A New Planet in the Outer Solar System?
Michael “Migo” Mueller Rijksuniversiteit Groningen, Kapteyn Astronomical Ins tute
6th Quantum Universe Symposium Groningen March 2016
Planets move rela ve to stars: ἀστήρ πλανήτης ~ wandering star 5 planets are visible to the naked eye
February 5, 2016. Photo by Greg Hogan 5 planets are visible to the naked eye
February 5, 2016. Photo by Greg Hogan Pre Copernicus: Post Copernicus: Planeten Saturn
Jupiter
Mercury Venus
Earth Mars
1 AU Post Copernicus: Planeten Saturn
Jupiter
Mercury Venus
Earth Mars
1 AU ~ 1.5e27 fm First discovery of a planet: William Herschel discovers Uranus (1781)
Herschel was actually studying stellar parallax, found a moving object (“comet”) serendipitously. First discovery of a planet: William Herschel discovers Uranus (1781)
Herschel was actually studying stellar parallax, found a moving object (“comet”) serendipitously.
Previous observers had seen Uranus, but failed to recognize its apparent mo on (or resolvable size). Uranus
Saturn
Jupiter Enter classical mechanics / perturba on theory
1766—1786: Laplace and Lagrange pioneer what we now call ‘perturba on theory’ to explain planetary mo on. Enter classical mechanics / perturba on theory
1766—1786: Laplace and Lagrange pioneer what we now call ‘perturba on theory’ to explain planetary mo on. 1840s: problems with Uranus
Le Verrier: mismatch between Uranus’ predicted and observed posi ons. Solu on: add an extra planet! Predicts posi on and mass of new planet.
U. Le Verrier 1846: Urbain Le Verrier predicts a planet. Johann Galle discovers it • within hours of receiving Le Verrier’s le er • within a degree of the predicted posi on
J. Galle, Sternwarte Berlin
U. Le Verrier, obs. Paris 1846: Urbain Le Verrier predicts a planet. Johann Galle discovers it • within hours of receiving Le Verrier’s le er • within a degree of the predicted posi on
J. Galle, Sternwarte Berlin
U. Le Verrier, obs. Paris Neptune
Uranus
Saturn
Jupiter Mercury’s perihelion precession
Leading order (secular) perturba on theory: Interac on term doesn’t depend on angular variables à argument of perihelion changes at constant rate (apsis precession)
U. Le Verrier Mercury’s perihelion precession
Le Verrier (1859): mismatch between predicted and observed perihelion precession of Mercury • Venus: ~280”/100yr • Jupiter: ~150”/100yr • Other planets: ~100”/100yr • Total predicted: ~530”/100yr
• Observed: ~570”/100yr
Is there another planet interior to Mercury?
U. Le Verrier Mercury’s perihelion precession
Le Verrier (1859): mismatch between predicted and observed perihelion precession of Mercury • Venus: ~280”/100yr • Jupiter: ~150”/100yr • Other planets: ~100”/100yr • Total predicted: ~530”/100yr
• Observed: ~570”/100yr
Is there another planet interior to Mercury?
NO!
U. Le Verrier Mercury’s perihelion precession
Le Verrier (1859): mismatch between predicted and observed perihelion precession of Mercury • Venus: ~280”/100yr • Jupiter: ~150”/100yr • Other planets: ~100”/100yr • Total predicted: ~530”/100yr
• Observed: ~570”/100yr
General Rela vity explains the small discrepancy. Mercury’s perihelion precession
Le Verrier (1859): mismatch between predicted and observed perihelion precession of Mercury • Venus: ~280”/100yr • Jupiter: ~150”/100yr • Other planets: ~100”/100yr • Total predicted: ~530”/100yr
• Observed: ~570”/100yr
General Rela vity explains the small discrepancy. Another outer planet? Small residuals in posi ons of Uranus and Neptune.
Percival Lowell
Lowell Observatory, Flagstaff 1930: Clyde Tombaugh discovers Pluto
Clyde Tombaugh: 23 years Pluto
Neptun Pluto’s exponen al mass loss
Lowell’s predic on
At discovery
First diameter measurement
Discovery of moon Charon
M. Standish, 1993: new mass measurement of Neptune (by Voyager) explains orbits of Uranus and Neptune. Pluto is not needed (yet present) Pluto’s exponen al mass loss
Lowell’s predic on
At discovery
First diameter measurement
Discovery of moon Charon
M. Standish, 1993: new mass measurement of Neptune (by Voyager) explains orbits of Uranus and Neptune. Pluto is not needed (yet present)
2016: discovery of a new planet adver zed in press. Batygin & Brown, 2016 Frequently referred to as “Planet X”, we’ll call it P9.
M. Brown K. Batygin M. Brown K. Batygin 2016: discovery of a new planet adver zed in press. Batygin & Brown, 2016
M. Brown K. Batygin
Sedna has siblings! (on similarly detached orbits) • Sedna et al. (green) display conspicuous clustering. • Perihelion precession should randomize orbits, this happens in Kuiper belt (red).
1000 AU Also, same orienta on rela ve to eclip c plane.
Above eclip c Below eclip c Also, same orienta on rela ve to eclip c plane.
Likelihood of both things happening coincidentally: 0.007% ~ 3.8σ Batygin & Brown: A new distant planet stabilizes these orbits (and destabilizes others). N-body simula ons over 4 Gyr:
t=-4.0E9 yr N-body simula ons over 4 Gyr:
t=-3.0E9 yr N-body simula ons over 4 Gyr:
t=-2.0E9 yr N-body simula ons over 4 Gyr:
t= now
What do we know about Planet 9?
• We have not seen it, yet. What do we know about Planet 9?
• We have not seen it, yet. • We do know where to look, and the search is on! What do we know about Planet 9?
• We have not seen it, yet. • We do know where to look, and the search is on! • Orbit • Perihelion ~ 200 AU • Aphelion ~ 1,200 AU • Period 10,000—20,000 yr • Inclina on ~ 20 deg (!) • Mass • 5—10 * Earth ~ 0.5 * Neptune • Composi on • Ice giant? How come we haven’t seen it, yet?
aphelion
perihelion faint
çè
Bright
P9 isn’t par cularly faint, but the sky is big. Orbital phase unknown! Near perihelion, we’d probably have seen P9. But it could easily be hiding elsewhere. Even at aphelion, P9 is easily detectable with dedicated telescope obs. xkcd.com/1633 The search is on!
Two strategies • Direct detec on of P9; survey of orbit should take ~5 yr • Try and find more Sednas (similar or dissimilar orbits?) Conclusions
It’s hard to make predic ons, especially about the future (a ributed to Niels Bohr)
• 1846, Neptune: right predic on, planet found.
• 1930, Pluto: wrong predic on, found something unexpected.
• 2016, P9: convincing predic on. The planet, if it exists, should be found in the next few years. Telescope me well spent.
• If P9 exists: why? A highly inclined, detached planet is difficult to fit in. If not: how else can we explain Sednas?
It stays interes ng!