474640 Alicanto

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474640 Alicanto
Discovery 
Perihelion
47.289 AU
328 AU (barycentric)[5]
332.80 AU
Eccentricity0.8579
5900 yr (barycentric)[5]
6071 yr (2,217,590 d)
0.6822°
0° 0m 0.72s / day
Inclination25.572°
65.996°
326.72°
Physical characteristics
Mean diameter
0.04 (est.)[6]
23.3[10]
6.5[1][3]

474640 Alicanto (

Andrew C. Becker at Cerro Tololo Inter-American Observatory in Chile. It never gets closer than 47 AU from the Sun (near the outer edge of the main Kuiper belt) and averages more than 300 AU from the Sun. Its large eccentricity strongly suggests that it was gravitationally scattered onto its current orbit. Because it is, like all detached objects, outside the current gravitational influence of Neptune, how it came to have this orbit cannot yet be explained. It was named after Alicanto
, a nocturnal bird in Chilean mythology.

Discovery and orbit

Alicanto's orbit in red with hypothetical Planet Nine

Alicanto was discovered by American astronomer

opposition
at the start of November.

With an

AU, Alicanto is an extreme trans-Neptunian object which are practically detached from Neptune's gravitational influence. Its orbit is characterized by high eccentricity (0.850), moderate inclination (25.58°) and a semi-major axis of 316 AU.[1] Upon discovery, it was classified as a trans-Neptunian object. Its orbit is well determined; as of 11 January 2017 its orbital solution is based on 34 observations spanning a data-arc of 5821 days.[3] Alicanto's orbit is similar to that of 2013 RF98, indicating that they may have both been thrown onto the orbit by the same body, or that they may have been the same object (single or binary) at one point.[9][12]

Naming

On 14 May 2021, the object was named by the

Working Group for Small Bodies Nomenclature (WGSBN) after Alicanto from Chilean mythology. The nocturnal bird of the Atacama Desert has wings that shine at night with beautiful, metallic colors.[2]

Physical characteristics

Alicanto has an absolute magnitude of 6.5 which gives a characteristic diameter of 130 to 300 km for an assumed albedo in the range 0.25–0.05.[7]

Michael Brown's website lists it as a possible dwarf planet with a diameter of 314 kilometres (195 mi) based on an assumed albedo of 0.04.[6] The albedo is expected to be low because the object has a blue (neutral) color.[6] However, if the albedo is higher, the object could easily be half that size.

Alicanto's visible spectrum is very different from that of 90377 Sedna.[9][13] The value of its spectral slope suggests that the surface of this object can have pure methane ices (like in the case of Pluto) and highly processed carbons, including some amorphous silicates.[9] Its spectral slope is similar to that of 2013 RF98.[9]

Relevance to the Planet Nine Hypothesis

Main article: Planet Nine

This minor planet is one of a number of objects discovered in the Solar System to have a

argument of perihelion of 340 ± 55°.[14]
Of these, only eight, including Alicanto, have perihelia beyond Neptune's current influence.

Comparison

The orbits of Sedna, 2012 VP113, Leleākūhonua, and other very distant objects along with the predicted orbit of Planet Nine. The three sednoids (pink) along with the red-colored extreme trans-Neptunian object (eTNO) orbits are suspected to be aligned with the hypothetical Planet Nine while the blue-colored eTNO orbits are anti-aligned. The highly elongated orbits colored brown include centaurs and damocloids with large aphelion distances over 200 AU.

See also

References

  1. ^ a b c d e f g "(474640) Alicanto". Minor Planet Center. Retrieved 18 May 2021.
  2. ^ a b c "WGSBN Bulletin Archive". Working Group for Small Bodies Nomenclature. 14 May 2021. Retrieved 16 May 2021. (Bulletin #1)
  3. ^ a b c d e f g h "JPL Small-Body Database Browser: 474640 (2004 VN112)" (2016-09-03 last obs.). Jet Propulsion Laboratory. Retrieved 18 May 2021.
  4. ^
    Marc W. Buie (8 November 2007). "Orbit Fit and Astrometric record for 04VN112". SwRI (Space Science Department). Archived from the original
    on 18 August 2010. Retrieved 17 July 2008.
  5. ^ a b c Horizons output. "Barycentric Osculating Orbital Elements for 2004 VN112". Retrieved 20 September 2021. (Ephemeris Type:Elements and Center:@0)
  6. ^ a b c d e Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. Retrieved 18 September 2016.
  7. ^ a b "Asteroid Size Estimator". CNEOS NASA/JPL. Retrieved 12 November 2017.
  8. ^ a b c d "LCDB Data for (474640) Alicanto". Asteroid Lightcurve Database (LCDB). Retrieved 18 May 2021.
  9. ^
    S2CID 119419889
    .
  10. ^ a b "AstDyS 2004 VN112 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 28 March 2014.
  11. ^ Discovery MPEC
  12. S2CID 118890903
    .
  13. ^ "JPL Small-Body Database Browser: 90377 Sedna (2003 VB12)". Retrieved 28 March 2014.
  14. JPL Solar System Dynamics
    . Retrieved 9 April 2014.

External links

Retrieved from "https://en.wikipedia.org/w/index.php?title=474640_Alicanto&oldid=1209202496"