, and it is exactly zero along the Equator or along a meridian. The penalty grows with distance, with east-west orientation and with latitude.
The vertex is where the great circle reaches its maximum latitude. It coincides with the midpoint only when departure and destination are at the same latitude — and it may lie entirely outside the segment flown.
Great circles plot as curves concave to the Equator. Only the Equator itself and the meridians plot as straight lines and are also great circles.
An oblique rhumb line approaches and spirals toward the pole mathematically, circling it an infinite number of times without ever arriving. A meridian is the exception: it does reach the pole.
Fourteen questions in ATPL style. One retry is allowed per question, 75% is a pass, and you can restart as often as you like.
Question 1 of 14 · Multiple choice
Great-circle definition
0/14
Everything from this chapter on one revision sheet.
Plane
Passes through Earth's centre
Division
Divides Earth into equal hemispheres
Distance
Shortest spherical route
Track
True track normally changes
On Mercator
Curved, concave to the Equator
Vertices
Has a northern and a southern vertex
Angle
Constant angle with all meridians
Track
Constant true track
Distance
Normally longer
On Mercator
Straight line
Extended
Spirals toward the poles
Practical
Historically easy to steer
Equator
Great circle and rhumb line
Meridian
Great circle and rhumb line
Other parallels
Rhumb line only
Chapter in progress
Work through the remaining sections and score at least 75% on the knowledge check, then mark the chapter complete.
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Chapter completion