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Cosmic Algebra

Algebra

Advanced mathematical problems rooted in astronomical constants and orbital mechanics.

astronomy mathematics physics science
18 Questions Hard Ages 16+ Sep 11, 2026

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This study set covers Algebra through 18 practice questions. Advanced mathematical problems rooted in astronomical constants and orbital mechanics. Every question includes the correct answer so you can learn as you go — pick any format above to get started.

Questions & Answers

Browse all 18 questions from the Cosmic Algebra study set below. Each question shows the correct answer — select a study format above to practice interactively.

1 If the orbital period P of a planet in years is related to its semi-major axis a in AU by Kepler's Third Law (P^2 = a^3), calculate the semi-major axis of a planet with an orbital period of 64 years.
  • A 4 AU
  • B 8 AU
  • C 16 AU
  • D 32 AU
2 The luminosity L of a star is proportional to the square of its radius R and the fourth power of its surface temperature T (L = kR^2T^4). If the temperature doubles and the radius remains constant, by what factor does the luminosity increase?
  • A 2
  • B 4
  • C 8
  • D 16
3 The escape velocity v of a planet is given by v = sqrt(2GM/r). If a planet's mass M is multiplied by 9 and its radius r is multiplied by 4, by what factor does the escape velocity change?
  • A 1.5
  • B 2.25
  • C 3
  • D 4.5
4 Using the inverse-square law for light (I = P / 4πd^2), if the distance d to a star is tripled, by what factor does the observed intensity I decrease?
  • A 1/3
  • B 1/6
  • C 1/9
  • D 1/27
5 The Schwarzschild radius R_s of a black hole is calculated as 2GM/c^2. If you double the mass M of a black hole, how does the Schwarzschild radius change?
  • A It remains the same
  • B It doubles
  • C It quadruples
  • D It halves
6 A satellite orbits Earth at a velocity v proportional to 1/sqrt(r). If the orbital radius r is increased by a factor of 4, what is the new velocity relative to the original?
  • A 1/2 v
  • B 2 v
  • C 1/4 v
  • D 4 v
7 The gravitational force F between two objects is F = G(m1*m2)/r^2. If the mass of both objects is doubled and the distance between them is halved, by what factor does the force increase?
  • A 4
  • B 8
  • C 16
  • D 32
8 The apparent magnitude m of a star is related to its distance d in parsecs by m = M + 5log10(d) - 5. If the distance d is 100 parsecs, what is the value of 5log10(d)?
  • A 5
  • B 10
  • C 15
  • D 20
9 The period of a simple pendulum on a planet is T = 2π*sqrt(L/g). If gravity g on the planet is 4 times that of Earth, what is the ratio of the period on that planet to the period on Earth?
  • A 1:2
  • B 1:4
  • C 2:1
  • D 4:1
10 Hubble's Law states v = H_0 * d. If a galaxy is 500 Megaparsecs away and H_0 is 70 km/s/Mpc, what is its recessional velocity v?
  • A 350 km/s
  • B 3,500 km/s
  • C 35,000 km/s
  • D 350,000 km/s
11 The surface area of a spherical planet is A = 4πr^2. If you increase the radius of the planet by a factor of 10, how does the surface area change?
  • A 10 times
  • B 20 times
  • C 100 times
  • D 400 times
12 The volume of a gas cloud is V = (4/3)πr^3. If the radius of the cloud triples, what is the ratio of the new volume to the original volume?
  • A 3:1
  • B 9:1
  • C 27:1
  • D 81:1
13 In the equation E = mc^2, if mass m is converted to energy entirely and the speed of light c is approximated as 3x10^8 m/s, what is the factor by which mass is multiplied to find energy?
  • A 9x10^16
  • B 3x10^8
  • C 6x10^16
  • D 9x10^8
14 The flux of radiation from a star is F = σT^4. If the temperature T of the star increases from 5,000K to 10,000K, the flux increases by what factor?
  • A 2
  • B 4
  • C 8
  • D 16
15 The density ρ of a planet is M / ((4/3)πr^3). If you double the radius while keeping the mass constant, what is the new density relative to the original?
  • A 1/2
  • B 1/4
  • C 1/8
  • D 1/16
16 Centripetal force is F = mv^2/r. If a moon's velocity v is doubled and its orbit radius r remains constant, by what factor does the centripetal force increase?
  • A 2
  • B 4
  • C 8
  • D 16
17 The Stefan-Boltzmann law relates total power P to area A and temperature T as P = AσT^4. If a star's radius is halved and its temperature is doubled, what happens to the power P?
  • A P is halved
  • B P is doubled
  • C P is quadrupled
  • D P remains the same
18 The orbital energy of a satellite is E = -GMm/2r. If the distance r is doubled, what happens to the total orbital energy E?
  • A It becomes half as negative
  • B It becomes twice as negative
  • C It becomes four times as negative
  • D It remains the same
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