See photon sphere in All languages combined, or Wiktionary
Download JSON data for photon sphere meaning in English (5.6kB)
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"2": "photon",
"3": "sphere"
},
"expansion": "photon + sphere",
"name": "compound"
}
],
"etymology_text": "photon + sphere.",
"forms": [
{
"form": "photon spheres",
"tags": [
"plural"
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"expansion": "photon sphere (plural photon spheres)",
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"pos": "noun",
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{
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"kind": "other",
"name": "English entries with incorrect language header",
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"kind": "topical",
"langcode": "en",
"name": "Black holes",
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"name": "Light",
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"kind": "topical",
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"name": "Orbits",
"orig": "en:Orbits",
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"examples": [
{
"text": "The radius of the photon sphere is also the lower bound for any stable orbit.",
"type": "example"
},
{
"text": "For a Schwarzschild (non-spinning) black hole, the radius of the photon sphere is 1.5 times the Schwarzschild radius.",
"type": "example"
},
{
"ref": "2000, Edward Harrison, Cosmology, 2nd edition, Cambridge University Press, page 250",
"text": "The redshift of light leaking outward from the photon sphere is #x5C;sqrt#x7B;3#x7D;-1#x3D;0.732. All light rays approaching a black hole closer than #x5C;sqrt#x7B;3#x7D; times the radius of the photon sphere spiral inwards and are captured (see Figure 13.5).",
"type": "quotation"
},
{
"ref": "2015, Katherine Blundell, Black Holes: A Very Short Introduction, Oxford University Press, page 44",
"text": "For a Kerr black hole though, one that has spin, the situation is different for the orbits near the black hole. In particular, there are two photon spheres, in contrast with the one photon sphere around a stationary Schwarzschild black hole. The outermost sphere is for photons that are orbiting oppositely to the direction of rotation of the black hole (the ones we say are on retrograde orbits). Inside this is the photon sphere for photons travelling in the same sense around the black hole as it is rotating (on prograde orbits). For a very slowly rotating black hole that isn't so very different from a Schwarzschild black hole, these two photon spheres are very nearly co-spatial. For black holes of increasing spin, these surfaces are increasingly further apart.",
"type": "quotation"
},
{
"text": "2017, Lori Gardi, The Mandelbrot Set as a Quasi-Black Hole, David de Hilster (editor), John Chappell Natural Philosophy Society: 2017 Proceedings, John Chappell Natural Philosophy Society, page 65,\nThe lesser known region just outside the black hole is referred to as the photon sphere (outer grey region in Figure 9). The photon sphere is a region of space just outside the black hole where photons are forced to travel in complex orbits due to the extreme curvature of space within this region [2]. […] Finally, the boundary that exactly separates the black hole from the photon sphere is referred to as the event horizon (white circle surrounding the black region in Figure 9)."
},
{
"ref": "2022, Wouter Schmitz, Understanding Relativity, Springer, page 277",
"text": "The region inside the photon sphere has a diameter of 1.5× Schwarzschild diameter D(s), but due to the curvature, this region gets magnified to 2.6× D(s).",
"type": "quotation"
}
],
"glosses": [
"A spherical limit around a black hole at such distance that any photon meeting it tangentially is constrained to travel in a circular orbit; (more loosely) the region between this limit and the event horizon."
],
"id": "en-photon_sphere-en-noun-ZW~EwN6a",
"links": [
[
"black hole",
"black hole"
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[
"orbit",
"orbit"
],
[
"event horizon",
"event horizon"
]
],
"raw_glosses": [
"(of a black hole) A spherical limit around a black hole at such distance that any photon meeting it tangentially is constrained to travel in a circular orbit; (more loosely) the region between this limit and the event horizon."
],
"raw_tags": [
"of a black hole"
],
"related": [
{
"word": "accretion disc"
},
{
"word": "black hole"
},
{
"word": "black hole jet"
},
{
"word": "ergosphere"
},
{
"word": "event horizon"
},
{
"word": "innermost stable circular orbit"
},
{
"english": "visible surface of a star",
"word": "photosphere"
},
{
"word": "Roche limit"
},
{
"word": "singularity"
}
],
"synonyms": [
{
"word": "photon circle"
},
{
"word": "last photon orbit"
}
],
"translations": [
{
"code": "fr",
"lang": "French",
"sense": "spherical boundary surrounding a black hole in which photons travel in circular orbits",
"tags": [
"feminine"
],
"word": "sphère de photons"
},
{
"code": "fr",
"lang": "French",
"sense": "spherical boundary surrounding a black hole in which photons travel in circular orbits",
"tags": [
"feminine"
],
"word": "sphère photonique"
},
{
"code": "it",
"lang": "Italian",
"sense": "spherical boundary surrounding a black hole in which photons travel in circular orbits",
"tags": [
"feminine"
],
"word": "sfera di fotoni"
},
{
"code": "it",
"lang": "Italian",
"sense": "spherical boundary surrounding a black hole in which photons travel in circular orbits",
"tags": [
"feminine"
],
"word": "sfera fotonica"
}
],
"wikipedia": [
"photon sphere"
]
}
],
"word": "photon sphere"
}
{
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],
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"forms": [
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],
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{
"args": {},
"expansion": "photon sphere (plural photon spheres)",
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"word": "accretion disc"
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{
"word": "black hole"
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{
"word": "black hole jet"
},
{
"word": "ergosphere"
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{
"word": "event horizon"
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{
"word": "innermost stable circular orbit"
},
{
"english": "visible surface of a star",
"word": "photosphere"
},
{
"word": "Roche limit"
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{
"word": "singularity"
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],
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"en:Black holes",
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"examples": [
{
"text": "The radius of the photon sphere is also the lower bound for any stable orbit.",
"type": "example"
},
{
"text": "For a Schwarzschild (non-spinning) black hole, the radius of the photon sphere is 1.5 times the Schwarzschild radius.",
"type": "example"
},
{
"ref": "2000, Edward Harrison, Cosmology, 2nd edition, Cambridge University Press, page 250",
"text": "The redshift of light leaking outward from the photon sphere is #x5C;sqrt#x7B;3#x7D;-1#x3D;0.732. All light rays approaching a black hole closer than #x5C;sqrt#x7B;3#x7D; times the radius of the photon sphere spiral inwards and are captured (see Figure 13.5).",
"type": "quotation"
},
{
"ref": "2015, Katherine Blundell, Black Holes: A Very Short Introduction, Oxford University Press, page 44",
"text": "For a Kerr black hole though, one that has spin, the situation is different for the orbits near the black hole. In particular, there are two photon spheres, in contrast with the one photon sphere around a stationary Schwarzschild black hole. The outermost sphere is for photons that are orbiting oppositely to the direction of rotation of the black hole (the ones we say are on retrograde orbits). Inside this is the photon sphere for photons travelling in the same sense around the black hole as it is rotating (on prograde orbits). For a very slowly rotating black hole that isn't so very different from a Schwarzschild black hole, these two photon spheres are very nearly co-spatial. For black holes of increasing spin, these surfaces are increasingly further apart.",
"type": "quotation"
},
{
"text": "2017, Lori Gardi, The Mandelbrot Set as a Quasi-Black Hole, David de Hilster (editor), John Chappell Natural Philosophy Society: 2017 Proceedings, John Chappell Natural Philosophy Society, page 65,\nThe lesser known region just outside the black hole is referred to as the photon sphere (outer grey region in Figure 9). The photon sphere is a region of space just outside the black hole where photons are forced to travel in complex orbits due to the extreme curvature of space within this region [2]. […] Finally, the boundary that exactly separates the black hole from the photon sphere is referred to as the event horizon (white circle surrounding the black region in Figure 9)."
},
{
"ref": "2022, Wouter Schmitz, Understanding Relativity, Springer, page 277",
"text": "The region inside the photon sphere has a diameter of 1.5× Schwarzschild diameter D(s), but due to the curvature, this region gets magnified to 2.6× D(s).",
"type": "quotation"
}
],
"glosses": [
"A spherical limit around a black hole at such distance that any photon meeting it tangentially is constrained to travel in a circular orbit; (more loosely) the region between this limit and the event horizon."
],
"links": [
[
"black hole",
"black hole"
],
[
"orbit",
"orbit"
],
[
"event horizon",
"event horizon"
]
],
"raw_glosses": [
"(of a black hole) A spherical limit around a black hole at such distance that any photon meeting it tangentially is constrained to travel in a circular orbit; (more loosely) the region between this limit and the event horizon."
],
"raw_tags": [
"of a black hole"
],
"synonyms": [
{
"word": "photon circle"
},
{
"word": "last photon orbit"
}
],
"wikipedia": [
"photon sphere"
]
}
],
"translations": [
{
"code": "fr",
"lang": "French",
"sense": "spherical boundary surrounding a black hole in which photons travel in circular orbits",
"tags": [
"feminine"
],
"word": "sphère de photons"
},
{
"code": "fr",
"lang": "French",
"sense": "spherical boundary surrounding a black hole in which photons travel in circular orbits",
"tags": [
"feminine"
],
"word": "sphère photonique"
},
{
"code": "it",
"lang": "Italian",
"sense": "spherical boundary surrounding a black hole in which photons travel in circular orbits",
"tags": [
"feminine"
],
"word": "sfera di fotoni"
},
{
"code": "it",
"lang": "Italian",
"sense": "spherical boundary surrounding a black hole in which photons travel in circular orbits",
"tags": [
"feminine"
],
"word": "sfera fotonica"
}
],
"word": "photon sphere"
}
This page is a part of the kaikki.org machine-readable English dictionary. This dictionary is based on structured data extracted on 2024-05-01 from the enwiktionary dump dated 2024-04-21 using wiktextract (f4fd8c9 and c9440ce). The data shown on this site has been post-processed and various details (e.g., extra categories) removed, some information disambiguated, and additional data merged from other sources. See the raw data download page for the unprocessed wiktextract data.
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