Conic Sections
Time limit: 75 minutes Total marks: 50 Instructions: Answer all questions. Show full working, justify all steps, and state theorems used. Calculators permitted but symbolic reasoning must be shown.
Question 1 — Classify, Reduce, and Prove (18 marks)
Consider the general second-degree curve
(a) Using the discriminant of the general conic , classify this curve. (3)
(b) The presence of the -term indicates the axes are rotated. Show that the rotation angle eliminating the cross-term satisfies , and hence find . (5)
(c) Reduce the equation to standard form in rotated coordinates , and hence determine the semi-major axis, semi-minor axis, eccentricity, and the coordinates of the foci in the rotated frame. (6)
(d) Prove that the quantity (the trace) is invariant under any rotation of axes, and verify this invariant for your reduced equation. (4)
Question 2 — Parabolic Reflector: Physics + Derivation (16 marks)
A satellite dish is modelled as the parabola rotated about its axis. Incoming signals travel parallel to the axis (the -axis).
(a) State the reflective property of the parabola and, using the fact that a tangent at has slope , prove that a ray travelling parallel to the axis and striking the parabola at is reflected through the focus . (You may use that the angle of incidence equals the angle of reflection about the tangent.) (8)
(b) A physical dish has depth at its centre and a rim diameter of . Taking the vertex at the origin with axis along , find and hence the location of the receiver (focus). (4)
(c) Light of a given wavelength focuses because all parallel rays travel equal optical path length to a common focal plane. Using the focus–directrix definition (), argue geometrically why the total path length "focus → point on parabola → directrix line" is the same for every ray, and state why this guarantees the signals arrive in phase. (4)
Question 3 — Orbit Reconstruction from Focal Data (16 marks)
A comet moves on an elliptical orbit with the Sun at one focus . Two positions are recorded: at perihelion (closest approach) the comet is AU from the Sun, and at aphelion (farthest) it is AU from the Sun.
(a) Using the focal-radii property (sum ) and the relations , , determine the semi-major axis , eccentricity , and the distance between the centre and focus. (5)
(b) Write the equation of the orbit in standard form (centre at origin, Sun at ), giving numerical . (3)
(c) Write a short pseudocode/Python function focal_sum(x, y) that, given a point on your ellipse, returns the sum of distances to both foci, and argue that it always returns . Test it symbolically at the point where the ellipse crosses the positive -axis. (4)
(d) Kepler's first law says orbits are ellipses with the Sun at a focus. Explain, using the eccentricity, why a circular orbit is the special degenerate case and state the value of for it. Then compute the ratio for this comet and comment on how eccentric the orbit is. (4)
Answer keyMark scheme & solutions
Question 1
(a) Here , , . Discriminant . Since and the curve is non-degenerate, it is an ellipse (not a circle since ). (3 marks: values 1, sign 1, conclusion 1)
(b) Under rotation , , the new cross-term coefficient is Setting : . (3) Here . So , , giving , so (i.e. ). (2)
(c) The rotated coefficients: (invariant), and So , . Equation becomes , i.e. Thus : semi-major (along ), semi-minor . ; eccentricity . Foci in rotated frame: . (6 marks: A',C' 3; standard form 1; a,b,e 1; foci 1)
(d) Under rotation, The -terms cancel. Hence is invariant. Check: . ✓ (4 marks: proof 3, verification 1)
Question 2
(a) Reflective property: the tangent at any point of a parabola makes equal angles with (i) the line from the point to the focus and (ii) the ray parallel to the axis. Equivalently all axis-parallel rays reflect through the focus. Proof: At , tangent slope . The incoming ray is horizontal (slope ). Focal line from to has slope Angle between horizontal ray and tangent: (for ). Angle between focal line and tangent: Since , the angle of incidence equals the angle of reflection about the tangent, so the reflected ray passes through . ∎ (8 marks: statement 2, slopes 2, tan α 1, tan β simplification 2, conclusion 1)
(b) Rim diameter cm ⇒ half-width cm at depth cm. Substitute into : Focus at — receiver is cm from the vertex along the axis. (4 marks: substitution 2, a 1, focus 1)
(c) By the focus–directrix definition with , every point on the parabola satisfies . Consider a wavefront perpendicular to the incoming rays (parallel to the directrix ). For a ray entering at height : the path from the directrix line to then to the focus equals (distance directrix→) + (distance →) = (dist →directrix) — but more directly, the incoming path from the directrix plane to is the horizontal distance, and equals that same horizontal distance (by ). Hence total optical path (plane wavefront → P → focus) is constant for all rays. Equal path lengths ⇒ all rays arrive at the focus with the same phase ⇒ constructive interference / in-phase reception. (4 marks: e=1 def 1, equal path argument 2, phase conclusion 1)
Question 3
(a) , . Sum: AU. Then . AU. (5 marks: sum 2, a 1, e 1, c 1)
(b) AU (equivalently ). Orbit: (3 marks: b² 2, equation 1)
(c)
import math
a2, b2 = 4.0, 2.04
c = math.sqrt(a2 - b2) # = 1.4
def focal_sum(x, y):
d1 = math.hypot(x - c, y) # to (+c, 0)
d2 = math.hypot(x + c, y) # to (-c, 0)
return d1 + d2It always returns because the ellipse is defined as the locus of points whose focal-radii sum is constant (property 3.4.5). At the -intercept : each focal radius , so the sum . ✓ (4 marks: code 2, invariance argument 1, test 1)
(d) A circle is the ellipse with , i.e. the two foci coincide at the centre; then . As the ellipse becomes circular (degenerate conic, 3.4.10). Ratio . Since is far from and the ratio is large, this is a highly eccentric (elongated) orbit — typical of a comet, unlike near-circular planetary orbits. (4 marks: e=0 case 2, ratio 1, comment 1)
[
{"claim":"Q1 discriminant is -144 (ellipse)","code":"A,B,C=5,-4,8; result=(B**2-4*A*C==-144)"},
{"claim":"Q1 reduced coefficients A'=4, C'=9 with cos2t=3/5,sin2t=4/5","code":"Ac=sympify(5); Cc=sympify(8); Bc=sympify(-4); c2=Rational(3,5); s2=Rational(4,5); sumAC=Ac+Cc; diff=(Ac-Cc)*c2+Bc*s2; Ap=(sumAC+diff)/2; Cp=(sumAC-diff)/2; result=(Ap==4 and Cp==9)"},
{"claim":"Q1 eccentricity sqrt5/3","code":"a2,b2=9,4; e=sqrt((a2-b2))/sqrt(a2); result=(simplify(e-sqrt(5)/3)==0)"},
{"claim":"Q2 a=22.5 from y=30,x=10","code":"a=Rational(900,40); result=(a==Rational(45,2))"},
{"claim":"Q3 a=2,e=0.7,c=1.4,b2=2.04","code":"a=Rational(4,2); e=Rational(6,20)*0+Rational(7,10); c=a*e; b2=a**2-c**2; result=(a==2 and e==Rational(7,10) and c==Rational(7,5) and b2==Rational(51,25))"},
{"claim":"Q3 focal sum at (0,b) equals 2a","code":"a=2; b2=Rational(51,25); c=Rational(7,5); s=sqrt((0-c)**2+b2)+sqrt((0+c)**2+b2); result=(simplify(s-4)==0)"}
]