Occultation
Encyclopedia
An occultation is an event that occurs when one object is hidden by another object that passes between it and the observer. The word is used in astronomy
(see below). It can also refer to any situation wherein an object in the foreground blocks from view (occult
s) an object in the background. In this general sense, occultation applies to the visual scene observed from low-flying aircraft (or computer-generated imagery
) wherein foreground objects obscure distant dynamically, as the scene changes over time.
the larger object, an occultation is also termed a secondary eclipse.
An eclipse occurs when a body disappears or partially disappears from view, either by an occultation, as with a solar eclipse
, or by passing into the shadow of another body, as with a lunar eclipse
(thus both are listed on NASA's eclipse page).
Transits, occultations and eclipses in general are all effects of a syzygy
.
Transits and occultations of the sun by Earth's moon are called solar eclipse
s regardless of whether the sun is completely or partially covered. By extension, transits of the sun by a satellite
of a planet may also be called eclipses, as with the transits of Phobos and Deimos shown here, as may the passage of a satellite into the planet's shadow, as with this eclipse of Phobos. The term eclipse is also used more generally for bodies passing in front of one another. For example, this entry from NASA's Astronomy Picture of the Day refers to the Moon eclipsing and occulting Saturn interchangeably.
passes in front of a star
during the course of its orbital motion around the Earth. Since the Moon, with an angular speed with respect to the stars of 0.55 arcsec/s or 2.7 µrad/s, has no atmosphere and stars have an angular diameter of at most 0.057 arcseconds or 0.28 µrad, a star that is occulted by the moon will disappear or reappear in 0.1 seconds or less on the moon's edge, or limb. Events that take place on the Moon's dark limb are of particular interest to observers, because the lack of glare allows these occultations to more easily be observed and timed.
The Moon's orbit is inclined to the ecliptic
(see orbit of the Moon), and any stars with an ecliptic latitude of less than about 6.5 degrees may be occulted by it. There are three first magnitude stars that are sufficiently close to the ecliptic that they may be occulted by the Moon and by planets – Regulus
, Spica
and Antares
. Occultations of Aldebaran
are presently only possible by the Moon, because the planets pass Aldebaran to the north. Neither planetary nor lunar occultations of Pollux
are currently possible. However, in the far future, occultations of Aldebaran and Pollux will be possible, as they were in the far past. Some deep-sky objects, such as the Pleiades
, can also be occulted by the moon.
Within a few kilometres of the edge of an occultation's predicted path, referred to as its northern or southern limit, an observer may see the star intermittently disappearing and reappearing as the irregular limb of the Moon moves past the star, creating what is known as a Grazing lunar occultation
. From an observational and scientific standpoint, these "grazes" are the most dynamic and interesting of lunar occultations.
The accurate timing of lunar occultations is performed regularly by (primarily amateur) astronomers. Lunar occultations timed to an accuracy of a few tenths of a second have various scientific uses, particularly in refining our knowledge of lunar topography. Photoelectric analysis of lunar occultations have also discovered some stars to be very close visual or spectroscopic binaries
. Some angular diameters of stars have been measured by timing of lunar occultations, which is useful for determining effective temperature
s of those stars. Early radio astronomers found occultations of radio sources by the Moon valuable for determining their exact positions, because the long wavelength of radio waves limited the resolution available through direct observation. This was crucial for the unambiguous identification of the radio source 3C 273 with the optical quasar and its jet, and a fundamental prerequisite for Maarten Schmidt
's discovery of the cosmological nature of quasars.
Several times during the year, someone on Earth can usually observe the Moon occulting a planet. Since planets, unlike stars, have significant angular sizes, lunar occultations of planets will create a narrow zone on earth from which a partial occultation of the planet will occur. An observer located within that narrow zone could observe the planet's disk partly blocked by the slowly moving moon.
occulted Regulus
. Uranus
' rings were first discovered when that planet occulted a star in 1977. On the evening of July 2-July 3, 1989, Saturn
passed in front of the 5th magnitude star 28 Sagittarii
. Pluto, which was re-designated as a dwarf planet in 2006, occulted stars in 1988, 2002, and 2006, allowing its tenuous atmosphere to be studied.
It is also possible for one planet to occult another planet. However, these mutual occultations of planets are extremely rare. The last such event occurred on January 3, 1818 and will next occur on November 22, 2065, in both cases involving the same two planets—Venus and Jupiter. Technically speaking, when the foreground planet is smaller in apparent size than the background planet, the event should be called a "mutual planetary transit." When the foreground planet is larger in apparent size than the background planet, the event should be called a "mutual planetary occultation." (See Transit
for a list of past and future events).
Twice during the orbital cycles of Jupiter and Saturn, the equatorial (and satellite) planes of those planets are aligned with earth's orbital plane, resulting in a series of mutual occultations and eclipses between the moons of these giant planets. These orbital alignments have also occurred artificially when unmanned spacecraft have traversed these planetary systems, resulting in photographs such as the one shown here. The terms "eclipse," "occultation" and "transit" are also used to describe these events. A satellite of Jupiter (for example) may be eclipsed (i.e. made dimmer because it moves into Jupiter's shadow), occulted (i.e. hidden from view because Jupiter lies on our line of sight), or may transit (i.e. pass in front of) Jupiter's disk.
(also known as a minor planet
) passes in front of a star
(occults a star), temporarily blocking its light (as seen from Earth
). Several events occur nearly every day over the world. From any particular place such events occur almost every night, although most require a telescope
to see.
Asteroid occultations are useful for measuring the size and position of asteroids much more precisely than can be done by any other means. A cross-sectional profile of the shape of an asteroid can even be determined if a number of observers at different, nearby, locations observe the occultation. For example, on March 12, 2009 there were 8 minor planet occulations, including (85) Io, (247) Eukrate, (1585) Union, (201) Penelope, (70) Panopaea, (980) Anacostia, (2448) Sholokhov, (1746) Brouwer, and (191) Kolga. Any one of these would be expected to occult at a time and place on the globe, at a certain magnitude, and with a certain star.
For example, according to the 1998 European Asteroidal Occultation Results from Euraster, 39 Laetitia was observed by over 38 observatories in one occultation on March 3, 1998, which resulted in many chords being determined.
Occultations have produced outlines of many asteroids. Some notable ones include:
Occultations have also been used to estimate the diameter of trans-Neptunian object
s such as (55636) 2002 TX300
, 28978 Ixion
, and 20000 Varuna
. Preliminary results of a 6 November 2010 occultation by the dwarf planet Eris
of a magnitude
17 star in the constellation
of Cetus
placed an upper limit on Eris's diameter of 2320 km, making it almost the same size as Pluto. Due to their slower movement through the night sky, occultations by TNOs are far less common than by asteroids in the main-belt.
.
that would work in conjunction with a telescope
to detect planet
s around distant stars. The satellite consists of a large, very lightweight sheet, and a set of maneuvering thrusters and navigation systems. It would maneuver to a position along the line of sight between the telescope and a nearby star. The satellite would thereby block the radiation from the star, permitting the orbiting planets to be observed.
The proposed satellite would have a dimension of 70 m × 70 m, a mass of about 600 kg, and maneuver by means of an ion drive engine in combination with using the sheet as a light sail. Positioned at a distance of 100,000 km from the telescope, it would block more than 99.998% of the starlight.
There are two possible configurations of this satellite. The first would work with a space telescope, most likely positioned near the Earth
's Lagrangian point
. The second would place the satellite in a highly elliptical orbit about the Earth, and work in conjunction with a ground telescope. At the apogee of the orbit, the satellite would remain relatively stationary with respect to the ground, allowing longer exposure times.
An updated version of this design is called the Starshade, which uses a sunflower
-shaped coronagraph
disc. A comparable proposal was also made for a satellite to occult bright X-ray sources, called an X-ray Occulting Steerable Satellite or XOSS.
These events are not visible everywhere the occulting body and the occulted body are above the skyline. Some events are barely visible, because they take place in close proximity to the Sun.
, when Venus near superior conjunction (with an angular diameter
of 10.6") will transit in front of Jupiter
(with an angular diameter of 30.9"); however, this will take place only 8° west of the Sun, and will therefore not be visible to the unaided/unprotected eye. When the nearer object has a larger angular diameter
than the farther object, thus covering it completely, the event is not a transit but an occultation. Before transiting Jupiter, Venus will occult Jupiter's moon
Ganymede
at around 11:24 UTC as seen from some southernmost parts of Earth. Parallax
will cause actual observed times to vary by a few minutes, depending on the precise location of the observer.
There are only 18 mutual planetary transits and occultations as seen from Earth between 1700 and 2200. Note the long break of events between 1818 and 2065.
The 1737 event was observed by John Bevis
at Greenwich Observatory – it is the only detailed account of a mutual planetary occultation. A transit of Mars across Jupiter on 12 Sep 1170 was observed by the monk Gervase at Canterbury
, and by Chinese astronomers. In addition, an occultation of Mars by Venus was observed by M. Möstlin
at Heidelberg
on October 3, 1590.
is a term used to designate the hidden state of the Imam of the Time
.
Astronomy
Astronomy is a natural science that deals with the study of celestial objects and phenomena that originate outside the atmosphere of Earth...
(see below). It can also refer to any situation wherein an object in the foreground blocks from view (occult
Occult
The word occult comes from the Latin word occultus , referring to "knowledge of the hidden". In the medical sense it is used to refer to a structure or process that is hidden, e.g...
s) an object in the background. In this general sense, occultation applies to the visual scene observed from low-flying aircraft (or computer-generated imagery
Computer-generated imagery
Computer-generated imagery is the application of the field of computer graphics or, more specifically, 3D computer graphics to special effects in art, video games, films, television programs, commercials, simulators and simulation generally, and printed media...
) wherein foreground objects obscure distant dynamically, as the scene changes over time.
Occultations, transits and eclipses
An occultation occurs when an apparently larger body passes in front of an apparently smaller one. A transit occurs when an apparently smaller body passes in front of an apparently larger one. In the combined case where the smaller body regularly transitsAstronomical transit
The term transit or astronomical transit has three meanings in astronomy:* A transit is the astronomical event that occurs when one celestial body appears to move across the face of another celestial body, hiding a small part of it, as seen by an observer at some particular vantage point...
the larger object, an occultation is also termed a secondary eclipse.
An eclipse occurs when a body disappears or partially disappears from view, either by an occultation, as with a solar eclipse
Solar eclipse
As seen from the Earth, a solar eclipse occurs when the Moon passes between the Sun and the Earth, and the Moon fully or partially blocks the Sun as viewed from a location on Earth. This can happen only during a new moon, when the Sun and the Moon are in conjunction as seen from Earth. At least...
, or by passing into the shadow of another body, as with a lunar eclipse
Lunar eclipse
A lunar eclipse occurs when the Moon passes behind the Earth so that the Earth blocks the Sun's rays from striking the Moon. This can occur only when the Sun, Earth, and Moon are aligned exactly, or very closely so, with the Earth in the middle. Hence, a lunar eclipse can only occur the night of a...
(thus both are listed on NASA's eclipse page).
Transits, occultations and eclipses in general are all effects of a syzygy
Syzygy (astronomy)
In astronomy, a syzygy is a straight line configuration of three celestial bodies in a gravitational system. The word is usually used in reference to the Sun, the Earth and either the Moon or a planet, where the latter is in conjunction or opposition. Solar and lunar eclipses occur at times of...
.
Transits and occultations of the sun by Earth's moon are called solar eclipse
Solar eclipse
As seen from the Earth, a solar eclipse occurs when the Moon passes between the Sun and the Earth, and the Moon fully or partially blocks the Sun as viewed from a location on Earth. This can happen only during a new moon, when the Sun and the Moon are in conjunction as seen from Earth. At least...
s regardless of whether the sun is completely or partially covered. By extension, transits of the sun by a satellite
Satellite
In the context of spaceflight, a satellite is an object which has been placed into orbit by human endeavour. Such objects are sometimes called artificial satellites to distinguish them from natural satellites such as the Moon....
of a planet may also be called eclipses, as with the transits of Phobos and Deimos shown here, as may the passage of a satellite into the planet's shadow, as with this eclipse of Phobos. The term eclipse is also used more generally for bodies passing in front of one another. For example, this entry from NASA's Astronomy Picture of the Day refers to the Moon eclipsing and occulting Saturn interchangeably.
Occultations by the Moon
The term occultation is most frequently used to describe those relatively frequent occasions when the MoonMoon
The Moon is Earth's only known natural satellite,There are a number of near-Earth asteroids including 3753 Cruithne that are co-orbital with Earth: their orbits bring them close to Earth for periods of time but then alter in the long term . These are quasi-satellites and not true moons. For more...
passes in front of a star
Star
A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...
during the course of its orbital motion around the Earth. Since the Moon, with an angular speed with respect to the stars of 0.55 arcsec/s or 2.7 µrad/s, has no atmosphere and stars have an angular diameter of at most 0.057 arcseconds or 0.28 µrad, a star that is occulted by the moon will disappear or reappear in 0.1 seconds or less on the moon's edge, or limb. Events that take place on the Moon's dark limb are of particular interest to observers, because the lack of glare allows these occultations to more easily be observed and timed.
The Moon's orbit is inclined to the ecliptic
Ecliptic
The ecliptic is the plane of the earth's orbit around the sun. In more accurate terms, it is the intersection of the celestial sphere with the ecliptic plane, which is the geometric plane containing the mean orbit of the Earth around the Sun...
(see orbit of the Moon), and any stars with an ecliptic latitude of less than about 6.5 degrees may be occulted by it. There are three first magnitude stars that are sufficiently close to the ecliptic that they may be occulted by the Moon and by planets – Regulus
Regulus
Regulus is the brightest star in the constellation Leo and one of the brightest stars in the night sky, lying approximately 77.5 light years from Earth. Regulus is a multiple star system composed of four stars which are organized into two pairs...
, Spica
Spica
Spica is the brightest star in the constellation Virgo, and the 15th brightest star in the nighttime sky. It is 260 light years distant from Earth...
and Antares
Antares
Antares is a red supergiant star in the Milky Way galaxy and the sixteenth brightest star in the nighttime sky . Along with Aldebaran, Spica, and Regulus it is one of the four brightest stars near the ecliptic...
. Occultations of Aldebaran
Aldebaran
Aldebaran is a red giant star located about 65 light years away in the zodiac constellation of Taurus. With an average apparent magnitude of 0.87 it is the brightest star in the constellation and is one of the brightest stars in the nighttime sky...
are presently only possible by the Moon, because the planets pass Aldebaran to the north. Neither planetary nor lunar occultations of Pollux
Pollux (star)
Pollux is an orange giant star approximately 34 light-years from the Earth in the constellation of Gemini . Pollux is the brightest star in the constellation, brighter than Castor...
are currently possible. However, in the far future, occultations of Aldebaran and Pollux will be possible, as they were in the far past. Some deep-sky objects, such as the Pleiades
Pleiades (star cluster)
In astronomy, the Pleiades, or Seven Sisters , is an open star cluster containing middle-aged hot B-type stars located in the constellation of Taurus. It is among the nearest star clusters to Earth and is the cluster most obvious to the naked eye in the night sky...
, can also be occulted by the moon.
Within a few kilometres of the edge of an occultation's predicted path, referred to as its northern or southern limit, an observer may see the star intermittently disappearing and reappearing as the irregular limb of the Moon moves past the star, creating what is known as a Grazing lunar occultation
Grazing lunar occultation
A lunar occultation occurs when the Moon, moving along its orbital path, passes in front of a star or other celestial object, as seen by an observer...
. From an observational and scientific standpoint, these "grazes" are the most dynamic and interesting of lunar occultations.
The accurate timing of lunar occultations is performed regularly by (primarily amateur) astronomers. Lunar occultations timed to an accuracy of a few tenths of a second have various scientific uses, particularly in refining our knowledge of lunar topography. Photoelectric analysis of lunar occultations have also discovered some stars to be very close visual or spectroscopic binaries
Binary star
A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star, comes, or secondary...
. Some angular diameters of stars have been measured by timing of lunar occultations, which is useful for determining effective temperature
Effective temperature
The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation...
s of those stars. Early radio astronomers found occultations of radio sources by the Moon valuable for determining their exact positions, because the long wavelength of radio waves limited the resolution available through direct observation. This was crucial for the unambiguous identification of the radio source 3C 273 with the optical quasar and its jet, and a fundamental prerequisite for Maarten Schmidt
Maarten Schmidt
Maarten Schmidt is a Dutch astronomer who measured the distances of quasars.Born in Groningen, The Netherlands, Schmidt studied with Jan Hendrik Oort. He earned his Ph.D. degree from Leiden Observatory in 1956....
's discovery of the cosmological nature of quasars.
Several times during the year, someone on Earth can usually observe the Moon occulting a planet. Since planets, unlike stars, have significant angular sizes, lunar occultations of planets will create a narrow zone on earth from which a partial occultation of the planet will occur. An observer located within that narrow zone could observe the planet's disk partly blocked by the slowly moving moon.
Occultation by planets
Stars may also be occulted by planets. In 1959, VenusVenus
Venus is the second planet from the Sun, orbiting it every 224.7 Earth days. The planet is named after Venus, the Roman goddess of love and beauty. After the Moon, it is the brightest natural object in the night sky, reaching an apparent magnitude of −4.6, bright enough to cast shadows...
occulted Regulus
Regulus
Regulus is the brightest star in the constellation Leo and one of the brightest stars in the night sky, lying approximately 77.5 light years from Earth. Regulus is a multiple star system composed of four stars which are organized into two pairs...
. Uranus
Uranus
Uranus is the seventh planet from the Sun. It has the third-largest planetary radius and fourth-largest planetary mass in the Solar System. It is named after the ancient Greek deity of the sky Uranus , the father of Cronus and grandfather of Zeus...
' rings were first discovered when that planet occulted a star in 1977. On the evening of July 2-July 3, 1989, Saturn
Saturn
Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn is named after the Roman god Saturn, equated to the Greek Cronus , the Babylonian Ninurta and the Hindu Shani. Saturn's astronomical symbol represents the Roman god's sickle.Saturn,...
passed in front of the 5th magnitude star 28 Sagittarii
Sagittarius (constellation)
Sagittarius is a constellation of the zodiac, the one containing the galactic center. Its name is Latin for the archer, and its symbol is , a stylized arrow. Sagittarius is commonly represented as a centaur drawing a bow...
. Pluto, which was re-designated as a dwarf planet in 2006, occulted stars in 1988, 2002, and 2006, allowing its tenuous atmosphere to be studied.
It is also possible for one planet to occult another planet. However, these mutual occultations of planets are extremely rare. The last such event occurred on January 3, 1818 and will next occur on November 22, 2065, in both cases involving the same two planets—Venus and Jupiter. Technically speaking, when the foreground planet is smaller in apparent size than the background planet, the event should be called a "mutual planetary transit." When the foreground planet is larger in apparent size than the background planet, the event should be called a "mutual planetary occultation." (See Transit
Astronomical transit
The term transit or astronomical transit has three meanings in astronomy:* A transit is the astronomical event that occurs when one celestial body appears to move across the face of another celestial body, hiding a small part of it, as seen by an observer at some particular vantage point...
for a list of past and future events).
Twice during the orbital cycles of Jupiter and Saturn, the equatorial (and satellite) planes of those planets are aligned with earth's orbital plane, resulting in a series of mutual occultations and eclipses between the moons of these giant planets. These orbital alignments have also occurred artificially when unmanned spacecraft have traversed these planetary systems, resulting in photographs such as the one shown here. The terms "eclipse," "occultation" and "transit" are also used to describe these events. A satellite of Jupiter (for example) may be eclipsed (i.e. made dimmer because it moves into Jupiter's shadow), occulted (i.e. hidden from view because Jupiter lies on our line of sight), or may transit (i.e. pass in front of) Jupiter's disk.
Occultations by asteroids
An asteroid occultation occurs when an asteroidAsteroid
Asteroids are a class of small Solar System bodies in orbit around the Sun. They have also been called planetoids, especially the larger ones...
(also known as a minor planet
Minor planet
An asteroid group or minor-planet group is a population of minor planets that have a share broadly similar orbits. Members are generally unrelated to each other, unlike in an asteroid family, which often results from the break-up of a single asteroid...
) passes in front of a star
Star
A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...
(occults a star), temporarily blocking its light (as seen from Earth
Earth
Earth is the third planet from the Sun, and the densest and fifth-largest of the eight planets in the Solar System. It is also the largest of the Solar System's four terrestrial planets...
). Several events occur nearly every day over the world. From any particular place such events occur almost every night, although most require a telescope
Telescope
A telescope is an instrument that aids in the observation of remote objects by collecting electromagnetic radiation . The first known practical telescopes were invented in the Netherlands at the beginning of the 1600s , using glass lenses...
to see.
Asteroid occultations are useful for measuring the size and position of asteroids much more precisely than can be done by any other means. A cross-sectional profile of the shape of an asteroid can even be determined if a number of observers at different, nearby, locations observe the occultation. For example, on March 12, 2009 there were 8 minor planet occulations, including (85) Io, (247) Eukrate, (1585) Union, (201) Penelope, (70) Panopaea, (980) Anacostia, (2448) Sholokhov, (1746) Brouwer, and (191) Kolga. Any one of these would be expected to occult at a time and place on the globe, at a certain magnitude, and with a certain star.
For example, according to the 1998 European Asteroidal Occultation Results from Euraster, 39 Laetitia was observed by over 38 observatories in one occultation on March 3, 1998, which resulted in many chords being determined.
Occultations have produced outlines of many asteroids. Some notable ones include:
Name | Chords | Measured Profile (km) |
---|---|---|
704 Interamnia 704 Interamnia 704 Interamnia is a very large asteroid, with an estimated diameter of 350 kilometres. Its mean distance from the Sun is 3.067 . It was discovered on October 2, 1910 by Vincenzo Cerulli, and named after the Latin name for Teramo, Italy, where Cerulli worked... |
35 | 350×304 |
39 Laetitia 39 Laetitia 39 Laetitia is a large, bright main-belt asteroid.Laetitia was discovered by J. Chacornac on February 8, 1856, and named after Laetitia, a minor Roman goddess of gaiety.... |
~16 | 219×142 |
94 Aurora 94 Aurora 94 Aurora is one of the largest main-belt asteroids. With an albedo of only 0.04, it is darker than soot, and has a primitive compositions consisting of carbonaecous material. It was discovered by J. C... |
9 | 225×173 |
375 Ursula 375 Ursula 375 Ursula is one of the largest asteroids from the asteroid belt. It was discovered by Auguste Charlois on September 18, 1893, in Nice.Observations of an occultation on November 15, 1984, produced six chords indicating an estimated diameter of 216±10 km.-External links:* from JPL /... |
6 | 216±10 |
444 Gyptis 444 Gyptis 444 Gyptis is a very large main-belt asteroid. It is classified as a C-type asteroid and is probably composed of carbonaceous material.It was discovered by J... |
6 | 179×150 |
48 Doris 48 Doris 48 Doris is one of the largest main belt asteroids. It was discovered by Hermann Goldschmidt on September 19, 1857 from his balcony in Paris.-Name:... |
4 | 278×142 |
Occultations have also been used to estimate the diameter of trans-Neptunian object
Trans-Neptunian object
A trans-Neptunian object is any minor planet in the Solar System that orbits the Sun at a greater distance on average than Neptune.The first trans-Neptunian object to be discovered was Pluto in 1930...
s such as (55636) 2002 TX300
(55636) 2002 TX300
is a bright Kuiper belt object in the outer Solar System estimated to be about 286 km in diameter. It is a large member of the Haumea family, discovered on October 15, 2002, by the Near-Earth Asteroid Tracking program....
, 28978 Ixion
28978 Ixion
28978 Ixion is a Kuiper belt object discovered on May 22, 2001. Ixion is a plutino and a very likely dwarf planet; its diameter of 650 km estimated by Spitzer makes it about the fifth largest plutino. It is named after Ixion, a figure from Greek mythology...
, and 20000 Varuna
20000 Varuna
20000 Varuna is a large classical Kuiper belt object and a probable dwarf planet. It previously had the provisional designation ' and has been precovered in plates dating back to 1953.-Name:Varuna is named after the Hindu deity,...
. Preliminary results of a 6 November 2010 occultation by the dwarf planet Eris
Eris (dwarf planet)
Eris, formal designation 136199 Eris, is the most massive known dwarf planet in the Solar System and the ninth most massive body known to orbit the Sun directly...
of a magnitude
Apparent magnitude
The apparent magnitude of a celestial body is a measure of its brightness as seen by an observer on Earth, adjusted to the value it would have in the absence of the atmosphere...
17 star in the constellation
Constellation
In modern astronomy, a constellation is an internationally defined area of the celestial sphere. These areas are grouped around asterisms, patterns formed by prominent stars within apparent proximity to one another on Earth's night sky....
of Cetus
Cetus
Cetus is a constellation. Its name refers to Cetus, a sea monster in Greek mythology, although it is often called 'the whale' today. Cetus is located in the region of the sky that contains other water-related constellations such as Aquarius, Pisces, and Eridanus.-Ecliptic:Although Cetus is not...
placed an upper limit on Eris's diameter of 2320 km, making it almost the same size as Pluto. Due to their slower movement through the night sky, occultations by TNOs are far less common than by asteroids in the main-belt.
Double occultations
It is possible that the moon or another celestial body can occult multiple celestial bodies at the same time. Such events are extremely rare and can be seen only from a small part of the world. The last event of such type was on April 23, 1998 when the moon occulted Venus and Jupiter simultaneously for observers on Ascension IslandAscension Island
Ascension Island is an isolated volcanic island in the equatorial waters of the South Atlantic Ocean, around from the coast of Africa and from the coast of South America, which is roughly midway between the horn of South America and Africa...
.
Occulting satellites
The Big Occulting Steerable Satellite (BOSS) was a proposed satelliteSatellite
In the context of spaceflight, a satellite is an object which has been placed into orbit by human endeavour. Such objects are sometimes called artificial satellites to distinguish them from natural satellites such as the Moon....
that would work in conjunction with a telescope
Telescope
A telescope is an instrument that aids in the observation of remote objects by collecting electromagnetic radiation . The first known practical telescopes were invented in the Netherlands at the beginning of the 1600s , using glass lenses...
to detect planet
Planet
A planet is a celestial body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.The term planet is ancient, with ties to history, science,...
s around distant stars. The satellite consists of a large, very lightweight sheet, and a set of maneuvering thrusters and navigation systems. It would maneuver to a position along the line of sight between the telescope and a nearby star. The satellite would thereby block the radiation from the star, permitting the orbiting planets to be observed.
The proposed satellite would have a dimension of 70 m × 70 m, a mass of about 600 kg, and maneuver by means of an ion drive engine in combination with using the sheet as a light sail. Positioned at a distance of 100,000 km from the telescope, it would block more than 99.998% of the starlight.
There are two possible configurations of this satellite. The first would work with a space telescope, most likely positioned near the Earth
Earth
Earth is the third planet from the Sun, and the densest and fifth-largest of the eight planets in the Solar System. It is also the largest of the Solar System's four terrestrial planets...
's Lagrangian point
Lagrangian point
The Lagrangian points are the five positions in an orbital configuration where a small object affected only by gravity can theoretically be stationary relative to two larger objects...
. The second would place the satellite in a highly elliptical orbit about the Earth, and work in conjunction with a ground telescope. At the apogee of the orbit, the satellite would remain relatively stationary with respect to the ground, allowing longer exposure times.
An updated version of this design is called the Starshade, which uses a sunflower
Sunflower
Sunflower is an annual plant native to the Americas. It possesses a large inflorescence . The sunflower got its name from its huge, fiery blooms, whose shape and image is often used to depict the sun. The sunflower has a rough, hairy stem, broad, coarsely toothed, rough leaves and circular heads...
-shaped coronagraph
Coronagraph
A coronagraph is a telescopic attachment designed to block out the direct light from a star so that nearby objects – which otherwise would be hidden in the star's bright glare – can be resolved...
disc. A comparable proposal was also made for a satellite to occult bright X-ray sources, called an X-ray Occulting Steerable Satellite or XOSS.
Occultations and transits by planets between 1800 and 2100
This table lists occultations and transits of bright stars and planets by solar planets.Day | Time (UT) | Foreground planet | Background object | Elongation |
---|---|---|---|---|
9 December 1802 | 07:36 | Mercury Mercury (planet) Mercury is the innermost and smallest planet in the Solar System, orbiting the Sun once every 87.969 Earth days. The orbit of Mercury has the highest eccentricity of all the Solar System planets, and it has the smallest axial tilt. It completes three rotations about its axis for every two orbits... |
Acrab | 16,2° West |
9 December 1808 | 20:34 | Mercury | Saturn Saturn Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn is named after the Roman god Saturn, equated to the Greek Cronus , the Babylonian Ninurta and the Hindu Shani. Saturn's astronomical symbol represents the Roman god's sickle.Saturn,... |
20,3° West |
22 December 1810 | 06:32 | Venus Venus Venus is the second planet from the Sun, orbiting it every 224.7 Earth days. The planet is named after Venus, the Roman goddess of love and beauty. After the Moon, it is the brightest natural object in the night sky, reaching an apparent magnitude of −4.6, bright enough to cast shadows... |
Xi-2 Sagittarii Xi-2 Sagittarii Xi-2 Sagittarii is a spectral type G8 or K0 giant which has an apparent magnitude of +3.52. It is 372 light years from Earth.... |
11,1° East |
3 January 1818 | 21:52 | Venus | Jupiter Jupiter Jupiter is the fifth planet from the Sun and the largest planet within the Solar System. It is a gas giant with mass one-thousandth that of the Sun but is two and a half times the mass of all the other planets in our Solar System combined. Jupiter is classified as a gas giant along with Saturn,... |
16,5° West |
11 July 1825 | 09:10 | Venus | Delta-1 Tauri | 44,4° West |
11 July 1837 | 12:50 | Mercury | Eta Geminorum Eta Geminorum Eta Geminorum is a triple star system in the constellation Gemini. It has the traditional names Tejat Prior, Propus and Praepes and Pish Pai .... |
17,8° West |
9 May 1841 | 19:35 | Venus | 17 Tauri | 9,2° East |
27 September 1843 | 18:00 | Venus | Eta Virginis Eta Virginis Eta Virginis is a star in the constellation Virgo. It has the traditional name Zaniah .Zaniah is about 204 light years distant from the Sun, and has apparent magnitude +3.9 and is of spectral type A2IV.... |
3,2° West |
16 December 1850 | 11:28 | Mercury | Lambda Sagittarii Lambda Sagittarii Lambda Sagittarii is a star within the constellation Sagittarius. The star marks the top of the Archer's bow, whence its traditional name Kaus Borealis. It also marks the top of the lid of the so-called "Teapot" asterism... |
10,2° East |
22 May 1855 | 05:04 | Venus | Epsilon Geminorum Epsilon Geminorum Epsilon Geminorum is a star in the constellation of Gemini. It has the traditional name Mebsuta .... |
37,4° East |
30 June 1857 | 00:25 | Saturn Saturn Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn is named after the Roman god Saturn, equated to the Greek Cronus , the Babylonian Ninurta and the Hindu Shani. Saturn's astronomical symbol represents the Roman god's sickle.Saturn,... |
Delta Geminorum Delta Geminorum Delta Geminorum is a star in the constellation Gemini. It has the traditional name Wasat. The traditional name comes from the Arabic word for "middle".... |
8,4° East |
5 December 1865 | 14:20 | Mercury | Lambda Sagittarii | 21,0° East |
28 February 1876 | 05:13 | Jupiter Jupiter Jupiter is the fifth planet from the Sun and the largest planet within the Solar System. It is a gas giant with mass one-thousandth that of the Sun but is two and a half times the mass of all the other planets in our Solar System combined. Jupiter is classified as a gas giant along with Saturn,... |
Acrab | 97,6° West |
7 June 1881 | 20:54 | Mercury | Epsilon Geminorum | 21,2° East |
9 December 1906 | 17:40 | Venus | Acrab | 14,9° West |
27 July 1910 | 02:53 | Venus | Eta Geminorum | 31,0° West |
24 December 1937 | 18:38 | Mercury | Omicron Sagittarii | 11,6° East |
10 June 1940 | 02:21 | Mercury | Epsilon Geminorum | 20,1° East |
25 October 1947 | 01:45 | Venus | Zuben-el-genubi (Alpha-2 Librae) Alpha Librae Alpha Librae is the second brightest star in the constellation Libra . It has the traditional name Zubenelgenubi. The name, from Arabic الزبن الجنوبي , means "southern claw" and was coined before Libra was recognized as distinct from Scorpius... |
13,5° East |
7 July 1959 | 14:30 | Venus | Regulus Regulus Regulus is the brightest star in the constellation Leo and one of the brightest stars in the night sky, lying approximately 77.5 light years from Earth. Regulus is a multiple star system composed of four stars which are organized into two pairs... |
44,5° East |
27 September 1965 | 15:30 | Mercury | Eta Virginis Eta Virginis Eta Virginis is a star in the constellation Virgo. It has the traditional name Zaniah .Zaniah is about 204 light years distant from the Sun, and has apparent magnitude +3.9 and is of spectral type A2IV.... |
2.6° West |
13 May 1971 | 20:00 | Jupiter | Beta Scorpii (both components) | 169,5° West |
8 April 1976 | 01:00 | Mars Mars Mars is the fourth planet from the Sun in the Solar System. The planet is named after the Roman god of war, Mars. It is often described as the "Red Planet", as the iron oxide prevalent on its surface gives it a reddish appearance... |
Epsilon Geminorum | 81,3° East |
17 November 1981 | 15:27 | Venus | Nunki | 47,0° East |
19 November 1984 | 01:32 | Venus | Lambda Sagittarii | 39,2° East |
4 December 2015 | 16.14 | Mercury | Theta Ophiuchi | 9,6° East |
17 February 2035 | 15:19 | Venus | Pi Sagittarii Pi Sagittarii Pi Sagittarii is a triple star system in the constellation Sagittarius. It has the traditional name Albaldah. It is known as 建三 in Chinese.... |
42,1° West |
1 October 2044 | 22:00 | Venus | Regulus | 38,9° West |
23 February 2046 | 19:24 | Venus | Rho-1 Sagittarii | 45,4° West |
10 November 2052 | 07:20 | Mercury | Zuben-el-genubi (Alpha-2 Librae) Alpha Librae Alpha Librae is the second brightest star in the constellation Libra . It has the traditional name Zubenelgenubi. The name, from Arabic الزبن الجنوبي , means "southern claw" and was coined before Libra was recognized as distinct from Scorpius... |
2,8° West |
22 November 2065 | 12:45 | Venus | Jupiter | 7,9° West |
15 July 2067 | 11:56 | Mercury | Neptune Neptune Neptune is the eighth and farthest planet from the Sun in the Solar System. Named for the Roman god of the sea, it is the fourth-largest planet by diameter and the third largest by mass. Neptune is 17 times the mass of Earth and is slightly more massive than its near-twin Uranus, which is 15 times... |
18,4° West |
11 August 2069 | 20.25 | Venus | Zavijava | 38,4° East |
3 October 2078 | 22:00 | Mars | Theta Ophiuchi | 71,4° East |
11 August 2079 | 01:30 | Mercury | Mars Mars Mars is the fourth planet from the Sun in the Solar System. The planet is named after the Roman god of war, Mars. It is often described as the "Red Planet", as the iron oxide prevalent on its surface gives it a reddish appearance... |
11,3° West |
27 October 2088 | 13:43 | Mercury | Jupiter | 4,7° West |
7 April 2094 | 10:48 | Mercury | Jupiter | 1,8° West |
These events are not visible everywhere the occulting body and the occulted body are above the skyline. Some events are barely visible, because they take place in close proximity to the Sun.
Mutual planetary transits and occultations
In rare cases, one planet can transit in front of another. The next time this will happen (as seen from Earth) will be on November 22, 2065 at about 12:43 UTCCoordinated Universal Time
Coordinated Universal Time is the primary time standard by which the world regulates clocks and time. It is one of several closely related successors to Greenwich Mean Time. Computer servers, online services and other entities that rely on having a universally accepted time use UTC for that purpose...
, when Venus near superior conjunction (with an angular diameter
Angular diameter
The angular diameter or apparent size of an object as seen from a given position is the “visual diameter” of the object measured as an angle. In the vision sciences it is called the visual angle. The visual diameter is the diameter of the perspective projection of the object on a plane through its...
of 10.6") will transit in front of Jupiter
Jupiter
Jupiter is the fifth planet from the Sun and the largest planet within the Solar System. It is a gas giant with mass one-thousandth that of the Sun but is two and a half times the mass of all the other planets in our Solar System combined. Jupiter is classified as a gas giant along with Saturn,...
(with an angular diameter of 30.9"); however, this will take place only 8° west of the Sun, and will therefore not be visible to the unaided/unprotected eye. When the nearer object has a larger angular diameter
Angular diameter
The angular diameter or apparent size of an object as seen from a given position is the “visual diameter” of the object measured as an angle. In the vision sciences it is called the visual angle. The visual diameter is the diameter of the perspective projection of the object on a plane through its...
than the farther object, thus covering it completely, the event is not a transit but an occultation. Before transiting Jupiter, Venus will occult Jupiter's moon
Natural satellite
A natural satellite or moon is a celestial body that orbits a planet or smaller body, which is called its primary. The two terms are used synonymously for non-artificial satellites of planets, of dwarf planets, and of minor planets....
Ganymede
Ganymede (moon)
Ganymede is a satellite of Jupiter and the largest moon in the Solar System. It is the seventh moon and third Galilean satellite outward from Jupiter. Completing an orbit in roughly seven days, Ganymede participates in a 1:2:4 orbital resonance with the moons Europa and Io, respectively...
at around 11:24 UTC as seen from some southernmost parts of Earth. Parallax
Parallax
Parallax is a displacement or difference in the apparent position of an object viewed along two different lines of sight, and is measured by the angle or semi-angle of inclination between those two lines. The term is derived from the Greek παράλλαξις , meaning "alteration"...
will cause actual observed times to vary by a few minutes, depending on the precise location of the observer.
There are only 18 mutual planetary transits and occultations as seen from Earth between 1700 and 2200. Note the long break of events between 1818 and 2065.
- 19 September 1702 – Jupiter occults Neptune
- 20 July 1705 – Mercury transits Jupiter
- 14 July 1708 – Mercury occults Uranus
- 4 October 1708 – Mercury transits Jupiter
- 28 May 1737 – Venus occults Mercury
- 29 August 1771 – Venus transits Saturn
- 21 July 1793 – Mercury occults Uranus
- 9 December 1808 – Mercury transits Saturn
- 3 January 1818 – Venus transits Jupiter
- 22 November 2065 – Venus transits Jupiter
- 15 July 2067 – Mercury occults Neptune
- 11 August 2079 – Mercury occults Mars
- 27 October 2088 – Mercury transits Jupiter
- 7 April 2094 – Mercury transits Jupiter
- 21 August 2104 – Venus occults Neptune
- 14 September 2123 – Venus transits Jupiter
- 29 July 2126 – Mercury occults Mars
- 3 December 2133 – Venus occults Mercury
The 1737 event was observed by John Bevis
John Bevis
John Bevis was an English doctor and astronomer. He is best known for discovering the Crab Nebula in 1731....
at Greenwich Observatory – it is the only detailed account of a mutual planetary occultation. A transit of Mars across Jupiter on 12 Sep 1170 was observed by the monk Gervase at Canterbury
Canterbury
Canterbury is a historic English cathedral city, which lies at the heart of the City of Canterbury, a district of Kent in South East England. It lies on the River Stour....
, and by Chinese astronomers. In addition, an occultation of Mars by Venus was observed by M. Möstlin
Michael Maestlin
Michael Maestlin was a German astronomer and mathematician, known for being the mentor of Johannes Kepler.-Career:...
at Heidelberg
Heidelberg
-Early history:Between 600,000 and 200,000 years ago, "Heidelberg Man" died at nearby Mauer. His jaw bone was discovered in 1907; with scientific dating, his remains were determined to be the earliest evidence of human life in Europe. In the 5th century BC, a Celtic fortress of refuge and place of...
on October 3, 1590.
Occultation in religion
In Shia Islam the OccultationThe Occultation
The Occultation in Shia Islam refers to a belief that the messianic figure, or Mahdi, who in Shi'i thought is an infallible male descendant of the founder of Islam, Muhammad, was born but disappeared, and will one day return and fill the world with justice. Some Shi'is, such as the Zaidi and...
is a term used to designate the hidden state of the Imam of the Time
Imamah (Shi'a doctrine)
Imāmah is the Shia doctrine of religious, spiritual and political leadership of the Ummah. The Shīa believe that the A'immah are the true Caliphs or rightful successors of Muḥammad, and further that Imams are possessed of divine knowledge and authority as well as being part of the Ahl al-Bayt,...
.
See also
- TransitAstronomical transitThe term transit or astronomical transit has three meanings in astronomy:* A transit is the astronomical event that occurs when one celestial body appears to move across the face of another celestial body, hiding a small part of it, as seen by an observer at some particular vantage point...
(also for occultations of planets by other planets) - List of minor planets
- List of Solar System objects by size
- Transit of MercuryTransit of MercuryA transit of Mercury across the Sun takes place when the planet Mercury comes between the Sun and the Earth, and Mercury is seen as a small black dot moving across the face of the Sun....
- Transit of VenusTransit of VenusA transit of Venus across the Sun takes place when the planet Venus passes directly between the Sun and Earth, becoming visible against the solar disk. During a transit, Venus can be seen from Earth as a small black disk moving across the face of the Sun...
- Solar eclipseSolar eclipseAs seen from the Earth, a solar eclipse occurs when the Moon passes between the Sun and the Earth, and the Moon fully or partially blocks the Sun as viewed from a location on Earth. This can happen only during a new moon, when the Sun and the Moon are in conjunction as seen from Earth. At least...
- Grazing lunar occultationGrazing lunar occultationA lunar occultation occurs when the Moon, moving along its orbital path, passes in front of a star or other celestial object, as seen by an observer...
- Grazing occultationGrazing occultationAn occultation is an astronomical event that occurs when one celestial object is hidden by another celestial object that passes between it and the observer. A grazing occultation is a special type of lunar occultation that occurs within a mile or two of the edge of an occultation's predicted path,...
- Syzygy (astronomy)Syzygy (astronomy)In astronomy, a syzygy is a straight line configuration of three celestial bodies in a gravitational system. The word is usually used in reference to the Sun, the Earth and either the Moon or a planet, where the latter is in conjunction or opposition. Solar and lunar eclipses occur at times of...
- Radio occultationRadio occultationRadio occultation is a remote sensing technique used for measuring the physical properties of a planetary atmosphere. It relies on the detection of a change in a radio signal as it passes through the planet's atmosphere i.e. as it is occulted by the atmosphere. When electromagnetic radiation...
- TAOS: The Taiwanese-American Occultation SurveyTAOS: The Taiwanese-American Occultation SurveyTAOS: The Taiwanese–American Occultation Survey is a robotic survey of the Outer Solar System. TAOS uses an array of four 50 cm aperture telescopes to monitor background stars awaiting the alignment of an Outer Solar System with a star target: an occultation...
External links
- Occultation Studies at Williams College
- International Occultation Timing Association (IOTA)
- Occultations of planets by other planets
- Big Occulting Steerable Satellite
- Moon, planets, asteroid occultations
- Mutual occultations (and conjunctions) of planets
- Society for Popular Astronomy – Occultation Section
- SPACE.com: Discovery Hints at a Quadrillion Space Rocks Beyond Neptune (Sara Goudarzi) 15 August 2006 06:13 am ET
- Scientists Use Novel Technique To Watch Occultations By Planets
- Mutual Planetary Transits – Fifteen millennium catalog: 5 000 BC – 10 000 AD
- asteroidoccultation.com/ Asteroid Occultation Updates
- Occultations by asteroids (Good visual aid of an occultation of a star by Phoebe)
- Society for Popular Astronomy (Asteroidal Occultations for the UK)
- Occultations of HIP and UCAC2 stars downto 15m by large TNO in 2004–2014
- Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes (arXiv : 21 Apr 2011)
- Lunar Occultation Workbench, a free software package for computing lunar occultations
External references
- Meeus, Jean: Astronomical Tables of the Sun, Moon and Planets. Richmond, Virginia: Willmann-Bell, Inc., 1995, ISBN 0-943396-45-X.
- Marco Peuschel http://www.marco-peuschel.de, Astronomische Tabellen für den Mond von 2007 bis 2016,Mondphasen, Apsiden, Knotendurchgänge, Maximale und minimale Deklinationswerte und Sternbedeckungen sowie ausführliche Ephemeriden für jeden Tag des Jahres, inkl. Mondauf-und Untergänge und physische Daten.