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PLANETARY MIGRATION

  • Planetary migration
  • Astronomical phenomenon

    Planetary migration occurs when a planet or other body in orbit around a star interacts with a disk of gas or planetesimals, resulting in the alteration

    Planetary migration

    Planetary migration

    Planetary_migration

  • Grand tack hypothesis
  • Theory of early changes in Jupiter's orbit

    halting near its current orbit at 5.2 AU. The reversal of Jupiter's planetary migration is likened to the path of a sailboat changing directions (tacking)

    Grand tack hypothesis

    Grand tack hypothesis

    Grand_tack_hypothesis

  • Planetary system
  • Set of non-stellar objects in orbit around a star

    A planetary system consists of a set of non-stellar bodies which are gravitationally bound to and in orbit of a star or star system. Generally speaking

    Planetary system

    Planetary system

    Planetary_system

  • Fifth Giant
  • Hypothetical Fifth Giant Planet

    System due to gravitational interactions during the chaotic phase of planetary migration, approximately 4 billion years ago. The Nice model, developed in

    Fifth Giant

    Fifth_Giant

  • Migration
  • Topics referred to by the same term

    physical chemistry and materials Planetary migration, the alteration of the satellite's orbital parameters Migration (virtualization), the process by

    Migration

    Migration

  • Gravitational capture
  • Entrance of one object in another's orbit

    hypothesized Planet Nine in the Solar System. (Planetary migration is a competing explanation.) Planetary capture (possibly planet swapping with neighboring

    Gravitational capture

    Gravitational_capture

  • Martyn Fogg
  • giant planet migration in 2008. Fogg lives in London. Fogg's scientific work started in 1985, with work on simulating extrasolar planetary systems. Starting

    Martyn Fogg

    Martyn_Fogg

  • Formation and evolution of the Solar System
  • might have shifted due to gravitational interactions. The process of planetary migration explains parts of the Solar System's current structure. In roughly

    Formation and evolution of the Solar System

    Formation and evolution of the Solar System

    Formation_and_evolution_of_the_Solar_System

  • Nice model
  • Scenario for the dynamical evolution of the Solar System

    differs from earlier models of the Solar System's formation. This planetary migration is used in dynamical simulations of the Solar System to explain historical

    Nice model

    Nice model

    Nice_model

  • Nebular hypothesis
  • Astronomical theory about the Solar System

    the migration of planetary embryos followed by collisions and mergers, or the radial drift of small solids from farther out in the disk. The migration of

    Nebular hypothesis

    Nebular hypothesis

    Nebular_hypothesis

  • Jupiter
  • Fifth planet from the Sun

    Bitsch, B.; Mustill, A.J.; Turrini, D. (March 2019). "Consequences of planetary migration on the minor bodies of the early solar system". Astronomy & Astrophysics

    Jupiter

    Jupiter

    Jupiter

  • Orbital resonance
  • Regular and periodic mutual gravitational influence of orbiting bodies

    Simulations indicate that this system of resonances must have formed via planetary migration. Kepler-80 d, e, b, c and g have periods in a ~ 1.000: 1.512: 2.296:

    Orbital resonance

    Orbital resonance

    Orbital_resonance

  • Lists of planets
  • exoplanets. As of 2 July 2026, there are 6,316 confirmed exoplanets in 4,725 planetary systems, with 1,055 systems having more than one planet. Most of these

    Lists of planets

    Lists of planets

    Lists_of_planets

  • Formation of Jupiter
  • Formation processes of the planet Jupiter

    peculiar orbits of hot Jupiters indicate that Jupiter underwent planetary migration shortly after its formation. The planet likely formed at about 5

    Formation of Jupiter

    Formation of Jupiter

    Formation_of_Jupiter

  • Protostar
  • Early stage in the process of star formation

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Protostar

    Protostar

    Protostar

  • Neptune trojan
  • Asteroid sharing the orbit of Neptune

    trojans to be captured when the planetary migration continues. For high-inclination trojans to be captured the migration must have been slow, or their inclinations

    Neptune trojan

    Neptune trojan

    Neptune_trojan

  • Jumping-Jupiter scenario
  • Scenario of giant planet migration

    multi-resonant planetary system. As the eccentricities of the planetesimals are excited by gravitational encounters with Pluto-mass objects, an inward migration of

    Jumping-Jupiter scenario

    Jumping-Jupiter_scenario

  • Dark nebula
  • Type of interstellar cloud that obscures visible light

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Dark nebula

    Dark nebula

    Dark_nebula

  • Bok globule
  • Isolated, small, and opaque nebula

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Bok globule

    Bok globule

    Bok_globule

  • Kelvin–Helmholtz mechanism
  • Process of energy release of a contracting star or planet

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Kelvin–Helmholtz mechanism

    Kelvin–Helmholtz mechanism

    Kelvin–Helmholtz_mechanism

  • Himalia group
  • Satellites of Jupiter

    already captured and the collisional family already created while planetary migration was ongoing, and gravitational interactions between Jupiter and other

    Himalia group

    Himalia group

    Himalia_group

  • T Tauri star
  • Class of young variable stars

    called protoplanetary discs because they are probably the progenitors of planetary systems like the Solar System. Circumstellar discs are estimated to dissipate

    T Tauri star

    T Tauri star

    T_Tauri_star

  • OGLE-2005-BLG-390Lb
  • Super-Earth ice exoplanet

    been compared to Hoth. Gliese 581 c Gliese 581 g OGLE-2005-BLG-169Lb Planetary habitability List of coolest exoplanets Brennan, Pat (May 1, 2019). "Meet

    OGLE-2005-BLG-390Lb

    OGLE-2005-BLG-390Lb

    OGLE-2005-BLG-390Lb

  • Hot Jupiter
  • High-mass planet orbiting close to a star

    In the migration hypothesis, a hot Jupiter forms beyond the frost line, from rock, ice, and gases via the core accretion method of planetary formation

    Hot Jupiter

    Hot Jupiter

    Hot_Jupiter

  • Five-planet Nice model
  • Numerical model of the early Solar System

    divergent migration of the planets leads to resonance crossings, exciting the eccentricities of the giant planets and destabilizing the planetary system

    Five-planet Nice model

    Five-planet_Nice_model

  • Jupiter trojan
  • Asteroid sharing the orbit of Jupiter

    Bitsch, B.; Mustill, A. J.; Turrini, D. (2019). "Consequences of planetary migration on the minor bodies of the early solar system". Astronomy & Astrophysics

    Jupiter trojan

    Jupiter trojan

    Jupiter_trojan

  • Homestead
  • Topics referred to by the same term

    (1920s), an American record company of the 1920s Homestead, fictional planetary migration company, Passengers Homestead (film), a 2024 American post-apocalyptic

    Homestead

    Homestead

  • Uranus
  • Seventh planet from the Sun

    nebular gas, never reached that critical point. Recent simulations of planetary migration have suggested that both ice giants formed closer to the Sun than

    Uranus

    Uranus

    Uranus

  • CFHTWIR-Oph 98 b
  • Substellar object in a binary system

    scenario is known, it may explain the formation of Planet Nine. Planetary migration may explain its formation, or it may be a brown dwarf.[citation needed]

    CFHTWIR-Oph 98 b

    CFHTWIR-Oph 98 b

    CFHTWIR-Oph_98_b

  • Young stellar object
  • Star in its early stage of evolution

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Young stellar object

    Young stellar object

    Young_stellar_object

  • GJ 1214 b
  • Sub-Neptune orbiting GJ 1214

    hydrogen and helium (c. 0.05%). Water planets could result from inward planetary migration and originate as protoplanets that formed from volatile ice-rich

    GJ 1214 b

    GJ 1214 b

    GJ_1214_b

  • List of largest exoplanets
  • List of largest planets by size

    Grootel, V. Van; Bellotti, S.; Poppenhaeger, K. (2025-01-13). "Planetary inward migration as the potential cause of GJ 504's fast rotation and bright X-ray

    List of largest exoplanets

    List of largest exoplanets

    List_of_largest_exoplanets

  • Yanqin Wu
  • Chinese-Canadian astrophysicist

    orbital resonance, and planetary migration, and the classification and distribution of exoplanets. She has theorized that planetary collisions have culled

    Yanqin Wu

    Yanqin_Wu

  • Molecular cloud
  • Type of interstellar cloud

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Molecular cloud

    Molecular cloud

    Molecular_cloud

  • Planetary core
  • Innermost layer(s) of a planet

    A planetary core consists of the innermost layers of a planet. Cores may be entirely liquid, or a mixture of solid and liquid layers as is the case in

    Planetary core

    Planetary core

    Planetary_core

  • Jeans instability
  • Star formation process

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Jeans instability

    Jeans instability

    Jeans_instability

  • Secular variation
  • Long-term non-periodic variation

    dynamics result in some effects which are unidirectional (for example, planetary migration). Secular phenomena create variations in the orbits of the Moon and

    Secular variation

    Secular_variation

  • Pre-main-sequence star
  • Star in the stage when it has not yet reached the main sequence

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Pre-main-sequence star

    Pre-main-sequence star

    Pre-main-sequence_star

  • Neptunian desert
  • Region around stars where hot Neptunes are rare

    that the Neptunian desert arises from physical phenomena such as planetary migration and subsequent evaporation by the star's intense heat. Some planets

    Neptunian desert

    Neptunian desert

    Neptunian_desert

  • TOI-700
  • Red dwarf in the constellation Dorado

    explain the arrangement of densities in this system is long-term planetary migration. Planet c might have migrated inwards, but this scenario is more

    TOI-700

    TOI-700

  • LHS 1903
  • Red dwarf star in the constellation Lynx

    depleted of gas. Alternative explanations, such as a dynamic process of planetary migration that rearranged the planets after their initial formation, or a giant

    LHS 1903

    LHS 1903

    LHS_1903

  • Herbig Ae/Be star
  • Young stars of spectral types A and B

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Herbig Ae/Be star

    Herbig Ae/Be star

    Herbig_Ae/Be_star

  • Main sequence
  • Continuous band of stars that appears on plots of stellar color versus brightness

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Main sequence

    Main sequence

    Main_sequence

  • Initial mass function
  • Empirical function in astronomy

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    Initial mass function

    Initial mass function

    Initial_mass_function

  • Timeline of Earth
  • Earth as well) by bolides and asteroids, produced possibly by the planetary migration of Neptune into the Kuiper belt as a result of orbital resonances

    Timeline of Earth

    Timeline_of_Earth

  • William Ward (astronomer)
  • American astronomer

    Technology in 1972. He became an astronomy theoretician, studying how planetary systems formed and evolved. His career began at the Harvard's Center for

    William Ward (astronomer)

    William_Ward_(astronomer)

  • Proplyd
  • Dust ring surrounding large stars thousands of solar radii wide

    tack hypothesis Late Heavy Bombardment Nice model Photoevaporation Planetary migration Wiki commons photos: Bright and dark proplyds in the Orion Nebula

    Proplyd

    Proplyd

    Proplyd

  • Disrupted planet
  • Planetary object disrupted by other body

    planet is a planet or exoplanet or, perhaps on a somewhat smaller scale, a planetary-mass object, planetesimal, moon, exomoon or asteroid that has been disrupted

    Disrupted planet

    Disrupted planet

    Disrupted_planet

  • Vulcanoid
  • Hypothetical asteroids orbiting close to the Sun

    other processes have been at work in the inner Solar System, such as planetary migration clearing out the area. 594913 ꞌAylóꞌchaxnim (the only known asteroid

    Vulcanoid

    Vulcanoid

    Vulcanoid

  • 51 Pegasi
  • Star in the constellation Pegasus

    with theories of planet formation and resulted in discussions of planetary migration. However, several hot Jupiters are now known to be oblique relative

    51 Pegasi

    51 Pegasi

    51_Pegasi

  • 55565 Aya
  • Classical Kuiper belt object

    gravitationally scattered out to its present location by Neptune's outward planetary migration in the Solar System's early history. Hence, Aya is sometimes classified

    55565 Aya

    55565 Aya

    55565_Aya

  • LHS 1140
  • Star in the constellation Cetus

    originate from stellar activity rather than a planet in 2023. MEarth Project Planetary habitability High Accuracy Radial Velocity Planet Searcher (HARPS) Super-Earth

    LHS 1140

    LHS 1140

    LHS_1140

  • Habitable zone
  • Orbits where planets may have liquid surface water

    white dwarfs may support a relatively brief habitable zone through planetary migration. At the same time, others have written in similar support of semi-stable

    Habitable zone

    Habitable zone

    Habitable_zone

  • Solar System
  • Planetary system consisting of the Sun and objects orbiting it

    planets, of which Earth is one. The Solar System is an isolated single-star planetary system (not part of a larger star system) within the Milky Way Galaxy

    Solar System

    Solar System

    Solar_System

  • FU Orionis star
  • Type of eruptive variable star

    object Theoretical concepts Accretion Initial mass function Jeans instability Kelvin–Helmholtz mechanism Nebular hypothesis Planetary migration v t e

    FU Orionis star

    FU Orionis star

    FU_Orionis_star

  • IRAS 04125+2902 b
  • Young exoplanet orbiting a protostar

    for the misalignment of the disk is unclear. It could be due to planetary migration in the past which misaligned the orbit of IRAS 04125+2902 b's orbit

    IRAS 04125+2902 b

    IRAS 04125+2902 b

    IRAS_04125+2902_b

  • Peter Goldreich
  • American astrophysicist (born 1939)

    was confirmed in 1986. Goldreich, along with Tremaine predicted planetary migration in 1980, which would later be invoked to explain hot jupiters. In

    Peter Goldreich

    Peter Goldreich

    Peter_Goldreich

  • Gliese 581
  • Star in the constellation Libra

    581 (/ˈɡliːzə/) is a red dwarf star of spectral type M3V which hosts a planetary system, 20.5 light-years (6.3 parsecs) away from Earth in the constellation

    Gliese 581

    Gliese_581

  • Triple planetary crisis
  • Three intersecting global environmental crises

    Triple planetary crisis is a term and framework adopted by the United Nations system to describe the three intersecting global environmental crises of

    Triple planetary crisis

    Triple planetary crisis

    Triple_planetary_crisis

  • Circumplanetary disk
  • Accumulation of matter around a planet

    circumstellar disk, despite not being around a star, but around a 5–6 MJup planetary-mass object. In August 2018, astronomers reported the probable detection

    Circumplanetary disk

    Circumplanetary disk

    Circumplanetary_disk

  • Tidally detached exomoon
  • Planet that was formerly a moon of another planet

    their orbits around their parent planets by tidal forces during planetary migration, and becoming planets in their own right. As of 2026, no tidally

    Tidally detached exomoon

    Tidally_detached_exomoon

  • 307261 Máni
  • Classical Kuiper belt object

    gravitationally scattered to its present location by Neptune's outward planetary migration in the Solar System's early history. Máni's present orbit is far

    307261 Máni

    307261 Máni

    307261_Máni

  • Circumstellar disc
  • Accumulation of matter around a star

    formation has taken place, and around white dwarfs, they indicate that planetary material survived the whole of stellar evolution. Such a disc can manifest

    Circumstellar disc

    Circumstellar disc

    Circumstellar_disc

  • 51 Eridani b
  • Extrasolar planet

    4.1±0.4 Jupiter masses (MJ), whereas self-consistent modelling of the planetary atmosphere and interior yields a mass of 3.13+0.05 −0.04 MJ. Astrometric

    51 Eridani b

    51 Eridani b

    51_Eridani_b

  • Gravitational scattering
  • Alteration of orbits of celestial bodies through gravity

    the planets that had gravitational encounters. Celestial mechanics Planetary migration Three-body problem Stellar dynamics Stellar kinematics  This article

    Gravitational scattering

    Gravitational scattering

    Gravitational_scattering

  • Kepler-1647b
  • Circumbinary gas giant orbiting the Kepler-1647 star system

    stars Molecular cloud Nebular hypothesis Oort cloud Outer space Planetary migration Planetary system Planetesimal Planet formation Protoplanetary disk Radial

    Kepler-1647b

    Kepler-1647b

    Kepler-1647b

  • OGLE-2016-BLG-1190Lb
  • Exosolar object orbiting OGLE-2016-BLG-1190L

    stars Molecular cloud Nebular hypothesis Oort cloud Outer space Planetary migration Planetary system Planetesimal Planet formation Protoplanetary disk Radial

    OGLE-2016-BLG-1190Lb

    OGLE-2016-BLG-1190Lb

  • K2-33b
  • Young Super-Neptune orbiting K2-33

    1995. Given the young age of this exoplanet, several theories of planetary migration can be ruled out because they take too long to form close-in planets

    K2-33b

    K2-33b

    K2-33b

  • Ruth Murray-Clay
  • North American astrophysicist

    Murray-Clay" (PDF). Murray-Clay, Ruth Ann (2008). Consequences of planetary migration: Kuiper belt dynamics and atmospheric escape from hot Jupiters (PhD)

    Ruth Murray-Clay

    Ruth Murray-Clay

    Ruth_Murray-Clay

  • TOI-421
  • Planetary system in the constellation Lepus

    evolutionary models for a planet forming this close to the star. Planetary migration is a plausible explanation, meaning that the planet could have formed

    TOI-421

    TOI-421

  • WASP-47
  • Star in the constellation Aquarius

    further out in the system or was ejected billions of years ago. Planetary migration Nice model 55 Cancri e, another large rocky planet very similar to

    WASP-47

    WASP-47

  • (55636) 2002 TX300
  • Haumea family Kuiper belt object

    gravitationally scattered out to its present location by Neptune's outward planetary migration in the Solar System's early history. Because of this, 2002 TX300

    (55636) 2002 TX300

    (55636) 2002 TX300

    (55636)_2002_TX300

  • Rossiter–McLaughlin effect
  • Spectroscopic phenomenon in astronomy

    stars, strongly suggesting that dynamical interactions rather than planetary migration produce these objects if no additional processes are involved. J

    Rossiter–McLaughlin effect

    Rossiter–McLaughlin effect

    Rossiter–McLaughlin_effect

  • Stephanie C. Werner
  • German geologist and planetologist

    the Mojave impact crater on Mars, and an estimate that an era of planetary migration in the Solar System occurred earlier than previously thought. Werner

    Stephanie C. Werner

    Stephanie_C._Werner

  • Spectro-Polarimetric High-Contrast Exoplanet Research
  • characterizing a large number of such planets should offer insight into planetary migration, the hypothetical process whereby hot Jupiters, which theory indicates

    Spectro-Polarimetric High-Contrast Exoplanet Research

    Spectro-Polarimetric High-Contrast Exoplanet Research

    Spectro-Polarimetric_High-Contrast_Exoplanet_Research

  • Planetary mass
  • Measure of the mass of a planet-like astronomical body

    In astronomy, planetary mass is a measure of the mass of a planet-like astronomical object. Within the Solar System, planets are usually measured in the

    Planetary mass

    Planetary_mass

  • List of exoplanet search projects
  • 04413. doi:10.1117/12.2233002. S2CID 119210955. "FINDS Exo-Earths". www.planetary.org. Retrieved 2016-07-08. "Planet Imager » About". planetimager.org.

    List of exoplanet search projects

    List_of_exoplanet_search_projects

  • MP Muscae
  • Pre-main-sequence star in the constellation Musca

    that the planet formed in its current orbit, but instead underwent planetary migration. Although multiple young stars with protoplanetary disks are known

    MP Muscae

    MP Muscae

    MP_Muscae

  • Rossby wave
  • Inertial wave in rotating fluids

    Rossby waves, also known as planetary waves, are a type of inertial wave naturally occurring in rotating fluids. They were first identified by Sweden-born

    Rossby wave

    Rossby_wave

  • Kepler-84
  • Star in the constellation Cygnus

    S.; Charalambous, C.; Benítez-Llambay, P.; Beaugé, C. (2017), "Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in

    Kepler-84

    Kepler-84

  • Mirko Grmek
  • Croatian-French medical historian (1924–2000)

    determine the pathocenosis of today's world, since the constant planetary migration of large masses of people from south to north, as well as the development

    Mirko Grmek

    Mirko_Grmek

  • Kepler-223
  • G5V star in the constellation Cygnus

    S2CID 205248546. Koppes, S. (17 May 2016). "Kepler-223 System: Clues to Planetary Migration". Jet Propulsion Lab. Retrieved 18 May 2016. Chown, Marcus (28 February

    Kepler-223

    Kepler-223

  • OGLE-2016-BLG-1195Lb
  • Frigid super-Earth orbiting OGLE-2016-BLG-1195L

    from the Sun, although it was expected to be much colder. In 2023, the planetary mass estimate was significantly increased to 9.91±1.61 M🜨, resulting

    OGLE-2016-BLG-1195Lb

    OGLE-2016-BLG-1195Lb

    OGLE-2016-BLG-1195Lb

  • History of Solar System formation and evolution hypotheses
  • explain these so-called hot Jupiters, but one leading idea is that of planetary migration, similar to the process which is thought to have moved Uranus and

    History of Solar System formation and evolution hypotheses

    History of Solar System formation and evolution hypotheses

    History_of_Solar_System_formation_and_evolution_hypotheses

  • E-belt asteroids
  • Hypothetical extension of the asteroid belt

    estimates of the orbital density of the main asteroid belt before the planetary migration. Bottke, William F.; Vokrouhlický, David; Minton, David; Nesvorný

    E-belt asteroids

    E-belt asteroids

    E-belt_asteroids

  • Gary Ruvkun
  • American geneticist (born 1952)

    cooled, and the recent discoveries of hot Jupiters and disruptive planetary migrations in exoplanet systems favors the spread of DNA-based microbial life

    Gary Ruvkun

    Gary Ruvkun

    Gary_Ruvkun

  • Māori migration canoes
  • Aspect of Māori oral history involving migration on legendary canoes

    his newly discovered land. Other stories of various Māori tribes report migrations to escape famine, over-population, and warfare. These were made in legendary

    Māori migration canoes

    Māori migration canoes

    Māori_migration_canoes

  • OKEANOS
  • Proposed space probe to Trojan asteroids

    building blocks of Jupiter, or captured trans-Neptunian objects by planetary migration. The latest proposal included a lander to perform in situ analyses

    OKEANOS

    OKEANOS

  • Kepler-1649c
  • Earth-size exoplanet orbiting Kepler-1649

    habitable zone of the red dwarf star Kepler-1649, the outermost planet of the planetary system discovered by Kepler’s space telescope. It is located about 301

    Kepler-1649c

    Kepler-1649c

    Kepler-1649c

  • Pluto
  • Largest dwarf planet

    the Kuiper belt. It was immediately hailed as the ninth planet, but its planetary status was questioned when it was found to be much smaller than expected

    Pluto

    Pluto

    Pluto

  • Kepler-11e
  • Extrasolar planet orbiting Kepler-11

    tend to either facilitate the creation of gas giants or to promote planetary migration, in which the planet orbits more closely to its star. However, Kepler-11

    Kepler-11e

    Kepler-11e

    Kepler-11e

  • WD 1856+534
  • White dwarf located in the constellation Draco

    formation via common envelope and instead favour high eccentricity migration. The planetary transmission spectrum obtained with GTC OSIRIS is gray and featureless

    WD 1856+534

    WD 1856+534

    WD_1856+534

  • Exozodiacal dust
  • Small particles between exoplanets

    amorphous carbon and silicate dust that fill the plane of extrasolar planetary systems. It is the exoplanetary analog of zodiacal dust, the 1–100 micrometre-sized

    Exozodiacal dust

    Exozodiacal dust

    Exozodiacal_dust

  • Planetary phase of civilization
  • Speculative concept, global human unification

    The planetary phase of civilization is a term created by the Global Scenario Group (GSG) to describe the contemporary era in which increasing global interdependence

    Planetary phase of civilization

    Planetary_phase_of_civilization

  • Exoplanet orbital and physical parameters
  • zero axial tilt even if they had been in a Cassini state during planetary migration when they were further from their star. Hot Jupiters' orbits will

    Exoplanet orbital and physical parameters

    Exoplanet_orbital_and_physical_parameters

  • Sarah Ballard
  • American astronomer

    this theoretical search procedure and the discovery of the Kepler-19 planetary system with that technique. Ballard took part in the discovery of four

    Sarah Ballard

    Sarah Ballard

    Sarah_Ballard

  • Late Heavy Bombardment
  • Hypothesized astronomical event

    exists. The Nice model, popular among planetary scientists, postulates that the giant planets underwent orbital migration, scattering objects from the asteroid

    Late Heavy Bombardment

    Late Heavy Bombardment

    Late_Heavy_Bombardment

  • Planet
  • Large, round non-stellar astronomical object

    category; Ceres, Pluto, and Eris are in the category of dwarf planet. Many planetary scientists have nonetheless continued to apply the term planet more broadly

    Planet

    Planet

    Planet

  • Ocean world
  • Planet containing a significant amount of water or other liquid

    kind of exosea). The study of extraterrestrial oceans is referred to as planetary oceanography. Earth is the only astronomical object known to presently

    Ocean world

    Ocean world

    Ocean_world

  • GU Piscium b
  • Planetary mass companion orbiting GU Piscium

    GU Piscium b (GU Psc b) is a directly imaged planetary-mass companion orbiting the star GU Piscium, with an extremely large orbit of 2,000 AU (3.0×1011 km)

    GU Piscium b

    GU Piscium b

    GU_Piscium_b

AI & ChatGPT searchs for online references containing PLANETARY MIGRATION

PLANETARY MIGRATION

AI search references containing PLANETARY MIGRATION

PLANETARY MIGRATION

  • Hijrah
  • Girl/Female

    Arabic, Muslim

    Hijrah

    Migration of the Prophet from Makkah to Madinah

    Hijrah

  • Mountcastle
  • Surname or Lastname

    Irish

    Mountcastle

    Irish : in part at least, probably a further Anglicization of the Irish surname Mountcashell, itself an Anglicized form of Gaelic Ó Maolchaisil (see Cashel 2), which was associated with Ballymulcashell in County Clare. Woulfe says that a registrar in Munster changed the name to Mountcashel c. 1840.English : in England, this name is common in Lincolnshire. While this may well be the result of migration from Ireland, the possibility of a habitational name from an unidentified place should not be ruled out.

    Mountcastle

  • Hooker
  • Surname or Lastname

    English (mainly southeastern)

    Hooker

    English (mainly southeastern) : variant of Hook (in the occupational or topographic and habitational senses), with the addition of the agent suffix -er.Congregational clergyman Thomas Hooker (1586?–1647) sailed from England with John Cotton and Samuel Stone and arrived in Boston in 1633. He led the 1635 migration of most of his congregation to Hartford in the Connecticut Valley. Thomas is the earliest known entrant, but the name Hooker is common and was also introduced independently by others during the 17th and 18th centuries.

    Hooker

  • Skipwith
  • Surname or Lastname

    English (Yorkshire)

    Skipwith

    English (Yorkshire) : habitational name from a place in Yorkshire, recorded in Domesday Book as Schipwic, from Old English scēap, scīp ‘sheep’ + wīc ‘outlying settlement’. Under later Scandinavian influence the initial ‘s’ became ‘sk’ and the second element was changed to -with (Old Norse viðr ‘wood’).The main Skipwith family held the manor of Skipwith in England in the early Middle Ages, and direct descendants can be traced to the present day. In the 13th century they moved from Yorkshire to Lincolnshire, where their principal seat was at southern Ormsby. In the early 17th century there was further migration, to Leicestershire, Warwickshire, and across the Atlantic to VA. Other bearers of the name seem to have been tenants of Lincolnshire manors held by the Skipworth family, and to have taken the surname of their overlords.

    Skipwith

  • Warnes
  • Surname or Lastname

    English (East Anglia)

    Warnes

    English (East Anglia) : of uncertain origin. There is a family tradition that the name is of Low German origin; probably a variant of Warns. There was fairly extensive migration from the Low Counties to East Anglia during the Middle Ages in connection with the wool trade.

    Warnes

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Online names & meanings

  • Sawaira
  • Girl/Female

    Arabic

    Sawaira

    Morning

  • Najih |
  • Boy/Male

    Muslim

    Najih |

    Sound, Good opinion, Successful

  • Amesh
  • Boy/Male

    Indian, Tamil

    Amesh

    Sweet Like a Mango

  • Avikalp | அவிகல்ப
  • Boy/Male

    Tamil

    Avikalp | அவிகல்ப

    The meaning of this name is which has no options

  • Abul-Faraj
  • Boy/Male

    Arabic, Muslim

    Abul-Faraj

    Comfortable; Possessor of Comfort; Father of Comfort

  • Surarchita
  • Boy/Male

    Hindu, Indian, Kannada, Telugu

    Surarchita

    Worshipped by Celestials

  • Faun
  • Girl/Female

    Australian, French, Latin

    Faun

    Young Deer

  • Bhaumi | பௌமீ
  • Girl/Female

    Tamil

    Bhaumi | பௌமீ

    Goddess Sita

  • APOPHIS
  • Male

    Greek

    APOPHIS

    (Άποφις) Greek form of Egyptian Apep, possibly APOPHIS means "to slither."  In mythology, Apep is the personification of evil, seen as a giant snake, serpent or dragon. Known as the Serpent of the Nile or Evil Lizard, he was an enemy of the sun god. 

  • Walsworth
  • Surname or Lastname

    English (West Yorkshire)

    Walsworth

    English (West Yorkshire) : variant of Walworth.

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Other words and meanings similar to

PLANETARY MIGRATION

AI search in online dictionary sources & meanings containing PLANETARY MIGRATION

PLANETARY MIGRATION

  • Exodus
  • n.

    A going out; particularly (the Exodus), the going out or journey of the Israelites from Egypt under the conduct of Moses; and hence, any large migration from a place.

  • Planetary
  • a.

    Of or pertaining to the planets; as, planetary inhabitants; planetary motions; planetary year.

  • Planetary
  • a.

    Consisting of planets; as, a planetary system.

  • Transmigration
  • n.

    The act of passing from one country to another; migration.

  • Intermigration
  • n.

    Reciprocal migration; interchange of dwelling place by migration.

  • Commigration
  • n.

    Migration together.

  • Placentary
  • a.

    Having reference to the placenta; as, the placentary system of classification.

  • Planetary
  • a.

    Caused by planets.

  • Migration
  • n.

    The act of migrating.

  • Plantar
  • a.

    Of or pertaining to the sole of the foot; as, the plantar arteries.

  • Aberration
  • n.

    A small periodical change of position in the stars and other heavenly bodies, due to the combined effect of the motion of light and the motion of the observer; called annual aberration, when the observer's motion is that of the earth in its orbit, and daily or diurnal aberration, when of the earth on its axis; amounting when greatest, in the former case, to 20.4'', and in the latter, to 0.3''. Planetary aberration is that due to the motion of light and the motion of the planet relative to the earth.

  • Planary
  • a.

    Of or pertaining to a plane.

  • Planetary
  • a.

    Having the nature of a planet; erratic; revolving; wandering.

  • Planetary
  • a.

    Under the dominion or influence of a planet.

  • Hamster
  • n.

    A small European rodent (Cricetus frumentarius). It is remarkable for having a pouch on each side of the jaw, under the skin, and for its migrations.

  • Direct
  • a.

    In the direction of the general planetary motion, or from west to east; in the order of the signs; not retrograde; -- said of the motion of a celestial body.

  • Remigration
  • n.

    Migration back to the place from which one came.