Geometry Symbols and Shapes | Copy and Paste Measurements

Explore a wide collection of geometry symbols and shapes that you can copy and paste into projects, musings, designs and documents. Find circles, squares, triangles, diamonds, polygons, angle symbols, directional shapes, line patterns, and other geometric characters in one convenient place. Simply select your favorite symbol and copy it for use wherever standard Unicode text is supported.

Geometric Symbols

Browse through this collection of geometry symbols... such things as circles and squares, triangles and diamonds, polygons and angles, lines and crosses and arrows, and other geometric shapes maybe you've undiscovered.

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The Squares


Triangles and Polygons


Angles, Arrows, Other Markings

× ÷ ±

Trigonometry Marking Symbols

Now for some trigonometry markings or measurements, with symbols.

Trigonometry uses a wide variety of symbols to represent angles, measurements, variables, identities, coordinates, functions, and mathematical operations. The marks below include common angle notation, Greek letters frequently used for unknown angles, superscripts, subscripts, comparison signs, calculus symbols, and other characters that may appear in trigonometric formulas.

Hover over any symbol to see its short name or typical mathematical use. You can also click each character to copy it for equations, study notes, worksheets, diagrams, educational content, or other places that support Unicode text.

° π θ Θ φ Φ ϕ α β γ Γ δ Δ λ Λ ω Ω ρ σ Σ τ ψ Ψ ε ϵ η κ μ ν ξ Ξ ζ ¹ ² ³

Coordinate Geometry

Coordinate geometry uses symbols for ordered pairs, axes, points, lines, slopes, distances, functions, transformations, intervals, and coordinate systems. Unlike ordinary geometric shape symbols, many coordinate-geometry marks are letters, punctuation marks, or short mathematical expressions that work together to describe a point's exact location on a plane.

The horizontal axis is normally labeled x, while the vertical axis is labeled y. A point is commonly written as an ordered pair such as (x, y), with the x-coordinate appearing first and the y-coordinate second. Coordinate geometry also uses notation for slope, midpoint, distance, domains, ranges, vectors, mappings, and equations of lines and curves.

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The collection below includes individual characters and useful coordinate-geometry notation.

Hover over any particulate to see a short explanation of its usual mathematical meaning, then click it to copy the notation for worksheets, formulas, diagrams, educational pages, or study notes.

x y z O A B P Q M d m b r t f g h , ; : = + - ( ) [ ] { } ⟨ ⟩ ⟦ ⟧ ] [ | | (x, y) (x, y, z) (0, 0) (0, 0, 0) A(x₁, y₁) B(x₂, y₂) P(x, y) M(xₘ, yₘ) x₁ x₂ y₁ y₂ Δx Δy Δ x-axis y-axis z-axis xy-plane xyz-space x ↦ y P ↦ P′ P′ P″ (x, y) ↦ (x′, y′) f(x) y = f(x) y = mx + b y = k x = k Ax + By = C y - y₁ = m(x - x₁) m = Δy/Δx m = (y₂ - y₁)/(x₂ - x₁) d = √((x₂ - x₁)² + (y₂ - y₁)²) M = ((x₁ + x₂)/2, (y₁ + y₂)/2) (x - h)² + (y - k)² = r² x² + y² = r² ℝ² ℝ³ ℝ × ℝ Dom Ran Dom(f) Ran(f) f: A → B < > [a, b] (a, b) [a, b) (a, b] (-∞, ∞) ⟨x, y⟩ ⟨x, y, z⟩ AB⃗ OP⃗ î ĵ I II III IVQ₁ Q₂ Q₃ Q₄ x₀ y₀ z₀ (x₀, y₀) C(h, k) V(h, k) F(h, k) (a, 0) (0, b) (1, 0) (0, 1) (x, 0) (0, y) x = 0 y = 0 x′ y′ z′ A′(x′, y′) B′(x′, y′) T(a, b) (x, y) → (x + a, y + b) (x, y) → (x, −y) (x, y) → (−x, y) (x, y) → (y, x) (x, y) → (−y, −x) R₉₀° R₁₈₀° R₂₇₀° (x, y) → (−y, x) (x, y) → (−x, −y) (x, y) → (y, −x) Dₖ (x, y) → (kx, ky) m₁ = m₂ m₁m₂ = −1 m = tan θ tan θ = |(m₂ − m₁)/(1 + m₁m₂)| x/a + y/b = 1 x cos α + y sin α = p x = x₁ + at y = y₁ + bt L: Ax + By + C = 0 L₁ L₂ d = |Ax₀ + By₀ + C|/√(A² + B²) P = ((mx₂ + nx₁)/(m + n), (my₂ + ny₁)/(m + n)) G = ((x₁ + x₂ + x₃)/3, (y₁ + y₂ + y₃)/3) A = ½|x₁(y₂ − y₃) + x₂(y₃ − y₁) + x₃(y₁ − y₂)| |x₁ y₁ 1; x₂ y₂ 1; x₃ y₃ 1| = 0 Ax² + Bxy + Cy² + Dx + Ey + F = 0 y² = 4ax x² = 4ay (x − h)² = 4p(y − k) (y − k)² = 4p(x − h) x²/a² + y²/b² = 1 x²/a² − y²/b² = 1 x² + y² + 2gx + 2fy + c = 0 (r, θ) x = r cos θ y = r sin θ r = √(x² + y²) θ = tan⁻¹(y/x) PA = PB |PA| = |PB| dₓ = |y| dᵧ = |x| (+,+) (−,+) (−,−) (+,−) (x, y)ᵀ z = x + yi Re(z) = x Im(z) = y (y − y₁)/(y₂ − y₁) = (x − x₁)/(x₂ − x₁) |x y 1; x₁ y₁ 1; x₂ y₂ 1| = 0 A₁x + B₁y + C₁ = 0 A₂x + B₂y + C₂ = 0 x = (B₁C₂ − B₂C₁)/(A₁B₂ − A₂B₁) y = (C₁A₂ − C₂A₁)/(A₁B₂ − A₂B₁) L₁ + λL₂ = 0 L₁L₂ = 0 d = |C₂ − C₁|/√(A² + B²) tan θ = |(A₁B₂ − A₂B₁)/(A₁A₂ + B₁B₂)| (A₁x + B₁y + C₁)/√(A₁² + B₁²) = ±(A₂x + B₂y + C₂)/√(A₂² + B₂²) ax² + 2hxy + by² = 0 tan θ = 2√(h² − ab)/(a + b) a + b = 0 h² ≥ ab h² = ab Δc = B² − 4AC B² − 4AC < 0 B² − 4AC = 0 B² − 4AC > 0 (x − h)²/a² + (y − k)²/b² = 1 (x − h)²/a² − (y − k)²/b² = 1 (y − k)²/a² − (x − h)²/b² = 1 c² = a² − b² c² = a² + b² e = c/a PF/PD = e x = ±a/e y − k = ±(b/a)(x − h) y − k = ±(a/b)(x − h) (a cos t, b sin t) (a sec t, b tan t) (at², 2at) xx₁/a² + yy₁/b² = 1 xx₁/a² − yy₁/b² = 1 yy₁ = 2a(x + x₁) xx₁ + yy₁ = R² T = S₁ S₁ − S₂ = 0 Pow(P) = PO² − R² PT² = Pow(P) d² = R₁² + R₂² [X : Y : W] x = X/W y = Y/W [X : Y : 0] p = [X, Y, W]ᵀ ℓ = [a, b, c]ᵀ ℓᵀp = 0 ℓ = p₁ × p₂ p = ℓ₁ × ℓ₂ pᵀCp = 0 p′ = Ap + t p′ = Ap [x′; y′] = [a b; c d][x; y] + [e; f] R(θ) = [cos θ −sin θ; sin θ cos θ] S = [sₓ 0; 0 sᵧ] Hₓ = [1 k; 0 1] Hᵧ = [1 0; k 1] Fₓ = [1 0; 0 −1] Fᵧ = [−1 0; 0 1] Fₒ = [−1 0; 0 −1] det(A) = ad − bc Area′ = |det(A)|Area T = T₃T₂T₁ p = A⁻¹(p′ − t) P = αA + βB + γC α + β + γ = 1 P(α : β : γ) P = (αx₁ + βx₂ + γx₃, αy₁ + βy₂ + γy₃) G(1 : 1 : 1) I(a : b : c) P(x₁, y₁, z₁) v = ⟨a, b, c⟩ r = r₀ + λv x = x₀ + aλ, y = y₀ + bλ, z = z₀ + cλ (x − x₀)/a = (y − y₀)/b = (z − z₀)/c Ax + By + Cz + D = 0 n = ⟨A, B, C⟩ (r − r₀) · n = 0 A(x − x₀) + B(y − y₀) + C(z − z₀) = 0 d = |Ax₀ + By₀ + Cz₀ + D|/√(A² + B² + C²) cos θ = |n₁ · n₂|/(|n₁||n₂|) sin θ = |v · n|/(|v||n|) n₁ × n₂ = 0 n₁ · n₂ = 0 a · (b × c) = 0 d = |(r₂ − r₁) · (v₁ × v₂)|/|v₁ × v₂| (x − a)² + (y − b)² + (z − c)² = R² x² + y² + z² + ux + vy + wz + d = 0 xx₁ + yy₁ + zz₁ = R² x² + y² = R² x²/a² + y²/b² = 1 x²/a² + y²/b² − z²/c² = 0 x²/a² + y²/b² + z²/c² = 1 x²/a² + y²/b² − z²/c² = 1 z²/c² − x²/a² − y²/b² = 1 z = x²/a² + y²/b² z = x²/a² − y²/b² B(t) = (1 − t)²P₀ + 2(1 − t)tP₁ + t²P₂ B(t) = (1 − t)³P₀ + 3(1 − t)²tP₁ + 3(1 − t)t²P₂ + t³P₃ C(t) = (x(t), y(t)) C(t) = (x(t), y(t), z(t)) F(x, y) = 0 F(x, y, z) = 0

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Space And Time Symbolism

There is no single official master list of "space-time symbols." General relativity, black-hole physics, cosmology, and astronomy use standard notations that vary somewhat by coordinate system and sign convention. For example, Schwarzschild, Eddington-Finkelstein, Kruskal-Szekeres, and Boyer-Lindquist coordinates describe spacetime in different ways, while astronomers commonly locate objects with right ascension and declination.

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Hover over any particulate to observe its customary mathematical function, then select it to replicate the notation for worksheets, formulas, diagrams, instructional pages, or personal records.

x^μ {x^μ} (x⁰, x¹, x², x³) (ct, X, Y, Z) (ct, R, ϑ, ϕ) 𝒫(x^μ) Δt_coord Δτ_prop dℓ_prop ds² Δs² Δs² = −c²Δt² + ΔX² + ΔY² + ΔZ² Δs² = c²Δt² − ΔX² − ΔY² − ΔZ² Δs² = 0 Δs² < 0 Δs² > 0 g_{μν} g^{μν} η_{μν} η_{μν} = diag(−1, +1, +1, +1) η_{μν} = diag(+1, −1, −1, −1) ds² = g_{μν}dx^μdx^ν x_μ = g_{μν}x^ν g_{μρ}g^{ρν} = δ_μ^ν g_det = det(g_{μν}) d⁴V = √(−g_det)d⁴x Γ^ρ_{μν} ∇*μV^ν R^ρ*{σμν} R_{μν} R_scalar G_{μν} T_{μν} Λ_cos g_{μν} G_{μν} + Λ_cos g_{μν} = (8πG/c⁴)T_{μν} u^μ = dx^μ/dτ_prop g_{μν}u^μu^ν = −c² k^μk_μ = 0 d²x^μ/dτ_prop² + Γ^μ_{αβ}(dx^α/dτ_prop)(dx^β/dτ_prop) = 0 ∇_μT^{μν} = 0 (t_S, r_S, ϑ_S, ϕ_S) r_sch = 2GM_BH/c² r_S = r_sch r_S > r_sch 0 < r_S < r_sch r_S → 0 dΩ_S² = dϑ_S² + sin²ϑ_S dϕ_S² ds² = −(1 − r_sch/r_S)c²dt_S² + (1 − r_sch/r_S)⁻¹dr_S² + r_S²dΩ_S² r_ph = 3GM_BH/c² r_ISCO = 6GM_BH/c² A_sch = 4πr_sch² r_tort = r_S + r_sch ln|r_S/r_sch − 1| u_EF = ct_S − r_tort v_EF = ct_S + r_tort (v_EF, r_S, ϑ_S, ϕ_S) (u_EF, r_S, ϑ_S, ϕ_S) ds² = −(1 − r_sch/r_S)dv_EF² + 2dv_EFdr_S + r_S²dΩ_S² U_KS = −exp(−u_EF/2r_sch) V_KS = exp(v_EF/2r_sch) (U_KS, V_KS, ϑ_S, ϕ_S) T_KS = (V_KS + U_KS)/2 X_KS = (V_KS − U_KS)/2 X_KS² − T_KS² = (r_S/r_sch − 1)exp(r_S/r_sch) (t_BL, r_BL, ϑ_BL, ϕ_BL) a_Kerr = J_BH/(M_BHc) χ_BH = J_BHc/(GM_BH²) |χ_BH| ≤ 1 Σ_Kerr = r_BL² + a_Kerr²cos²ϑ_BL Δ_Kerr = r_BL² − r_sch r_BL + a_Kerr² r_+BH = (r_sch + √(r_sch² − 4a_Kerr²))/2 r_−BH = (r_sch − √(r_sch² − 4a_Kerr²))/2 r_ergo(ϑ_BL) = (r_sch + √(r_sch² − 4a_Kerr²cos²ϑ_BL))/2 Ω_H = a_Kerr c/(r_+BH² + a_Kerr²) A_Kerr = 4π(r_+BH² + a_Kerr²) κ_Kerr = c²(r_+BH − r_−BH)/(2(r_+BH² + a_Kerr²)) T_Hawk = ħκ_Kerr/(2πck_B) S_BH = k_Bc³A_Kerr/(4Għ) x_LC⁺ = ct + X x_LC⁻ = ct − X u_ret = t − R/c v_adv = t + R/c 𝓘⁺ 𝓘⁻ i_spatial⁰ i_time⁺ i_time⁻ ℋ_event⁺ ℋ_event⁻ J⁺(𝒫) J⁻(𝒫) I⁺(𝒫) I⁻(𝒫) dŝ² = Ω_conf²ds² Ω_conf → 0 (t_cos, χ_cos, ϑ_cos, ϕ_cos) (η_cos, χ_cos, ϑ_cos, ϕ_cos) R_phys(t) = a_cos(t)χ_cos dη_cos = cdt_cos/a_cos(t) χ_cos = ∫cdt_cos/a_cos(t) H_cos(t) = ȧ_cos(t)/a_cos(t) 1 + z_cos = a_cos(t₀)/a_cos(t_emit) k_cos ∈ {−1, 0, +1} ds² = −c²dt_cos² + a_cos²(t)[dχ_cos² + S_k²(χ_cos)dΩ_cos²] dΩ_cos² = dϑ_cos² + sin²ϑ_cos dϕ_cos² D_C,cos D_A,cos D_L,cos D_L,cos = (1 + z_cos)²D_A,cos (RA_sky, DEC_sky) RA_sky = hh:mm:ss DEC_sky = ±dd:mm:ss α_sky = 15° × RA_hours (ℓ_gal, b_gal) (λ_ecl, β_ecl) (Az_obs, Alt_obs) HA_local = LST − RA_sky ICRS-frame Epoch J2000.0 Epoch B1950.0 RA--TAN DEC--TAN GLON--TAN GLAT--TAN h_+(u_ret) h_×(u_ret) h^{GW}*{μν} g*{μν} = η_{μν} + h^{GW}_{μν} Φ_GW = k_μx^μ Ω_orb = 2πf_orb f_GW = 2f_orb 𝓜_chirp = (M₁M₂)^{3/5}/(M₁ + M₂)^{1/5}

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History Of Geometry and Space-Time Symbols

Basic History

Long before geometry became an academic subject, it served ordinary human needs. Ancient communities used measurements, proportions, lines, and angles to divide land, construct buildings, store food, track seasons, and organize trade.

Around 1500 BCE, the scribe Ahmose copied The Egyptian Rhind Mathematical Papyrus from older material. It contained dozens of mathematical problems. Some concern everyday activities such as distributing food, while others explain practical geometry, including how to calculate the slope of a pyramid.

Then around 300 BCE, Euclid of Alexandria gathered earlier geometric knowledge into The Elements. His system began with basic ideas such as points, lines, circles, angles, and equality, then used definitions and postulates to construct increasingly complex proofs. Euclid’s work influenced mathematical education for more than two thousand years and helped establish the familiar visual language of dots, straight edges, intersections, triangles, and circular forms.

As time moved forward and during the Middle Ages, scholars began exploring ways to represent changing quantities spatially. Nicole Oresme, who lived from about 1323 to 1382, used arrangements resembling coordinate graphs centuries before the modern Cartesian plane. A major turning point arrived in 1637, when René Descartes published La Géométrie and demonstrated how algebraic equations could represent geometric curves. Numbers, letters, axes, and ordered positions could now describe the same shapes that had previously been constructed mainly with compasses and straightedges.

Coordinate Geometry

Coordinate geometry soon became useful far beyond mathematics.

A location could be expressed with numerical coordinates, a road or boundary could be modeled as a line, and a curved path could be represented by an equation. Over time, these methods became fundamental to surveying, architecture, navigation, engineering, mechanical design, mapmaking, and eventually computer graphics.

The development of non-Euclidean geometry during the nineteenth century further revealed that geometry did not have to describe only flat surfaces; different mathematical spaces could possess their own definitions of distance, direction, and curvature.

In 1908, Hermann Minkowski introduced a four-dimensional interpretation in which three dimensions of space and one dimension of time form a single spacetime continuum. Under this approach, coordinates do not merely identify where an object exists; they can identify an event occurring at a particular place and time.

Albert Einstein developed general relativity between 1908 and 1915 and published a major overview in 1916, describing gravity not simply as an ordinary pulling force but as an effect associated with the geometry of spacetime. This required a new symbolic language involving coordinates, metrics, tensors, derivatives, curvature, mass, and energy.

The same notation opened a path toward the mathematical study of black holes.

In 1916, Karl Schwarzschild obtained the first solution describing a nonrotating, spherically symmetric gravitational field under Einstein’s theory. In 1963, Roy Kerr discovered the corresponding solution for a rotating mass. Coordinates such as Schwarzschild and Boyer–Lindquist coordinates allow physicists to distinguish an exterior region, an event horizon, an interior region, and other structures such as photon orbits and ergospheres. These symbols do not draw a black hole directly; instead, they encode how distance, time, light, and motion behave around it.

Galaxian Geometrical Thinking

Geometry also became the addressing system of the sky. Astronomers use angular coordinates, reference frames, distances, redshifts, and epochs to distinguish one star or galaxy from another. Modern surveys combine billions of such measurements to construct three-dimensional maps of the universe.

The European Space Agency’s Euclid mission, launched on July 1, 2023, was designed to map large-scale cosmic structure across more than one-third of the sky and study how galaxies, gravity, dark matter, and cosmic expansion have developed over billions of years.

Mathematical and geometric symbols have even been used in attempts to communicate beyond Earth.

Pioneer 10, launched in 1972, carried a plaque intended to identify its origin should another intelligence encounter it.

In 1974, the Arecibo message transmitted 1,679 binary digits toward the globular cluster M13, encoding numbers, chemical information, DNA, a human figure, the solar system, and the transmitting telescope.

The Voyager spacecraft, launched in 1977, carried Golden Records whose covers use binary quantities, a hydrogen transition as a time standard, and a map locating the Sun relative to 14 pulsars. These efforts were built on the hope that physical relationships, counting, proportion, and astronomical coordinates might be more universally recognizable than any human language.

What Do Geometry Symbols Mean?

Geometry and coordinate symbols are compact instructions for describing position, size, direction, motion, and relationships. A point names a location, an ordered pair supplies its coordinates, an arrow indicates direction, and an equation defines a line, curve, transformation, or surface. Subscripts distinguish related values, superscripts can represent powers or raised indices, and Greek letters frequently identify angles, parameters, curvature, or other quantities. Their meanings come from the mathematical system in which they appear rather than from the appearance of the characters alone.

Within relativity and astronomy, the notation expands from ordinary locations to events distributed across space and time. Metrics describe how intervals are measured, tensors represent matter and curvature, black-hole coordinates organize regions of extreme gravity, and celestial coordinates identify positions among stars and galaxies. When placed on an interstellar message, the same symbols become an attempted bridge between intelligences: not proof of extraterrestrial knowledge or a secret cosmic alphabet, but a carefully arranged expression of patterns that may arise from the shared physics of the universe.

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