Astronomy:(614689) 2020 XL5

Short description: Near-Earth Asteroid

(614689) 2020 XL₅

Discovery
Discovered by	Pan-STARRS 1
Discovery site	Haleakala Obs.
Discovery date	12 December 2020
Designations
MPC designation	(614689) 2020 XL5
Alternative designations	2020 XL5 · P11aRcq
Minor planet category	Earth trojan · NEO Apollo
Orbital characteristics
Epoch 21 January 2022 (JD 2459600.5)
Uncertainty parameter 0
Observation arc	8.88 yr (3,243 days)
Earliest precovery date	23 December 2012
|{{{apsis}}}|helion}}	1.388 AU
|{{{apsis}}}|helion}}	0.6133 AU
Semi-major axis	1.001 AU
Eccentricity	0.38713
Orbital period	1.00 yr (365.7 d)
Mean anomaly	316.420°
Mean motion	0° 59m 4.269s / day
Inclination	13.847°
Longitude of ascending node	153.598°
|{{{apsis}}}|helion}}	87.981°
Earth MOID	0.07571 AU (11,326,000 km)
Venus MOID	0.02726 AU (4,078,000 km)
Physical characteristics
Mean diameter	1.18±0.08 km
Geometric albedo	0.06±0.03
Spectral type	C
Apparent magnitude	20–23
Absolute magnitude (H)	18.58+0.16 −0.15 (r-band)

(614689) 2020 XL₅ is a near-Earth asteroid and Earth trojan discovered by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii on 12 December 2020. It oscillates around the Sun–Earth L₄ Lagrangian point (leading 60°), one of the dynamically stable locations where the combined gravitational force acts through the Sun's and Earth's barycenter. Analysis of 2020 XL₅'s trojan orbit stability suggests it will remain around Earth's L₄ point for at least four thousand years until gravitational perturbations from repeated close encounters with Venus destabilize its trojan configuration. With a diameter about 1.2 km (0.75 mi), 2020 XL₅ is the second Earth trojan discovered, after 2010 TK7, and is the largest of its kind known.

Discovery

2020 XL₅ was discovered by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii on 12 December 2020. It was first observed in the constellation Crater at an apparent magnitude of 21.4. The asteroid was moving at an on-sky rate of 3.02 arcseconds per minute, from a distance of 0.68 AU (102 million km; 63 million mi) from Earth.

The asteroid was subsequently listed on the Minor Planet Center's Near-Earth Object Confirmation Page (NEOCP) as P11aRcq. Over two days, follow-up observations were carried out by the Višnjan Observatory (L01), ESA Optical Ground Station (J04), and Cerro Tololo Observatory (807). The asteroid was identified in earlier Mount Lemmon Survey (G96) observations from 26 November 2020. The listing was confirmed and publicly announced as 2020 XL₅ on 14 December 2020.

Name and numbering

This minor planet was given the permanent number 614689 by the Minor Planet Center on 28 March 2022 and is now eligible for naming. In accordance with the International Astronomical Union's naming conventions for near-Earth objects, 2020 XL₅ will be given a mythological name.

Orbit and classification

Heliocentric orbit diagram of 2020 XL₅ along with the inner planets

The orbit of 2020 XL₅ is well known with an uncertainty parameter of 0 and a long observation arc over 8 years. The asteroid has been identified in several precovery observations by various sky surveys, including Pan-STARRS, from dates as far back as December 2012.

2020 XL₅ orbits the Sun at an average distance of 1.001 AU once every 365.8 days, or approximately 1 Earth year. Its orbit has a high eccentricity of 0.388 and an inclination of 13.8° with respect to the ecliptic plane. Over the course of its orbit, its distance from the Sun ranges from 0.61 AU at perihelion to 1.39 AU at aphelion, crossing the orbits of Venus and Earth. Since its orbit crosses that of Earth's while having a semi-major axis greater than 1 AU (by a small margin), 2020 XL₅ is classified as an Apollo asteroid.

Trojan orbit

Effective potential plot showing Earth's Lagrangian points (not to scale); contours around L₄ and L₅ represent tadpole loop paths

Animation of 2020 XL₅'s orbit from 1600 to 2500 - relative to Sun and Earth   Sun ·   Earth ·   2020 XL₅

Trojan objects are most easily conceived as orbiting at a Lagrangian point, a dynamically stable location (where the combined gravitational force acts through the Sun's and Earth's barycenter) 60 degrees ahead of (L₄) or behind (L₅) a massive orbiting body, in a type of 1:1 orbital resonance. In reality, they oscillate around such a point.

On 26 January 2021, amateur astronomer Tony Dunn reported that 2020 XL₅'s nominal trajectory appears to be librating about Earth's leading L₄ Lagrangian point, suspecting it to be an Earth trojan. Subsequent analysis confirmed modeling stability for at least several thousand years into the future based on existing orbital parameters. This would make 2020 XL₅ more stable than the prototype L₄ Earth trojan 2010 TK7, which is potentially unstable on timescales of less than 2,000 years. Additional follow-up observations and precoveries confirmed 2020 XL₅'s trojan nature, and showed that it will leave trojan orbit at least 4,000 years into the future. Numerical simulations indicate that 2020 XL₅ was likely captured into the L₄ Langrangian point since the 15th century.

2020 XL₅'s high orbital eccentricity results in wide, tadpole-shaped oscillation paths in a corotating reference frame with Earth and its Lagrangian points. Although the asteroid crosses Venus's orbit with a minimum orbit intersection distance (MOID) of 0.0273 AU (4.1 million km; 2.5 million mi), perturbations by the planet are currently negligible since its nominal orbit brings it either too high or too low from the plane of Venus's orbit. Venus's influence on 2020 XL₅'s orbit will become greater over time as their longitudes of the ascending node precess over hundreds of years, lowering 2020 XL₅'s Venus MOID and eventually destabilizing its trojan orbit by sending it to Earth's L₃ point in several thousand years.

Physical characteristics

Photometric measurements of optical observations from 2020 to 2021 show that 2020 XL₅ exhibits a color resembling that of carbonaceous C-type asteroids. Assuming that 2020 XL₅'s phase curve behaves similarly to those of C-type asteroids, the absolute magnitude (H) of the asteroid is 18.6, which corresponds to a mean diameter about 1.18 km (0.73 mi) for a typical C-type asteroid's geometric albedo of 0.06. This makes 2020 XL₅ the largest Earth trojan asteroid known to date, being up to three times as large as the 0.3 km (0.19 mi)-sized 2010 TK₇.

Because 2020 XL₅ is only visible at low altitudes in the sky during twilight, atmospheric distortions and scattered light from the Sun hinder accurate photometry of the asteroid's light curve, thus information about its rotation could not be determined.

Exploration

Due to 2020 XL₅'s high orbital inclination, a rendezvous mission to the asteroid from low Earth orbit (LEO) would require a minimum total delta-v of 10.3 km/s (6.4 mi/s)—too high to be considered an ideal target for a low-energy trajectory. On the other hand, a flyby trajectory to 2020 XL₅ from LEO could be more feasible with a minimum total delta-v of 3.3 km/s (2.1 mi/s).

See also

• Co-orbital configuration
• Claimed moons of Earth
• Horseshoe orbit
• Quasi-satellite

External links

• Data from NSF's NOIRLab Show Earth Trojan Asteroid Is the Largest Found, NOIRLab, 1 February 2022
• Second Earth Trojan Discovered, Jeff Hecht, Sky & Telescope, 4 February 2021
• (614689) 2020 XL5 at NeoDyS-2, Near Earth Objects—Dynamic Site
  • Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
• (614689) 2020 XL5 at ESA–space situational awareness
  • Ephemerides · Observations · Orbit · Physical Properties · Summary
• (614689) 2020 XL5 at the JPL Small-Body Database
  • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters