2013 FS28

2013 FS28 is an extreme trans-Neptunian object from the extended scattered disc on a highly eccentric orbit in the outermost region of the Solar System. It measures approximately 466 kilometers (290 miles) in diameter and is "probably" a dwarf planet. The detached, extended scattered disc object belongs to the group of extreme trans-Neptunian objects. It was first observed on 16 March 2013, by American astronomers Scott Sheppard and Chad Trujillo at the Cerro Tololo Observatory in Chile.[3][1][2]

2013 FS28
Discovery[1][2]
Discovered by(first observed only)
S. S. Sheppard[3]
C. Trujillo[3]
Discovery siteCerro Tololo Obs.
Discovery date16 March 2013
Designations
2013 FS28
TNO[4] · ESDO[5]
p-DP[6] · ETNO
distant[1]
Orbital characteristics[4]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 7
Observation arc1.13 yr (412 d)
Aphelion360.39 AU
Perihelion34.362 AU
197.37 AU
Eccentricity0.8259
2773 yr (1,012,826 d)
348.04°
 0m 1.44s / day
Inclination13.027°
204.66°
101.75°
Neptune MOID8.3 AU[1]
Physical characteristics
Mean diameter
464 km (est.)[5]
468 km (est.)[6]
0.07 (assumed)[6]
0.09 (assumed)[5]
4.9[1][4]

    Orbit and classification

    2013 FS28 orbits the Sun at a distance of 34.4–360 AU once every 2773 years (1,012,826 days; semi-major axis of 197 AU). Its orbit has an exceptionally high eccentricity of 0.83 and an inclination of 13° with respect to the ecliptic.[4] It has a minimum orbital intersection distance with Neptune of 8.3 AU.[1] The body's observation arc begins with its first official observation in March 2013, using the 4-meter Blanco Telescope at Cerro Tololo Observatory (807).[3][1]

    It belongs to a small group of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 150 AU or more.[7] Such extreme trans-Neptunian objects (ETNOs) can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine.

    Numbering and naming

    As of 2018, this minor planet has neither been numbered nor named by the Minor Planet Center. The official discoverer(s) will be defined when the object is numbered.[1]

    Physical characteristics

    According to the Johnston's archive and to American astronomer Michael Brown, 2013 FS28 measures 464 and 468 kilometers in diameter based on an assumed albedo of 0.09 and 0.07, respectively.[5][6] On his website, Michael Brown lists this object as "probably" a dwarf planet (400–500 km) based on his 5-class taxonomic system that ranges from "nearly certainly" to "possibly".[6] As of 2018, no rotational lightcurve of has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[4][8]

    See also

    References

    1. "2013 FS28". Minor Planet Center. Retrieved 25 October 2018.
    2. "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 25 October 2018.
    3. Sheppard, S. S.; Trujillo, C. (August 2016). "2013 FS28". Minor Planet Electronic Circular (2016-Q38). Bibcode:2016MPEC....Q...38S. Retrieved 25 October 2018.
    4. "JPL Small-Body Database Browser: (2013 FS28)" (2014-05-02 last obs.). Jet Propulsion Laboratory. Retrieved 25 October 2018.
    5. "List of Known Trans-Neptunian Objects". Johnston's Archive. 7 October 2018. Retrieved 25 October 2018.
    6. Brown, Michael E. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. Retrieved 25 October 2018.
    7. "Database Query: objects q>30, a>150". Minor Planet Center. Retrieved 25 October 2018.
    8. "LCDB Data for (2013+FS28)". Asteroid Lightcurve Database (LCDB). Retrieved 25 October 2018.

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