Angular diameter
How large a sphere or circle appears
title: "Angular diameter" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["elementary-geometry", "astrometry", "angle", "equations-of-astronomy"] description: "How large a sphere or circle appears" topic_path: "science/mathematics" source: "https://en.wikipedia.org/wiki/Angular_diameter" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0
::summary How large a sphere or circle appears ::
::figure[src="https://upload.wikimedia.org/wikipedia/commons/e/ed/Angular_diameter.jpg" caption="Angular diameter: the angle subtended by an object"] ::
The angular diameter, angular width, angular size, apparent diameter, or apparent size is an angular separation (in units of angle) describing how large a sphere or circle appears from a given point of view. In the vision sciences, it is called the visual angle, and in optics, it is the angular aperture (of a lens). The angular diameter can alternatively be thought of as the angular displacement through which an eye or camera must rotate to look from one side of an apparent circle to the opposite side.
A person can resolve with their naked eyes diameters down to about 1 arcminute (approximately 0.017° or 0.0003 radians). This corresponds to 0.3 m at a 1 km distance, or to perceiving Venus as a disk under optimal conditions.
Formulation
::figure[src="https://upload.wikimedia.org/wikipedia/commons/c/ce/Angular_diameter_formula.svg" caption="Diagram for the formula of the angular diameter"] ::
The angular diameter of a circle whose plane is perpendicular to the displacement vector between the point of view and the center of said circle can be calculated using the formula :\delta = 2\arctan \left(\frac{d}{2D}\right), in which \delta is the angular diameter (in units of angle, normally radians, sometimes in degrees, depending on the arctangent implementation), d is the linear diameter of the object (in units of length), and D is the distance to the object (also in units of length). When D \gg d, we have: :\delta \approx d / D, and the result obtained is necessarily in radians.
For a sphere
For a spherical object whose linear diameter equals d and where D is the distance to the center of the sphere, the angular diameter can be found by the following modified formula :\delta = 2\arcsin \left(\frac{d}{2D}\right)
Such a different formulation is because the apparent edges of a sphere are its tangent points, which are closer to the observer than the center of the sphere, and have a distance between them which is smaller than the actual diameter. The above formula can be found by understanding that in the case of a spherical object, a right triangle can be constructed such that its three vertices are the observer, the center of the sphere, and one of the sphere's tangent points, with D as the hypotenuse and \frac{d_\mathrm{act}}{2D} as the sine.
The formula is related to the zenith angle to the horizon, :\delta = \pi - 2\arccos\left(\frac{R}{R+h}\right) where R is the radius of the sphere and h is the distance to the near surface of the sphere.
The difference with the case of a perpendicular circle is significant only for spherical objects of large angular diameter, since the following small-angle approximations hold for small values of x: :\arcsin x \approx \arctan x \approx x.
Estimating angular diameter using the hand
::figure[src="https://upload.wikimedia.org/wikipedia/commons/7/79/Estimating_angular_size_with_hand.gif" caption="Approximate angles of 10°, 20°, 5°, and 1° for the hand outstretched at arm's length"] ::
Estimates of angular diameter may be obtained by holding the hand at right angles to a fully extended arm, as shown in the figure.
Use in astronomy
::figure[src="https://upload.wikimedia.org/wikipedia/commons/f/f9/Elements_of_astronomy-_accompanied_with_numerous_illustrations,_a_colored_representation_of_the_solar,_stellar,_and_nebular_spectra,and_celestial_charts_of_the_northern_and_the_southern_hemisphere(14804687203).jpg" caption="A 19th century depiction of the apparent size of the Sun as seen from the Solar System's planets (including asteroids [[72 Feronia]] and [[65 Cybele]], here ''Maximiliana'')."] ::
In astronomy, the sizes of celestial objects are often given in terms of their angular diameter as seen from Earth, rather than their actual sizes. Since these angular diameters are typically small, it is common to present them in arcseconds (). An arcsecond is 1/3600th of one degree (1°) and a radian is 180/π degrees. So one radian equals 3,600 × 180/\pi arcseconds, which is about 206,265 arcseconds (1 rad ≈ 206,264.806247"). Therefore, the angular diameter of an object with physical diameter d at a distance D, expressed in arcseconds, is given by: :\delta = 206,265 ~ (d / D) ~ \mathrm{arcseconds}.
These objects have an angular diameter of 1:
- an object of diameter 1 cm at a distance of 2.06 km
- an object of diameter 725.27 km at a distance of 1 astronomical unit (AU)
- an object of diameter 45 866 916 km at 1 light-year
- an object of diameter 1 AU (149 597 871 km) at a distance of 1 parsec (pc)
Thus, the angular diameter of Earth's orbit around the Sun as viewed from a distance of 1 pc is 2, as 1 AU is the mean radius of Earth's orbit.
The angular diameter of the Sun, from a distance of one light-year, is 0.03, and that of Earth 0.0003. The angular diameter 0.03 of the Sun given above is approximately the same as that of a human body at a distance of the diameter of Earth.
This table shows the angular sizes of noteworthy celestial bodies as seen from Earth, and various other noteworthy celestial objects:
::data[format=table]
| Celestial object | Angular diameter or size | Relative size |
|---|---|---|
| Magellanic Stream | over 100° | |
| Gum Nebula | 36° | |
| Milky Way | 30° (by 360°) | |
| Width of spread out hand with arm stretched out | 20° | covering 353 meter of something viewed from a distance of 1 km |
| Serpens-Aquila Rift | 20° by 10° | |
| Jupiter in the sky of Io | 19.5° | |
| Canis Major Overdensity | 12° by 12° | |
| Smith's Cloud | 11° | |
| Large Magellanic Cloud | 10.75° by 9.17° | Note: brightest galaxy, other than the Milky Way, in the night sky (0.9 apparent magnitude (V)) |
| Barnard's Loop | 10° | |
| Zeta Ophiuchi Sh2-27 nebula | 10° | |
| Width of fist with arm stretched out | 10° | covering 175 meter of something viewed from a distance of 1 km |
| Sagittarius Dwarf Spheroidal Galaxy | 7.5° by 3.6° | |
| Northern Coalsack Nebula | 7° by 5° | |
| Coalsack Nebula | 7° by 5° | |
| Cygnus OB7 | 4° by 7° | |
| Huya's moon (from the surface of 38628 Huya) | 6° 25” | Largest moon from the perspective of a dwarf planet (?) primary |
| Rho Ophiuchi cloud complex | 4.5° by 6.5° | |
| Hyades | 5°30 | Note: brightest star cluster in the night sky, 0.5 apparent magnitude (V) |
| Small Magellanic Cloud | 5°20 by 3°5 | |
| Saturn in the sky of Titan | 5.09° | |
| Andromeda Galaxy | 3°10 by 1° | About six times the size of the Sun or the Moon. Only the much smaller core is visible without long-exposure photography. |
| Charon (from the surface of Pluto) | 3°9’ | |
| Veil Nebula | 3° | |
| Heart Nebula | 2.5° by 2.5° | |
| Westerhout 5 | 2.3° by 1.25° | |
| Sh2-54 | 2.3° | |
| Carina Nebula | 2° by 2° | Note: brightest nebula in the night sky, 1.0 apparent magnitude (V) |
| North America Nebula | 2° by 100 | |
| Earth in the Moon's sky | 2° - 1°48 | Appearing about three to four times larger than the Moon in Earth's sky |
| Moon as it appeared in Earth's sky 3.9 billion years ago | 1.5° | title=Earth-Moon Dynamics |
| The Sun in the sky of Mercury | 1.15° - 1.76° | title=The Sun and Transits as Seen From the Planets |
| Orion Nebula | 1°5 by 1° | |
| Width of little finger with arm stretched out | 1° | covering 17.5 meter of something viewed from a distance of 1 km |
| The Sun in the sky of Venus | 0.7° | title=How large does the Sun appear from Mercury and Venus, as compared to how we see it from Earth? |
| Io (as seen from the “surface” of Jupiter) | 35’ 35” | |
| Moon | 346 – 2920 | 32.5–28 times the maximum value for Venus (orange bar below) / 2046–1760 the Moon has a diameter of 3,474 km |
| Sun | 3232 – 3127 | 31–30 times the maximum value for Venus (orange bar below) / 1952–1887 the Sun has a diameter of 1,391,400 km |
| Triton (from the “surface” of Neptune) | 28’ 11” | |
| Angular size of the distance between Earth and the Moon as viewed from Mars, at inferior conjunction | about 25 | |
| Ariel (from the “surface” of Uranus) | 24’ 11” | |
| Ganymede (from the “surface” of Jupiter) | 18’ 6” | |
| Europa (from the “surface” of Jupiter) | 17’ 51” | |
| Umbriel (from the “surface” of Uranus) | 16’ 42” | |
| Helix Nebula | about 16 by 28 | |
| Miranda (from the “surface” of Uranus) | 15’ 30” | |
| Tethys (from the “surface” of Saturn) | 15’ 30” | |
| Titan (from the “surface” of Saturn) | 15’ 12” | |
| Titania (from the “surface” of Uranus) | 13’ 12” | |
| Phobos (from the surface of Mars) | 12’ 56” | |
| Dione (from the “surface” of Saturn) | 12’ 5” | |
| Rhea (from the “surface” of Saturn) | 11’ 12” | |
| Mimas (from the “surface” of Saturn) | 10’ 42” | |
| Enceladus (from the “surface” of Saturn) | 9’ 38” | |
| Oberon (from the “surface” of Uranus) | 9’ 22” | |
| Callisto (from the “surface” of Jupiter) | 9’ 8” | |
| Jupiter if it were as close to Earth as Mars | 9.0 – 1.2 | |
| Spire in Eagle Nebula | 440 | length is 280 |
| Deimos (from the surface of Mars) | 2’ 7” | |
| Iapetus (from the “surface” of Saturn) | 1’ 26” | |
| Venus | – | |
| International Space Station (ISS) | 13 | title=Problem 346: The International Space Station and a Sunspot: Exploring angular scales |
| Minimum resolvable diameter by the human eye | 1 | 0.3 meter at 1 km distance |
| About 100 km on the surface of the Moon | 1 | Comparable to the size of features like large lunar craters, such as the Copernicus crater, a prominent bright spot in the eastern part of Oceanus Procellarum on the waning side, or the Tycho crater within a bright area in the south, of the lunar near side. |
| Jupiter | 50.1 – 29.8 | |
| Earth as seen from Mars | 48.2 – 6.6 | |
| Minimum resolvable gap between two lines by the human eye | 40 | last=Wong |
| Mars | 25.1 – 3.5 | |
| Saturn | 20.1 – 14.5 | |
| Mercury | 13.0 – 4.5 | |
| Earth's Moon as seen from Mars | 13.27 – 1.79 | |
| Uranus | 4.1 – 3.3 | |
| Neptune | 2.4 – 2.2 | |
| Apparent size of Sun, seen from 90377 Sedna at aphelion | 2.04" | |
| Ganymede | 1.8 – 1.2 | Ganymede has a diameter of 5,268 km |
| An astronaut (~1.7 m) at a distance of 350 km, the average altitude of the ISS | 1 | |
| Minimum resolvable diameter by Galileo Galilei's largest 38mm refracting telescopes | ~1 | last=Graney |
| Ceres | 0.84 – 0.33 | |
| Vesta | 0.64 – 0.20 | |
| Pluto | 0.11 – 0.06 | |
| Eris | 0.089 – 0.034 | |
| R Doradus | 0.062 – 0.052 | Note: R Doradus is thought to be the extrasolar star with the largest apparent size as viewed from Earth |
| Betelgeuse | 0.060 – 0.049 | |
| Alphard | 0.00909 | |
| Alpha Centauri A | 0.007 | |
| Canopus | 0.006 | |
| Sirius | 0.005936 | |
| Altair | 0.003 | |
| Rho Cassiopeiae | 0.0021 | |
| Deneb | 0.002 | |
| Proxima Centauri | 0.001 | |
| Alnitak | 0.0005 | |
| Proxima Centauri b | 0.00008 | |
| Event horizon of black hole M87* at center of the M87 galaxy, imaged by the Event Horizon Telescope in 2019. | 0.000025 | Comparable to a tennis ball on the Moon |
| A star like Alnitak at a distance where the Hubble Space Telescope would just be able to see it | arcsec | |
| :: |
::figure[src="https://upload.wikimedia.org/wikipedia/commons/3/38/Diffraction_limit_diameter_vs_angular_resolution.svg" caption="Log-log plot of [[aperture]] diameter vs [[angular resolution]] at the diffraction limit for various light wavelengths compared with various astronomical instruments. For example, the blue star shows that the [[Hubble Space Telescope]] is almost diffraction-limited in the visible spectrum at 0.1 arcsecs, whereas the red circle shows that the human eye should have a resolving power of 20 arcsecs in theory, though normally only 60 arcsecs."] ::
::figure[src="https://upload.wikimedia.org/wikipedia/commons/f/f8/Comparison_angular_diameter_solar_system.svg" caption="Comparison of angular diameter of the Sun, Moon and planets. To get a true representation of the sizes, view the image at a distance of 103 times the width of the "Moon: max." circle. For example, if this circle is 5 cm wide on your monitor, view it from 5.15 m away."] ::
::figure[src="https://upload.wikimedia.org/wikipedia/commons/2/20/Jupiter.mit.Io.Ganymed.Europa.Calisto.Vollmond.10.4.2017.jpg" caption="conjunction]] on 10 April 2017."] ::
The angular diameter of the Sun, as seen from Earth, is about 250,000 times that of Sirius. (Sirius has twice the diameter and its distance is 500,000 times as much; the Sun is 1010 times as bright, corresponding to an angular diameter ratio of 105, so Sirius is roughly 6 times as bright per unit solid angle.)
The angular diameter of the Sun is also about 250,000 times that of Alpha Centauri A (it has about the same diameter and the distance is 250,000 times as much; the Sun is 4×1010 times as bright, corresponding to an angular diameter ratio of 200,000, so Alpha Centauri A is a little brighter per unit solid angle).
The angular diameter of the Sun is about the same as that of the Moon. (The Sun's diameter is 400 times as large and its distance also; the Sun is 200,000 to 500,000 times as bright as the full Moon (figures vary), corresponding to an angular diameter ratio of 450 to 700, so a celestial body with a diameter of 2.5–4 and the same brightness per unit solid angle would have the same brightness as the full Moon.)
Even though Pluto is physically larger than Ceres, when viewed from Earth (e.g., through the Hubble Space Telescope) Ceres has a much larger apparent size.
Angular sizes measured in degrees are useful for larger patches of sky. (For example, the three stars of the Belt cover about 4.5° of angular size.) However, much finer units are needed to measure the angular sizes of galaxies, nebulae, or other objects of the night sky.
Degrees, therefore, are subdivided as follows:
- 360 degrees (°) in a full circle
- 60 arc-minutes () in one degree
- 60 arc-seconds () in one arc-minute
To put this in perspective, the full Moon as viewed from Earth is about °, or 30 (or 1800). The Moon's motion across the sky can be measured in angular size: approximately 15° every hour, or 15 per second. A one-mile-long line painted on the face of the Moon would appear from Earth to be about 1 in length.
In astronomy, it is typically difficult to directly measure the distance to an object, yet the object may have a known physical size (perhaps it is similar to a closer object with known distance) and a measurable angular diameter. In that case, the angular diameter formula can be inverted to yield the angular diameter distance to distant objects as :d \equiv 2 D \tan \left( \frac{\delta}{2} \right).
In non-Euclidean space, such as our expanding universe, the angular diameter distance is only one of several definitions of distance, so that there can be different "distances" to the same object. See Distance measures (cosmology).
Non-circular objects
Many deep-sky objects such as galaxies and nebulae appear non-circular and are thus typically given two measures of diameter: major axis and minor axis. For example, the Small Magellanic Cloud has a visual apparent diameter of × .
Defect of illumination
Defect of illumination is the maximum angular width of the unilluminated part of a celestial body seen by a given observer. For example, if an object is 40 of arc across and is 75% illuminated, the defect of illumination is 10.
Horizon effect
Adding to the apparent size as an angular size depending on distance, is the issue of the horizon effect. When viewing a spacious non-transcluscent object it is not viewed as a whole at the edges, making it not visible in its full width.
References
References
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- Michael A. Seeds. (2010). "Stars and Galaxies". Brooks Cole.
- O'Meara, Stephen James. (2019-08-06). "The coalsacks of Cygnus".
- (2014-11-24). "Colliding Filaments and a Massive Dense Core in the Cygnus Ob 7 Molecular Cloud". American Astronomical Society.
- (2023-03-24). "Earth observations from the Moon's surface: dependence on lunar libration". Copernicus GmbH.
- "Earth-Moon Dynamics".
- (2018-11-05). "The Sun and Transits as Seen From the Planets".
- (2018-05-31). "How large does the Sun appear from Mercury and Venus, as compared to how we see it from Earth?".
- (2018-08-19). "Problem 346: The International Space Station and a Sunspot: Exploring angular scales".
- Wong, Yan. (2016-01-24). "How small can the naked eye see?".
- (2016-09-07). "Sharp eyes: how well can we really see?".
- Graney, Christopher M.. (Dec 10, 2006). "The Accuracy of Galileo's Observations and the Early Search for Stellar Parallax".
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- (2024-08-05). "CHARA Near-Infrared Imaging of the Yellow Hypergiant Star $\rho$ Cassiopeiae: Convection Cells and Circumstellar Envelope".
- 800 000 times smaller angular diameter than that of Alnitak as seen from Earth. Alnitak is a blue star so it gives off a lot of light for its size. If it were 800 000 times further away then it would be magnitude 31.5, at the limit of what Hubble can see.
- "HORIZON EFFECT".
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