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OBSERVATIONAL CONSTRAINTS ON PLANET NINE: ASTROMETRY OF PLUTO AND OTHER TRANS-NEPTUNIAN OBJECTS
Open accessAbstract
We use astrometry of Pluto and other trans-neptunian objects to constrain the sky location, distance, and mass of the possible additional planet (Planet Nine) hypothesized by Batygin & Brown. We find that over broad regions of the sky, the inclusion of a massive, distant planet degrades the fits to the observations. However, in other regions, the fits are significantly improved by the addition of such a planet. Our best fits suggest a planet that is either more massive or closer than argued for by Batygin & Brown based on the orbital distribution of distant trans-neptunian objects (or by Fienga et al. based on range measured to the Cassini spacecraft). The trend to favor larger and closer perturbing planets is driven by the residuals to the astrometry of Pluto, remeasured from photographic plates using modern stellar catalogs, which show a clear trend in decl. over the course of two decades, that drive a preference for large perturbations. Although this trend may be the result of systematic errors of unknown origin in the observations, a possible resolution is that the decl. trend may be due to perturbations from a body, in addition to Planet Nine, that is closer to Pluto but less massive than Planet Nine.
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Cites
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BackgroundChaotic capture of Jupiter's Trojan asteroids in the early Solar System
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BackgroundEvidence for a Distant Giant Planet in the Solar System
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BackgroundSelf-citationDiscovery of a Planetary-sized Object in the Scattered Kuiper Belt
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ORBITS AND MASSES OF THE SATELLITES OF THE DWARF PLANET HAUMEA (2003 EL61)
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A SEARCH FOR A DISTANT COMPANION TO THE SUN WITH THE WIDE-FIELD INFRARED SURVEY EXPLORER
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BackgroundConstraints on the location of a possible 9th planet derived from the Cassini data
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BackgroundA distant planetary-mass solar companion may have produced distant detached objects
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“…Planet Nine could account for peculiar features of that distribution, upper limits from dynamical effects that are not observed (Hogg et al. 1991; Iorio 2009, 2012, 2014), nondetections in optical (Brown et al. 2015) and infrared surveys (Luhman 2014), and models of the physical properties such…”
BackgroundPhysical properties of trans-neptunian binaries (120347) Salacia–Actaea and (42355) Typhon–Echidna
Stansberry, J., Grundy, W. M., Mueller, M. M., Benecchi, S., Rieke, G. H., Noll, K., Buie, M. W., Levison, H. F., Porter, S. B., & Roe, H. G. (2012) · Icarus · doi:10.1016/j.icarus.2012.03.029 · Cited by 66
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“Some investigations have argued for closer planets, possibly more than one(Brunini & Melita 2002; Lykawka & Mukai 2008; Bromley & Kenyon 2016; Kenyon & Bromley 2016).”
BackgroundInfluentialDynamical limits on dark mass in the outer solar system
Hogg, D. W., Quinlan, G. D., & Tremaine, S. (1991) · The Astronomical Journal · doi:10.1086/115849 · Cited by 57 · cited 4×
“We further assume that Planet Ninefollows a keplerian orbit and is itself unperturbed by the other planets. We refer to this approach as the “moving planet model.” For our second approach, following Hogg et al. (1991), we assume that the additional planet is stationary and is suciently distant that its gravitational p…”
BackgroundInfluentialPlanet X revamped after the discovery of the Sedna-like object 2012 VP113?
Iorio, L. (2014) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1093/mnrasl/slu116 · Cited by 56 · cited 1×
“…Planet Nine could account for peculiar features of that distribution, upper limits from dynamical effects that are not observed (Hogg et al. 1991; Iorio 2009, 2012, 2014), nondetections in optical (Brown et al. 2015) and infrared surveys (Luhman 2014), and models of the physical properties such…”
BackgroundPlanet X - No dynamical evidence in the optical observations
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“was not suciently massive to account for them. Improved planetary ephemerides, based on more accurate planetary masses and careful vetting of observational data, eliminated most of those residuals (Standish 1993; Quinlan 1993). Nevertheless, the discovery of the Kuiper belt (Jewitt and Luu 1993), including its intrica…”
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The mass, orbit, and tidal evolution of the Quaoar–Weywot system
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“haller (2007) (134340) Pluto+Charon – 7:33 10 9 - Stern et al. (2015) (136108) Haumea 11-58 2:01 10 9 3:4 10 15 5:3 10 13 Ragozzine and Brown (2009) (50000) Quaoar 13-39 7:0 10 10 1:2 10 14 3:2 10 13 Fraser et al. (2013) (90377) Sedna 108-130 5:0 1610 10 3:2 10 5:6 10 16 Assumed (90482) Orcus 35-73 3:2 10 10 1:8 10 15…”
Precise predictions of stellar occultations by Pluto, Charon, Nix, and Hydra for 2008–2015
Assafin, M., Camargo, J. I. B., Vieira-Martins, R., Andrei, A. H., Sicardy, B., Young, L. A., Neto, D. N. D. S., & Braga-Ribas, F. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913690 · Cited by 48 · cited 5×
“1995); Pluto or Charon positions from recent occultation measurements of Pluto and Charon (Assafin et al. 2010; Benedetti-Rossi et al. 2014); and CCD observations from Pico dos Dias Observatory (Benedetti-Rossi et al. 2014), the USNO’s Flagstaff Station (Stone et al. 2003), and JPL’s Table Mountain Observatory (descri…”
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“rbidelli et al. 2005; Tsiganis et al. 2005; Levison et al. 2008), additional giant planets formed ˘5 35 AU from the Sun and then scattered within or ejected from the solar system (Chiang et al. 2007; Bromley and Kenyon 2014, 2016b), or the formation of planets at larger distances (Kenyon and Bromley 2015, 2016b). 1 ar…”
BackgroundAstrometric Microlensing Constraints on a Massive Body in the Outer Solar System withGaia
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“That celebrated success ensured that scientists would sporadically revisit the possibility of yet undiscovered planets in the solar system (see Tremaine 1990; Hogg et al. 1991 and Gaudi & Bloom 2005 for reviews).”
BackgroundResultInfluentialFORMATION OF SUPER-EARTH MASS PLANETS AT 125–250 AU FROM A SOLAR-TYPE STAR
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“…2005; Tsiganis et al. 2005; Levison et al. 2008), additional giant planets formed ~5 35 au– from the Sun and then scattered within or ejected from the solar system(Chiang et al. 2007, p. 895; Bromley & Kenyon 2014, 2016), or the formation of planets at larger distances(Kenyon & Bromley 2015, 2016).”
BackgroundIntegral-field spectroscopy of (90482) Orcus-Vanth
Carry, B., Hestroffer, D., DeMeo, F. E., Thirouin, A., Berthier, J., Lacerda, P., Sicardy, B., Doressoundiram, A., Dumas, C., Farrelly, D., et al. (2011) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201117486 · Cited by 41
Dark Matter in the Solar System
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“That celebrated success ensured that scientists would sporadically revisit the possibility of yet undiscovered planets in the solar system (see Tremaine 1990; Hogg et al. 1991 and Gaudi & Bloom 2005 for reviews).”
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BackgroundAccount of the Discovery of the Planet of Le Verrier at Berlin
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MAKING PLANET NINE: A SCATTERED GIANT IN THE OUTER SOLAR SYSTEM
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“Some investigations have argued for closer planets, possibly more than one(Brunini & Melita 2002; Lykawka & Mukai 2008; Bromley & Kenyon 2016; Kenyon & Bromley 2016).”
BackgroundRobert, V., de Cuyper, J. P., Arlot, J.-E., de Decker, G., Guibert, J., Lainey, V. J., Pascu, D., Winter, L., & Zacharias, N. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18747.x · Cited by 35
A SERENDIPITOUS ALL SKY SURVEY FOR BRIGHT OBJECTS IN THE OUTER SOLAR SYSTEM
Brown, M. E., Bannister, M. T., Schmidt, B. P., Drake, A. J., Djorgovski, S. G., Graham, M. J., Mahabal, A., Donalek, C., Larson, S., Christensen, E., et al. (2015) · The Astronomical Journal · doi:10.1088/0004-6256/149/2/69 · Cited by 33 · cited 2×
“ow Planet Ninecould account for peculiar features of that distribution; upper limits from dynamical eects that are not observed (Hogg et al. 1991; Iorio 2009, 2012, 2014); non-detections in optical (Brown et al. 2015) and infrared surveys (Luhman 2014); and models of the physical properties such a planet might have (G…”
BackgroundMaking planet nine: Pebble accretion at 250–750 AU in a gravitationally unstable ring
Kenyon, S. J., & Bromley, B. C. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/825/1/33 · Cited by 33 · cited 2×
“Some investigations have argued for closer planets, possibly more than one(Brunini & Melita 2002; Lykawka & Mukai 2008; Bromley & Kenyon 2016; Kenyon & Bromley 2016).”
BackgroundComputation of preliminary orbits
Herget, P. (1965) · The Astronomical Journal · doi:10.1086/109671 · Cited by 27 · cited 2×
“centric unit vector directed from the observatory to the observed location. However, when comparing the calculated sky position with those observed, we resolve the diflocal tangent plane projections (Herget 1965). 2.We replaced Orbfit’s analytic but approximate expressions for the derivatives of the observable properti…”
BackgroundMethodPluto: improved astrometry from 19 years of observations
Benedetti-Rossi, G., Vieira-Martins, R., Camargo, J. I. B., Assafin, M., & Braga-Ribas, F. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201424275 · Cited by 20 · cited 6×
“…occultation measurements of Pluto and Charon(Assafin et al. 2010; Benedetti-Rossi et al. 2014); and CCD observations from Pico dos Dias Observatory(Benedetti-Rossi et al. 2014), the USNO’s Flagstaff Station(Stone et al. 2003), and JPL’s Table Mountain Observatory (described in Buie & Folkner…”
BackgroundMethodResultInfluentialStone, R. C., Monet, D. G., Monet, A. K. B., Harris, F. H., Ables, H. D., Dahn, C. C., Canzian, B., Guetter, H. H., Harris, H. C., Henden, A. A., et al. (2003) · The Astronomical Journal · doi:10.1086/377622 · Cited by 19 · cited 2×
“…measurements of Pluto and Charon(Assafin et al. 2010; Benedetti-Rossi et al. 2014); and CCD observations from Pico dos Dias Observatory(Benedetti-Rossi et al. 2014), the USNO’s Flagstaff Station(Stone et al. 2003), and JPL’s Table Mountain Observatory (described in Buie & Folkner 2015).”
MethodThe edge of the Kuiper belt: the Planet X scenario
Melita, M. D., Williams, I. P., Collander-Brown, S. J., & Fitzsimmons, A. (2004) · Icarus · doi:10.1016/j.icarus.2004.05.014 · Cited by 16 · cited 1×
“…object embedded in the KB region, proposing that such an object could naturally explain the observed “edge” in the KB distribution at ∼50 au, although later work found that such a body would be inconsistent with other features of the observed orbital distribution of TNOs (Melita et al. 2004).”
BackgroundRyl'Kov, V. P., Vityazev, V. V., & Dementieva, A. (1995) · Astronomical and Astrophysical Transactions · doi:10.1080/10556799508232072 · Cited by 14
ASTROMETRY OF PLUTO FROM 1930–1951 OBSERVATIONS: THE LAMPLAND PLATE COLLECTION
Buie, M. W., & Folkner, W. M. (2014) · The Astronomical Journal · doi:10.1088/0004-6256/149/1/22 · Cited by 10 · cited 8×
“Buie and Folkner (2015) took great care to develop a reliable astrometric data set with which to better determine Pluto’s orbit.”
BackgroundMethodResultInfluentialConstraints on planet X/Nemesis from Solar System's inner dynamics
Iorio, L. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15458.x · Cited by 8 · cited 2×
“from the observed orbital distribution of TNOs and how Planet Ninecould account for peculiar features of that distribution; upper limits from dynamical eects that are not observed (Hogg et al. 1991; Iorio 2009, 2012, 2014); non-detections in optical (Brown et al. 2015) and infrared surveys (Luhman 2014); and models of…”
Background(1993) · Nature · doi:10.1038/363018b0 · Cited by 1 · cited 2×
“ntly massive to account for them. Improved planetary ephemerides, based on more accurate planetary masses and careful vetting of observational data, eliminated most of those residuals (Standish 1993; Quinlan 1993). Nevertheless, the discovery of the Kuiper belt (Jewitt and Luu 1993), including its intricate dynamical…”
Background
Flagged first, then by citations
Research works printed but not linked: 5
- Bouvard, 1824, AN, 2, 441
- Folkner, 2014, IPNPR, 42, 1
- Le Verrier, 1846a, AN, 25, 53
- Le Verrier, 1846b, AN, 25, 65
- Press, 1986
Cited by
Sorted by citations
Batygin, K., Adams, F. C., Brown, M. E., & Becker, J. C. (2019) · Physics Reports · doi:10.1016/j.physrep.2019.01.009 · Cited by 181
New Extreme Trans-Neptunian Objects: Toward a Super-Earth in the Outer Solar System
Sheppard, S. S., & Trujillo, C. (2016) · The Astronomical Journal · doi:10.3847/1538-3881/152/6/221 · Cited by 92
“Fienga et al. (2016) and Holman & Payne (2016a, 2016b) have looked further into the Cassini tracking and planetary ephemerides to put limits on the size and distance of an unseen massive planet in the outer solar system.”
BackgroundThe Curiously Warped Mean Plane of the Kuiper Belt
Volk, K., & Malhotra, R. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa79ff · Cited by 61
“It is also pertinent to note that Holman & Payne (2016a) recently identified ranges of mass and distance combinations for an unseen planet whose perturbations could improve the orbit-fit residuals for Pluto and other KBOs.”
BackgroundMethodInfluentialChen (陳英同), Y.-T., Lin (林省文), H. W., Holman, M. J., Payne, M. J., Fraser, W. C., Lacerda, P., Ip (葉永烜), W.-H., Chen (陳文屏), W.-P., Kudritzki, R.-P., Jedicke, R., et al. (2016) · The Astrophysical Journal Letters · doi:10.3847/2041-8205/827/2/l24 · Cited by 60
Self-citationZeebe, R. E. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa8cce · Cited by 55
“Note that P9’s existence and hence its orbit is entirely speculative at this point (Trujillo & Sheppard 2014; Brown & Batygin 2016; Batygin & Brown 2016; Fienga et al. 2016; Malhotra et al. 2016; Holman & Payne 2016; Shankman et al. 2017; Millholland & Laughlin 2017).”
BackgroundDynamical evolution induced by planet nine
Batygin, K., & Morbidelli, A. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/aa937c · Cited by 58
“…prospects for the direct detection of Planet Nine either through ongoing or future surveys are quite promising (Brown & 19 Batygin 2016; Holman & Payne 2016a,b; Fortney et al. 2016; Millholland & Laughlin 2017), and it is likely that the concluding assessment of the theoretical model…”
BackgroundBecker, J. C., Khain, T., Hamilton, S. J., Adams, F. C., Gerdes, D. W., Zullo, L., Franson, K., Millholland, S., Bernstein, G. M., Sako, M., et al. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aad042 · Cited by 52
“…and observational perspectives (Batygin & Brown 2016b; Bromley & Kenyon 2016; Chen et al. 2016; de la Fuente Marcos & de la Fuente Marcos 2016; Holman & Payne 2016a, 2016b; Kenyon & Bromley 2016; Li & Adams 2016; Malhotra et al. 2016; Mustill et al. 2016; Sheppard & Trujillo 2016; Batygin &…”
BackgroundConstraints on planet nine’s orbit and sky position within a framework of mean motion resonances
Millholland, S., & Laughlin, G. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/153/3/91 · Cited by 45
“Fienga et al. (2016) and Holman & Payne (2016b) derived similar constraints using the precise measurements of the Earth-Saturn distance obtained by the Cassini spacecraft.”
MethodInfluentialConsequences of a Distant Massive Planet on the Large Semimajor Axis Trans-Neptunian Objects
Shankman, C., Kavelaars, J. J., Lawler, S. M., Gladman, B. J., & Bannister, M. T. (2017) · The Astronomical Journal · doi:10.3847/1538-3881/153/2/63 · Cited by 42
“…and physical properties of P9 (Brown & Batygin 2016; de la Fuente Marcos & de la Fuente Marcos 2016a,b; Fienga et al. 2016; Fortney et al. 2016; Holman & Payne 2016b,a; Linder & Mordasini 2016; Philippov & Chobanu 2016; Toth 2016), the dynamical implications of P9 in the Solar System (de la…”
BackgroundResultThe fates of Solar system analogues with one additional distant planet
Veras, D. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2170 · Cited by 38
“…Brown & Batygin 2016; de la Fuente Marcos & de la Fuente Marcos 2016a,b; de la Fuente Marcos, de la Fuente Marcos & Aarseth 2016; Fienga et al. 2016; Holman & Payne 2016a,b; Lawler et al. 2016; Malhotra, Volk & Wang 2016) and intrinsic physical properties (Cowan, Holder & Kaib 2016; Fortney et…”
BackgroundWas Planet 9 captured in the Sun’s natal star-forming region?
Parker, R. J., Lichtenberg, T., & Quanz, S. P. (2017) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slx141 · Cited by 30
“A recent body of research (e.g. Trujillo & Sheppard 2014; Batygin & Brown 2016a,b; Brown & Batygin 2016; Holman & Payne 2016a,b) has suggested that the unusual orbital characteristics of several Edgeworth–Kuiper Belt Objects could be explained by the presence of an unseen/undiscovered ∼20M⊕ planet – the so-called ‘Pla…”
BackgroundInfluentialDi Ruscio, A., Fienga, A., Durante, D., Iess, L., Laskar, J., & Gastineau, M. (2020) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202037920 · Cited by 24
“Since then, many attempts to locate the elusive planet have followed (Fienga et al. 2016a, 2020; Folkner et al. 2016; Holman & Payne 2016a,b).”
BackgroundThe Secular Dynamics of TNOs and Planet Nine Interactions
Li, G., Hadden, S., Payne, M. J., & Holman, M. J. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aae83b · Cited by 26
“…of Planet Nine (Brown & Batygin 2016; de la Fuente Marcos & de la Fuente Marcos 2016) and by simulations of the tidal perturbation induced by Planet Nine on the relative distance between the Earth and the Cassini spacecraft (Holman & Payne 2016b) and Pluto and other TNOs (Holman & Payne 2016a).”
BackgroundSelf-citationIorio, L. (2017) · Astrophysics and Space Science · doi:10.1007/s10509-016-2993-8 · Cited by 21
“The possibility of using the ongoing telemetry of New Horizons, a further complementary feature of this work with respect to Fienga et al. (2016a); Holman & Payne (2016b), is discussed in Section 7.”
BackgroundMethodResultInfluentialRice, M., & Laughlin, G. (2020) · The Planetary Science Journal · doi:10.3847/psj/abc42c · Cited by 19
de León, J., Marcos, C. D. L. F., & Marcos, R. D. L. F. (2017) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slx003 · Cited by 16
Chaotic dynamics of trans-Neptunian objects perturbed by planet nine
Hadden, S., Li, G., Payne, M. J., & Holman, M. J. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aab88c · Cited by 16
“…by this suggestion, leading to a wide range of related topics being investigated, including: constraining its location (Brown & Batygin 2016; Holman & Payne 2016a,b); formation mechanisms (Bromley & Kenyon 2016; Kenyon & Bromley 2016; Li & Adams 2016; Mustill et al. 2016), atmospheric…”
BackgroundSelf-citationA Pluto–Charon Sonata: The Dynamical Architecture of the Circumbinary Satellite System
Kenyon, S. J., & Bromley, B. C. (2019) · The Astronomical Journal · doi:10.3847/1538-3881/aafa72 · Cited by 15
“The uncertain orbital path of Pluto across the sky is the main limitation in these predictions (e.g., Benedetti-Rossi et al. 2014; Holman & Payne 2016, and references therein).”
BackgroundMarcos, C. D. L. F., & Marcos, R. D. L. F. (2017) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slx106 · Cited by 11
“A closer perturber is also advocated by Holman & Payne (2016).”
BackgroundBinary stripping as a plausible origin of correlated pairs of extreme trans-Neptunian objects
Marcos, C. D. L. F., Marcos, R. D. L. F., & Aarseth, S. J. (2017) · Astrophysics and Space Science · doi:10.1007/s10509-017-3181-1 · Cited by 11
“…is more distant and more massive than the one thought to be sculpting the Kuiper Cliff, but its existence has not been ruled out by recent analyses carried out by e.g. Brown and Batygin (2016), Fienga et al. (2016), Holman and Payne (2016a, 2016b), Sheppard and Trujillo (2016), and Brown (2017).”
BackgroundInfluentialOldroyd, W. J., & Trujillo, C. A. (2021) · The Astronomical Journal · doi:10.3847/1538-3881/abfb6f · Cited by 11
Observational constraints on an undiscovered giant planet in our solar system
Trujillo, C. A. (2019) · Elsevier eBooks · doi:10.1016/b978-0-12-816490-7.00004-7 · Cited by 10
Gomes, D. C. H., Murray, Z., Gomes, R. C. H., Holman, M. J., & Bernstein, G. M. (2023) · The Planetary Science Journal · doi:10.3847/psj/acc7a2 · Cited by 9
“Fienga et al. (2020) reprised the investigation using the INPOP19a model, which includes the gravitational influence of the Kuiper Belt, and a tidal model as in Holman & Payne (2016b).”
BackgroundMethodInfluentialSelf-citationPaučo, R. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201630335 · Cited by 7
“…not result of an observational bias and/or smallness of the sample, and the quest of finding P9 was prompted (Brown & Batygin 2016; Cowan et al. 2016; de la Fuente Marcos & de la Fuente Marcos 2016; de la Fuente Marcos et al. 2016; Fortney et al. 2016; Fienga et al. 2016; Holman & Payne 2016b,a).”
BackgroundThe Influence of Planet Nine on the Orbits of Distant TNOs: The Case for a Low-perihelion Planet
Cáceres, J., & Gomes, R. S. (2018) · The Astronomical Journal · doi:10.3847/1538-3881/aad77a · Cited by 5
“…the location of Planet 9 on its orbit from the reduction of the residuals in Saturn’s orbital motion based on Cassini data (Fienga et al. 2016; Holman & Payne 2016a), or in Pluto’s orbit (Holman & Payne 2016b), or assuming that several of the distant TNOs are in mean motion resonance (MMR)…”
MethodOn the origin of extreme trans-Neptunian objects within Modified Newtonian Dynamics
Migaszewski, C. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad2250 · Cited by 6
A new approach to distant solar system object detection in large survey data sets
Perdelwitz, V., Völschow, M., & Müller, H. M. (2018) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201732254/pdf · Cited by 6
Paučo, R. (2017) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201630335/pdf · Cited by 5
The Case for a Large-scale Occultation Network
Rice, M., & Laughlin, G. (2019) · The Astronomical Journal · doi:10.3847/1538-3881/ab21df · Cited by 6
“Numerical simulations by Holman & Payne (2016b), Millholland & Laughlin (2017), Becker et al. (2017), and Batygin & Morbidelli (2017) (among others) have steadily refined the dynamical evidence and now point toward a planet with m ∼ 5− 10M⊕ with semimajor axis a ∼ 400− 800 AU.”
BackgroundA new approach to distant solar system object detection in large survey data sets
Perdelwitz, V., Völschow, M., & Müller, H. M. (2018) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201732254 · Cited by 5
“Several authors provide restrictions on the location of Planet Nine based on Cassini data (Fienga et al. 2016; Holman & Payne 2016b), motion of comets (Medvedev et al. 2017), a Monte Carlo approach (de la Fuente Marcos & de la Fuente Marcos 2016), astrometry of Trans-Neptunian Objects (TNOs)…”
MethodHas Kronos Devoured Planet Nine and Its Epigones?
Iorio, L. (2026) · Universe · doi:10.3390/universe12020042
“From the definition of Θ µν and using equation (2), we have In other words, Θ µν will depend on the Lagrangian of matter, that is, this can refer to the case of the electromagnetic field, the massless scalar field, the case of the perfect fluid, among others.”
Edmonds, I. (2022) · International Journal of Astronomy and Astrophysics · doi:10.4236/ijaa.2022.123013
Pulkovo Observations of the Major Planets, their Satellites and Pluto
Pitjeva, E. V., & Pavlov, D. (2025) · Solar System Research · doi:10.1134/s0038094624601646
Metadata
- Authors
- Holman, M. J., & Payne, M. J.
- Affiliations
- Center for Astrophysics Harvard & Smithsonian (US)
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2016-09-09
- Volume
- 152
- Issue
- 4
- Pages
- 80
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W2317010023
- Cited by
- 32
- References
- 56
- Citations by year
- 2025: 1 · 2023: 2 · 2022: 1 · 2021: 1 · 2020: 2 · 2019: 4 · 2018: 6 · 2017: 11 · 2016: 4
- FWCI
- 3.99
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- Locations
- The Astronomical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Engineering › Aerospace Engineering › Space Satellite Systems and Control
- Keywords
- Planet Nine, trans-Neptunian objects, orbital perturbations
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