Archimedes & Apollonius
The greatest mathematician of antiquity and the master of conic sections — proto-calculus, mathematical physics, and the geometry of curves
5.1 Archimedes of Syracuse (c. 287–212 BCE)
Archimedes of Syracuse is widely regarded as the greatest mathematician of the ancient world — and one of the greatest of all time, ranked alongside Newton and Gauss. Born around 287 BCE in the Greek colony of Syracuse on the island of Sicily, he was the son of the astronomer Phidias and may have been related to King Hieron II, the ruler of Syracuse. As a young man, he studied at Alexandria, the intellectual capital of the Hellenistic world, where he likely encountered the works of Euclid and the mathematical traditions of the great Library.
Returning to Syracuse, Archimedes spent most of his life in the service of King Hieron, producing a body of work that spanned pure mathematics, mathematical physics, engineering, and astronomy. His mathematical achievements include the computation of areas and volumes using proto-calculus techniques, the most accurate ancient approximation of $\pi$, the foundations of hydrostatics and statics, and a number system capable of expressing astronomically large quantities.
Key Events in Archimedes' Life
- c. 287 BCE — Born in Syracuse, Sicily
- c. 267 BCE — Studies at Alexandria under successors of Euclid
- c. 260 BCE — Returns to Syracuse; begins major mathematical works
- c. 250 BCE — Writes On the Sphere and Cylinder, On the Measurement of a Circle
- c. 240 BCE — Writes The Sand Reckoner, On Floating Bodies
- 214–212 BCE — Siege of Syracuse by Rome; Archimedes designs war machines
- 212 BCE — Syracuse falls; Archimedes killed by a Roman soldier
The “Eureka” Story
The most famous anecdote about Archimedes, told by Vitruvius, involves King Hieron's golden crown. The king suspected that his goldsmith had secretly alloyed the crown with cheaper silver, but could not prove it without melting the crown down. He challenged Archimedes to determine the truth.
While bathing, Archimedes noticed that the water level rose as he lowered his body into the tub. He realized that the volume of water displaced equals the volume of the submerged object. Since gold is denser than silver, a crown of pure gold would displace less water than an equal-weight crown alloyed with silver. Overcome with excitement, he leapt from the bath and ran through the streets of Syracuse shouting “Eureka!” (“I have found it!”).
Archimedes' Principle of Buoyancy
A body immersed in a fluid experiences an upward buoyant force equal to the weight of the fluid it displaces. If the density of the object is $\rho_{\text{obj}}$ and the density of the fluid is $\rho_{\text{fluid}}$, then the object floats if $\rho_{\text{obj}} < \rho_{\text{fluid}}$ and sinks if $\rho_{\text{obj}} > \rho_{\text{fluid}}$. The buoyant force is:
$$F_b = \rho_{\text{fluid}} \cdot g \cdot V_{\text{displaced}}$$
War Machines and the Siege of Syracuse
During the Second Punic War, the Roman general Marcellus besieged Syracuse (214–212 BCE). Archimedes designed ingenious defensive machines that held the Romans at bay for over two years. Ancient sources describe giant catapults that could hurl massive boulders, cranes (the “Claw of Archimedes”) that could lift enemy ships out of the water and capsize them, and — most controversially — burning mirrors that could focus sunlight to set ships on fire.
When Syracuse finally fell in 212 BCE, Archimedes was killed by a Roman soldier, reportedly while engrossed in a geometric diagram drawn in the sand. His last words, according to tradition, were “Do not disturb my circles” (Noli turbare circulos meos). Marcellus, who had given orders that Archimedes be taken alive, was said to be greatly distressed by his death.
5.2 The Method of Exhaustion
Archimedes's most profound mathematical achievement was his use of the method of exhaustion— developed by Eudoxus — to compute areas and volumes that had eluded all previous mathematicians. By inscribing and circumscribing sequences of polygons or other known shapes, he “exhausted” the region in question, trapping the true area or volume between ever-tighter bounds.
The Quadrature of the Parabola
In his treatise Quadrature of the Parabola, Archimedes proved one of his most beautiful results: the area of a parabolic segment (the region between a parabola and a chord) is exactly$\frac{4}{3}$ times the area of the inscribed triangle with the same base and vertex.
Theorem: Area of a Parabolic Segment
Let $S$ be a parabolic segment with chord $AB$, and let $C$ be the point on the parabola where the tangent is parallel to $AB$. Then:
$$\text{Area}(S) = \frac{4}{3} \cdot \text{Area}(\triangle ABC)$$
Archimedes's proof proceeds by repeatedly subdividing the parabolic segment. Start with triangle $\triangle ABC$ inscribed in the segment. Then, in each of the two remaining parabolic segments (between the parabola and the sides $AC$ and $BC$), inscribe new triangles in the same way. Archimedes showed that each new pair of triangles has a combined area equal to $\frac{1}{4}$ of the previous triangle.
Let $T$ denote the area of $\triangle ABC$. After the first step, the total inscribed area is $T$. After the second step, it is $T + \frac{1}{4}T$. After the third step,$T + \frac{1}{4}T + \frac{1}{16}T$. Continuing this process indefinitely:
$$\text{Area}(S) = T + \frac{T}{4} + \frac{T}{16} + \frac{T}{64} + \cdots = T \sum_{k=0}^{\infty} \frac{1}{4^k}$$
Summing the Geometric Series
Archimedes needed to evaluate the geometric series $\sum_{k=0}^{\infty} \frac{1}{4^k}$. He did this by a clever algebraic identity. Consider the finite sum:
$$S_n = 1 + \frac{1}{4} + \frac{1}{4^2} + \cdots + \frac{1}{4^n}$$
Archimedes established the identity:
$$1 + \frac{1}{4} + \frac{1}{4^2} + \cdots + \frac{1}{4^n} + \frac{1}{3} \cdot \frac{1}{4^n} = \frac{4}{3}$$
To see why this holds, note that each term satisfies $\frac{1}{4^k} = \frac{4}{3} \cdot \frac{1}{4^k} - \frac{1}{3} \cdot \frac{1}{4^k}$. Summing telescopically:
$$S_n = \frac{4}{3}\left(1 - \frac{1}{4^{n+1}}\right) = \frac{4}{3} - \frac{1}{3 \cdot 4^n}$$
As $n \to \infty$, the remainder term $\frac{1}{3 \cdot 4^n} \to 0$, so:
$$\sum_{k=0}^{\infty} \frac{1}{4^k} = \frac{4}{3}$$
Therefore, $\text{Area}(S) = \frac{4}{3} T$. Archimedes then completed the proof rigorously using the method of exhaustion (double contradiction), showing that the area can be neither greater nor less than $\frac{4}{3}T$.
Numerical Example
Consider the parabola $y = x^2$ from $x = 0$ to $x = 1$. The chord connects $(0, 0)$ to $(1, 1)$. The vertex of the parabolic segment is at$x = 1/2$, $y = 1/4$. The inscribed triangle has vertices at$(0, 0)$, $(1, 1)$, and $(1/2, 1/4)$.
The area of this triangle is:
$$T = \frac{1}{2} |0(1 - 1/4) + 1(1/4 - 0) + 1/2(0 - 1)| = \frac{1}{2} \cdot |0 + 1/4 - 1/2| = \frac{1}{8}$$
By Archimedes' theorem:
$$\text{Area of segment} = \frac{4}{3} \cdot \frac{1}{8} = \frac{1}{6}$$
We can verify by integration: $\int_0^1 (x - x^2)\,dx = \left[\frac{x^2}{2} - \frac{x^3}{3}\right]_0^1 = \frac{1}{2} - \frac{1}{3} = \frac{1}{6}$. $\checkmark$
5.3 Archimedes' Calculation of $\pi$
In his treatise Measurement of a Circle, Archimedes established the most accurate ancient approximation of $\pi$ — a result that would not be surpassed for several centuries. His method was beautifully simple in concept: he trapped the circle between inscribed and circumscribed regular polygons, computing their perimeters to obtain lower and upper bounds for $\pi$.
Archimedes' Bound on π
$$3\frac{10}{71} < \pi < 3\frac{1}{7}$$
In decimal notation: $3.14084\ldots < \pi < 3.14285\ldots$, pinning down $\pi$ to two decimal places of accuracy.
The Method of Inscribed and Circumscribed Polygons
Consider a circle with diameter 1 (so circumference $= \pi$). A regular $n$-gon inscribed in this circle has perimeter:
$$p_n = n \sin\!\left(\frac{\pi}{n}\right)$$
A regular $n$-gon circumscribed about this circle has perimeter:
$$P_n = n \tan\!\left(\frac{\pi}{n}\right)$$
Since the circle lies between the two polygons: $p_n < \pi < P_n$ for all $n$. As $n$ increases, both bounds converge to $\pi$.
Archimedes started with hexagons ($n = 6$) and doubled the number of sides five times, reaching 96-gons ($n = 96$). He didn't use trigonometric functions (which hadn't been developed yet), but instead used a recursive geometric relationship. If $s_n$ is the side length of the inscribed $n$-gon in a circle of diameter 1, then the side of the inscribed $2n$-gon is:
$$s_{2n} = \sqrt{\frac{1 - \sqrt{1 - s_n^2}}{2}}$$
Similarly, if $S_n$ is the side of the circumscribed $n$-gon, then:
$$S_{2n} = \frac{S_n}{\sqrt{1 + S_n^2} + 1} \cdot 2$$
Archimedes' Computation Step by Step
Starting with a regular hexagon inscribed in a circle of diameter 1:
- 6-gon: $p_6 = 3.0000$, $P_6 = 3.4641\ldots$
- 12-gon: $p_{12} = 3.1058\ldots$, $P_{12} = 3.2153\ldots$
- 24-gon: $p_{24} = 3.1326\ldots$, $P_{24} = 3.1596\ldots$
- 48-gon: $p_{48} = 3.1393\ldots$, $P_{48} = 3.1460\ldots$
- 96-gon: $p_{96} = 3.14103\ldots$, $P_{96} = 3.14271\ldots$
The 96-gon bounds yield $3\frac{10}{71} < \pi < 3\frac{1}{7}$. Archimedes performed all of these calculations by hand, using only rational arithmetic with careful upper and lower bound tracking for the square roots — a tour de force of computational skill.
The upper bound $\frac{22}{7}$ became the standard approximation of $\pi$ used for centuries. It is accurate to about 0.04%. The method itself could be extended to arbitrarily many sides for greater accuracy; later mathematicians (notably the Chinese mathematician Zu Chongzhi, c. 480 CE) used Archimedes's approach with polygons of up to 12,288 and 24,576 sides to obtain$\pi \approx \frac{355}{113} = 3.1415929\ldots$, correct to six decimal places.
5.4 Archimedes' Principle of the Lever
In his treatise On the Equilibrium of Planes, Archimedes established the mathematical foundations of statics — the study of bodies in equilibrium. His treatment of the lever is considered the first-ever example of mathematical physics: physical laws derived from axioms through rigorous logical deduction.
The Law of the Lever
Two weights balance on a lever when they are inversely proportional to their distances from the fulcrum:
$$m_1 d_1 = m_2 d_2$$
where $m_1, m_2$ are the weights and $d_1, d_2$ are their respective distances from the fulcrum. Equivalently, the fulcrum must be at the center of gravity of the system.
Archimedes famously declared: “Give me a place to stand and I will move the Earth” (Dos moi pa sto, kai tan gan kinaso). This was not empty boasting — it is a direct consequence of the lever principle. With a sufficiently long lever and a fulcrum, any weight can be moved by any force, however small, simply by making the lever arm long enough.
Moving the Earth: How Long a Lever?
The mass of the Earth is approximately $M_E \approx 6 \times 10^{24}$ kg. Suppose a person can exert a downward force equivalent to $m = 80$ kg. To “lift” the Earth by even 1 cm, the lever ratio would need to be:
$$\frac{d_1}{d_2} = \frac{M_E}{m} = \frac{6 \times 10^{24}}{80} = 7.5 \times 10^{22}$$
If your arm moves 1 meter, the Earth moves $\frac{1}{7.5 \times 10^{22}}$ meters — about $10^{-23}$ meters, far smaller than an atomic nucleus. The principle is correct, but the practical difficulties are insurmountable!
Archimedes also computed the centers of gravity of various figures: triangles (intersection of medians, at $\frac{1}{3}$ of the way from each side), parallelograms (intersection of diagonals), and parabolic segments. The center of gravity of a parabolic segment lies at$\frac{3}{5}$ of the distance from the vertex to the midpoint of the base — a result that required the full power of his exhaustion methods.
5.5 The Sand Reckoner
In The Sand Reckoner (Psammites), Archimedes set himself an audacious challenge: to show that a number can be named that exceeds the number of grains of sand required to fill the entire universe. This was not merely an exercise in large numbers — it was a fundamental contribution to the theory of numeration and a demonstration that mathematics can handle quantities of any magnitude.
The Greek number system, like most ancient systems, had difficulty expressing very large numbers. The largest named Greek number was the myriad ($\mu = 10{,}000$). A “myriad myriad” was $10^8$. Archimedes needed to go far beyond this.
Archimedes' Large Number System
Archimedes defined a hierarchy of “orders” and “periods”:
- First order: Numbers up to $10^8$ (a myriad myriad)
- Second order: Numbers up to $(10^8)^2 = 10^{16}$
- Third order: Numbers up to $(10^8)^3 = 10^{24}$
- Continuing up to the $10^8$-th order: numbers up to $(10^8)^{10^8} = 10^{8 \times 10^8}$
This is the “first period.” The second period extends to $10^{8 \times 10^{16}}$, and so on for $10^8$ periods. The largest number expressible in this system is$10^{8 \times 10^{16}}$ — an astronomically large quantity.
Archimedes then estimated the size of the universe (using Aristarchus's heliocentric model, which he mentions is the largest cosmos anyone has proposed) and the size of a grain of sand. He concluded that the number of grains of sand that would fill the universe is less than$10^{63}$ — a number easily expressible in his system, well within the first period.
The Sand Reckoner is remarkable for several reasons: it shows Archimedes's awareness of Aristarchus's heliocentric model (centuries before Copernicus), it essentially develops a system of exponent notation and the laws of exponents ($10^a \times 10^b = 10^{a+b}$), and it demonstrates the power of mathematical abstraction to transcend the limits of the physical world.
5.6 Surface Area and Volume
Archimedes's masterpiece, On the Sphere and Cylinder, contains results that he himself regarded as his greatest achievements. He proved exact formulas for the surface area and volume of a sphere, and discovered a beautiful relationship between a sphere and its circumscribed cylinder that he wanted inscribed on his tombstone.
Surface Area of a Sphere
The surface area of a sphere with radius $r$ is:
$$A_{\text{sphere}} = 4\pi r^2$$
This equals exactly four times the area of a great circle — a result that Archimedes proved using the method of exhaustion, approximating the sphere by surfaces of revolution of inscribed and circumscribed polygons.
Volume of a Sphere
The volume of a sphere with radius $r$ is:
$$V_{\text{sphere}} = \frac{4}{3}\pi r^3$$
The Cylinder–Sphere Relationship
Consider a sphere of radius $r$ inscribed in a cylinder (a cylinder with radius $r$ and height $2r$). Archimedes proved that the ratios of their volumes and surface areas are both $2 : 3$:
Archimedes' Proudest Result: The 2:3 Ratio
Volume comparison:
$$V_{\text{cylinder}} = \pi r^2 \cdot 2r = 2\pi r^3$$
$$V_{\text{sphere}} = \frac{4}{3}\pi r^3$$
$$\frac{V_{\text{sphere}}}{V_{\text{cylinder}}} = \frac{\frac{4}{3}\pi r^3}{2\pi r^3} = \frac{2}{3}$$
Surface area comparison (including the two circular ends of the cylinder):
$$A_{\text{cylinder}} = 2\pi r \cdot 2r + 2\pi r^2 = 4\pi r^2 + 2\pi r^2 = 6\pi r^2$$
$$A_{\text{sphere}} = 4\pi r^2$$
$$\frac{A_{\text{sphere}}}{A_{\text{cylinder}}} = \frac{4\pi r^2}{6\pi r^2} = \frac{2}{3}$$
Archimedes was so proud of this result that he asked for a sphere inscribed in a cylinder to be engraved on his tombstone. The Roman orator Cicero, visiting Syracuse in 75 BCE — more than a century after Archimedes's death — reported finding the neglected tomb with this very emblem.
The Cone
Archimedes also used the elegant relationship between the cone, sphere, and cylinder. A cone with the same base and height as a cylinder has exactly one-third the volume:
$$V_{\text{cone}} = \frac{1}{3}\pi r^2 h$$
For a cone inscribed in the same cylinder as the sphere (radius $r$, height $2r$):
$$V_{\text{cone}} = \frac{1}{3}\pi r^2 \cdot 2r = \frac{2}{3}\pi r^3$$
Thus $V_{\text{cone}} : V_{\text{sphere}} : V_{\text{cylinder}} = 1 : 2 : 3$ — a strikingly elegant ratio.
The Three Bodies in the Same Cylinder
For a cylinder of radius $r = 5$ cm and height $h = 10$ cm:
- $V_{\text{cone}} = \frac{1}{3}\pi(25)(10) = \frac{250\pi}{3} \approx 261.8 \text{ cm}^3$
- $V_{\text{sphere}} = \frac{4}{3}\pi(125) = \frac{500\pi}{3} \approx 523.6 \text{ cm}^3$
- $V_{\text{cylinder}} = \pi(25)(10) = 250\pi \approx 785.4 \text{ cm}^3$
Ratios: $261.8 : 523.6 : 785.4 = 1 : 2 : 3$ $\checkmark$
5.7 The Archimedean Spiral
In his treatise On Spirals, Archimedes studied a curve that now bears his name — the first mathematical curve to be defined by an equation in what we would now call polar coordinates.
The Archimedean Spiral
The Archimedean spiral is the locus of a point moving uniformly along a ray that rotates uniformly about a fixed point. In polar coordinates:
$$r = a + b\theta$$
where $a$ is the initial distance from the origin and $b$ controls how tightly the spiral is wound. When $a = 0$: $r = b\theta$.
Archimedes proved two remarkable results about this spiral. First, he showed how to construct the tangent line at any point on the spiral — a result that anticipates differential calculus by nearly two millennia. If $P$ is a point on the spiral at distance $r$ from the origin, then the tangent at $P$ makes an angle $\psi$ with the radius vector such that:
$$\tan \psi = \frac{r}{b} = \frac{a + b\theta}{b}$$
Area Enclosed by the Spiral
Archimedes computed the area enclosed between the spiral $r = b\theta$ (with $a = 0$) and the initial ray after one complete revolution ($\theta$ from $0$ to $2\pi$).
Area of One Turn of the Archimedean Spiral
The area enclosed by one complete turn of the spiral $r = b\theta$ is:
$$A = \frac{1}{2}\int_0^{2\pi} r^2\,d\theta = \frac{1}{2}\int_0^{2\pi} b^2\theta^2\,d\theta = \frac{b^2}{2} \cdot \frac{(2\pi)^3}{3} = \frac{4\pi^3 b^2}{3}$$
Archimedes expressed this as: the area is one-third the area of the circle with radius equal to the distance traveled in one revolution. Since $r_1 = 2\pi b$ after one turn, the circle has area $\pi(2\pi b)^2 = 4\pi^3 b^2$, and indeed $\frac{1}{3} \cdot 4\pi^3 b^2 = \frac{4\pi^3 b^2}{3}$. $\checkmark$
The Archimedean spiral also provides a theoretical solution to two of the great problems of ancient geometry: the trisection of an angle and the squaring of the circle. However, since the spiral itself cannot be constructed with compass and straightedge, these solutions were not considered admissible by the strict standards of Greek geometric construction.
5.8 The Archimedes Palimpsest
In 1906, the Danish philologist Johan Ludvig Heiberg discovered a remarkable document in Constantinople (modern Istanbul): a 10th-century Byzantine manuscript of Archimedes's works that had been scraped clean in the 13th century and overwritten with Christian prayers — a palimpsest. Beneath the prayers, using a magnifying glass, Heiberg could still make out the original mathematical text.
The palimpsest contained seven treatises by Archimedes, including the only surviving copy of The Method of Mechanical Theorems — a work that had been lost for over a thousand years. This discovery revolutionized our understanding of Archimedes's thought process.
The Method of Mechanical Theorems
In The Method, addressed to Eratosthenes, Archimedes revealed how he actually discoveredhis results — not through the rigorous method of exhaustion found in his published works, but through a brilliantly intuitive technique that combined mechanics (the lever principle) with a form of proto-integration.
Archimedes imagined geometric figures decomposed into infinitely thin “slices” (what we would call infinitesimals), which he then “weighed” on a balance. By comparing the aggregate weight of the slices of an unknown figure against those of a known one, he could deduce areas and volumes.
Example: Finding the Volume of a Sphere
Consider a sphere, a cone, and a cylinder, all with the same radius $r$ and the cylinder having height $2r$. At height $x$ above the center:
- The cross-section of the sphere is a circle of radius $\sqrt{r^2 - x^2}$, with area $\pi(r^2 - x^2)$
- The cross-section of the cone is a circle of radius $|x|$, with area $\pi x^2$
Adding these at each height:
$$\pi(r^2 - x^2) + \pi x^2 = \pi r^2$$
This is exactly the cross-section of the cylinder! By Cavalieri's principle (or Archimedes's mechanical reasoning), the volume of the sphere plus the volume of the cone equals the volume of the cylinder:
$$V_{\text{sphere}} + V_{\text{cone}} = V_{\text{cylinder}}$$
$$V_{\text{sphere}} + \frac{2}{3}\pi r^3 = 2\pi r^3$$
$$V_{\text{sphere}} = 2\pi r^3 - \frac{2}{3}\pi r^3 = \frac{4}{3}\pi r^3$$
Archimedes considered this mechanical method heuristic, not rigorous — it was his way of discoveringresults, which he then proved using the method of exhaustion for publication. He wrote to Eratosthenes: “I thought it worthwhile to write out the method and publish it, partly because I have already spoken of it, and partly because I am convinced that it will prove very useful for mathematics; for I suspect that some of the theorems which have not yet been proved could be discovered by this method.”
The Palimpsest's Journey
- c. 10th century — Byzantine scribe copies Archimedes' works onto parchment
- c. 1229 — Parchment scraped and overwritten with a prayer book
- 1906 — Heiberg identifies the underlying text in Constantinople
- 1998 — Sold at auction for $2 million to an anonymous buyer
- 1999–2008 — Conserved and imaged at the Walters Art Museum using multispectral imaging and X-ray fluorescence
- 2008 — Full transcription made publicly available; reveals The Method, Stomachion, and other lost texts
5.9 Apollonius of Perga
Apollonius of Perga (c. 262–190 BCE) was the greatest geometer of the ancient world after Archimedes. Born in Perga (modern Turkey), he studied at Alexandria and spent time at Pergamum. His masterwork, the Conics (eight books, of which seven survive — four in the original Greek, three in Arabic translation), is the definitive ancient treatise on conic sections and remained the standard reference for nearly two millennia.
The Conic Sections
A conic section is the curve obtained by intersecting a cone with a plane. Depending on the angle of the plane relative to the cone, one obtains three fundamentally different types of curves. Apollonius was the first to show that all three can be obtained from a single double-napped cone (two cones joined at their apex), and he gave them the names we still use:
Apollonius's Names for the Conics
- Parabola (from Greek parabole, “application”): the cross-section that falls “alongside” — the plane is parallel to a slant side of the cone. Equation: $y^2 = lx$, where $l$ is the latus rectum.
- Ellipse (from Greek elleipsis, “falling short”): the cross-section where the application “falls short.” Equation: $y^2 = lx - \frac{l}{a}x^2$, where $a$ is the semi-major axis.
- Hyperbola (from Greek hyperbole, “throwing beyond”): the cross-section where the application “exceeds.” Equation: $y^2 = lx + \frac{l}{a}x^2$.
The terminology comes from the ancient Greek method of “application of areas.” For a parabola, the rectangle “applied” to the latus rectum exactly matches the square on the ordinate. For an ellipse, it “falls short” (elleipsis); for a hyperbola, it “exceeds” (hyperbole).
Focal Properties
Apollonius discovered the remarkable focal properties of the conics. Every ellipse has two foci, $F_1$ and $F_2$, such that for any point $P$ on the ellipse:
$$|PF_1| + |PF_2| = 2a \quad \text{(constant)}$$
For a hyperbola:
$$\big||PF_1| - |PF_2|\big| = 2a \quad \text{(constant)}$$
For a parabola with focus $F$ and directrix $d$:
$$|PF| = \text{distance from } P \text{ to } d$$
The Reflection Property
Apollonius proved that a ray of light directed toward one focus of an ellipse will reflect off the ellipse and pass through the other focus. Similarly, parallel rays hitting a parabolic mirror all reflect through the focus. In modern terms, the tangent at any point on an ellipse makes equal angles with the two focal radii:
$$\angle F_1PT = \angle F_2PT$$
where $T$ is the tangent line at point $P$. This property has practical applications in satellite dishes, flashlight reflectors, and whispering galleries.
Tangent Constructions
Apollonius developed sophisticated methods for constructing tangent lines to conics. For a parabola$y^2 = lx$, the tangent at the point $(x_0, y_0)$ has the equation:
$$yy_0 = \frac{l}{2}(x + x_0)$$
He also proved that the tangent at the vertex of a parabola is perpendicular to the axis, and that the subnormal (the projection of the normal onto the axis) is constant and equal to $l/2$.
Modern Standard Forms of Conics
Apollonius's equations translate into modern standard forms:
- Ellipse: $\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1$, where$b^2 = a^2 - c^2$ and $c$ is the focal distance. Latus rectum: $l = \frac{2b^2}{a}$
- Hyperbola: $\frac{x^2}{a^2} - \frac{y^2}{b^2} = 1$, where$b^2 = c^2 - a^2$. Asymptotes: $y = \pm \frac{b}{a}x$
- Parabola: $y^2 = 4px$, where $p$ is the distance from vertex to focus. Focus at $(p, 0)$, directrix $x = -p$
Nearly two thousand years after Apollonius, Johannes Kepler discovered that planets move in ellipses with the Sun at one focus (Kepler's First Law, 1609). Isaac Newton then proved that any body moving under an inverse-square gravitational force follows a conic section — an ellipse, parabola, or hyperbola depending on its energy. The purely geometric investigation that Apollonius had pursued for its own sake turned out to describe the fundamental orbits of celestial mechanics.
5.10 Legacy
Archimedes is universally regarded as the greatest mathematician of antiquity and one of the greatest of all time. His work anticipated integral calculus by nearly two millennia, founded the science of mathematical physics, and demonstrated a level of mathematical ingenuity that was not matched until Newton and Leibniz in the 17th century.
Archimedes' Major Achievements
- • Area of a parabolic segment ($\frac{4}{3}$ of inscribed triangle)
- • Surface area and volume of a sphere
- • The cylinder-sphere 3:2 ratio
- • Best ancient approximation of $\pi$
- • The Archimedean spiral and its properties
- • Foundations of hydrostatics (buoyancy)
- • Foundations of statics (the lever)
- • Large number system (The Sand Reckoner)
- • Proto-calculus using infinitesimals (The Method)
Apollonius's Major Achievements
- • Definitive treatise on conic sections (8 books)
- • Named the ellipse, parabola, and hyperbola
- • Focal properties of all conics
- • Reflection property of conics
- • Tangent and normal constructions
- • All conics from a double-napped cone
- • Foundation for Kepler's planetary orbits
- • Foundation for Newton's celestial mechanics
“Give me a place to stand, and I will move the Earth.” — Archimedes (attributed by Pappus)
The work of Archimedes and Apollonius represents the pinnacle of Greek mathematical achievement. After them, Hellenistic mathematics entered a period of consolidation rather than breakthrough, though important contributions would continue to be made by Diophantus, Heron, Pappus, and others. The methods of exhaustion and the theory of conics would remain the most advanced mathematics in the world until the Islamic Golden Age and, ultimately, the invention of calculus in the 17th century.
Video Lectures
These video lectures demonstrate Archimedes' method for computing $\pi$ using inscribed and circumscribed polygons — one of the greatest achievements of ancient mathematics.