Existence of Earth Trojan Asteroid Confirmed – Could Become “Ideal Bases” for Advanced Exploration of the Solar System

Data from NSF’s NOIRLab Show Earth Trojan Asteroid Is the Largest Found

The SOAR Telescope, part of NOIRLab’s Cerro Tololo Inter-American Observatory, has helped astronomers refine the size and orbit of the largest known Earth Trojan companion.

By scanning the sky very close to the horizon at sunrise, the SOAR Telescope in Chile, part of Cerro-Tololo Inter-American Observatory, a Program of NSF’s NOIRLab, has helped astronomers confirm the existence of only the second-known Earth Trojan asteroid and reveals that it is over a kilometer wide — about three times larger than the first.

Astronomers have confirmed the existence of the second known Earth Trojan asteroid and found that it is much bigger than the first. An Earth Trojan is an asteroid that follows the same path around the Sun as Earth does, either ahead of or behind Earth in its orbit. Called 2020 XL5 the asteroid was discovered by the Pan-STARRS1 survey telescope in 2020, but astronomers were not sure then whether it was an Earth Trojan. The SOAR Telescope operated by NOIRLab in Chile helped confirm that it is an Earth Trojan and found that it is over a kilometer across — almost three times bigger than the other Earth Trojan known.

Using the 4.1-meter SOAR (Southern Astrophysical Research) Telescope on Cerro Pachón in Chile, astronomers led by Toni Santana-Ros of the University of Alicante and the Institute of Cosmos Sciences of the University of Barcelona observed the recently discovered asteroid 2020 XL₅ to constrain its orbit and size. Their results confirm that 2020 XL₅ is an Earth Trojan — an asteroid companion to Earth that orbits the Sun along the same path as our planet does — and that it is the largest one yet found.

“Trojans are objects sharing an orbit with a planet, clustered around one of two special gravitationally balanced areas along the orbit of the planet known as Lagrange points,”^[1] says Cesar Briceño of NSF’s NOIRLab, who is one of the authors of a paper published today in Nature Communications reporting the results, and who helped make the observations with the SOAR Telescope at Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab, in March 2021.

Several planets in the Solar System are known to have Trojan asteroids, but 2020 XL₅ is only the second known Trojan asteroid found near Earth.^[2]

Observations of 2020 XL₅ were also made with the 4.3-meter Lowell Discovery Telescope at Lowell Observatory in Arizona and by the European Space Agency’s 1-meter Optical Ground Station in Tenerife in the Canary Islands.

Discovered on December 12, 2020, by the Pan-STARRS1 survey telescope in Hawai‘i, 2020 XL₅ is much larger than the first Earth Trojan discovered, called 2010 TK₇. The researchers found that 2020 XL₅ is about 1.2 kilometers (0.73 miles) in diameter, about three times as wide as the first (2010 TK₇ is estimated to be less than 400 meters or yards across).

When 2020 XL₅ was discovered, its orbit around the Sun was not known well enough to say whether it was merely a near-Earth asteroid crossing our orbit, or whether it was a true Trojan. SOAR’s measurements were so accurate that Santana-Ros’s team was then able to go back and search for 2020 XL₅ in archival images from 2012 to 2019 taken as part of the Dark Energy Survey using the Dark Energy Camera (DECam) on the Víctor M. Blanco 4-meter Telescope located at CTIO in Chile. With almost 10 years of data on hand, the team was able to vastly improve our understanding of the asteroid’s orbit.

Although other studies have supported the Trojan asteroid’s identification,^[3] the new results make that determination far more robust and provide estimates of the size of 2020 XL₅ and what type of asteroid it is.

“SOAR’s data allowed us to make a first photometric analysis of the object, revealing that 2020 XL₅ is likely a C-type asteroid, with a size larger than one kilometer,” says Santana-Ros. A C-type asteroid is dark, contains a lot of carbon, and is the most common type of asteroid in the Solar System.

The findings also showed that 2020 XL₅ will not remain a Trojan asteroid forever. It will remain stable in its position for at least another 4000 years, but eventually it will be gravitationally perturbed and escape to wander through space.

2020 XL₅ and 2010 TK₇ may not be alone — there could be many more Earth Trojans that have so far gone undetected as they appear close to the Sun in the sky. This means that searches for, and observations of, Earth Trojans must be performed close to sunrise or sunset, with the telescope pointing near the horizon, through the thickest part of the atmosphere, which results in poor seeing conditions. SOAR was able to point down to 16 degrees above the horizon, while many 4-meter (and larger) telescopes are not able to aim that low.^[4].

“These were very challenging observations, requiring the telescope to track correctly at its lowest elevation limit, as the object was very low on the western horizon at dawn,” says Briceño.

Nevertheless, the prize of discovering Earth Trojans is worth the effort of finding them. Because they are made of primitive material dating back to the birth of the Solar System and could represent some of the building blocks that formed our planet, they are attractive targets for future space missions.

“If we are able to discover more Earth Trojans, and if some of them can have orbits with lower inclinations, they might become cheaper to reach than our Moon,” says Briceño. “So they might become ideal bases for an advanced exploration of the Solar System, or they could even be a source of resources.”

Notes

1. Lagrange points are gravitationally balanced regions around two massive bodies, such as the Sun and a planet. The Earth-Sun system has five Lagrange points: L1 is between Earth and the Sun; L2 is on the opposite side of Earth from the Sun; L3 is on the opposite side of the Sun from Earth; and L4 and L5 are along Earth’s orbit, one 60 degrees ahead of our planet along its orbit and the other 60 degrees behind it. (The image in the middle of this article illustrates their positions.) Trojan asteroids are found at L4 and L5. The two Earth Trojans found so far are at L4.
2. Jupiter has over 5000 known Trojan asteroids, and a ” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]”>NASA spacecraft called Lucy has recently launched on a mission to explore them. ” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]”>Venus, ” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]”>Mars, ” data-gt-translate-attributes=”[{“attribute”:”data-cmtooltip”, “format”:”html”}]”>Uranus, and Neptune are also known to have Trojan asteroids.
3. Man-To Hui (Macau University of Science and Technology) and collaborators published observations in the Astrophysical Journal Letters in December 2021 supporting the Trojan nature of 2020 XL₅.
4. These kinds of observations low in the sky are also the ones that will be most affected by the increasing number of satellite constellations.

More information

This research is presented in a paper titled “Orbital stability analysis and photometric characterization of the second Earth Trojan asteroid 2020 XL₅” published on 1 February 2022 in Nature Communications.

Reference: “Orbital stability analysis and photometric characterization of the second Earth Trojan asteroid 2020 XL₅” by T. Santana-Ros, M. Micheli, L. Faggioli, R. Cennamo, M. Devogèle, A. Alvarez-Candal, D. Oszkiewicz, O. Ramírez, P.-Y. Liu, P. G. Benavidez, A. Campo Bagatin, E. J. Christensen, R. J. Wainscoat, R. Weryk, L. Fraga, C. Briceño and L. Conversi, 1 February 2022, Nature Communications.
DOI: 10.1038/s41467-022-27988-4

The team is composed of T. Santana-Ros (Departamento de Fisica, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante; Institut de Ciències del Cosmos, Universitat de Barcelona), M. Micheli (ESA NEO Coordination Centre), L. Faggioli (ESA NEO Coordination Centre), R. Cennamo (ESA NEO Coordination Centre), M. Devogèle (Arecibo Observatory; University of Central Florida), A. Alvarez-Candal (Instituto de Astrofísica de Andalucía, CSIC; Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante; Observatório Nacional / MCTIC), D. Oszkiewicz (Faculty of Physics, Astronomical Observatory Institute), O. Ramírez (Solenix Deutschland), P.-Y. Liu (Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante), P.G. Benavidez (Departamento de Fisica, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante; Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante), A. Campo Bagatin (Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante; Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante), E.J. Christensen (Lunar and Planetary Laboratory, University of Arizona,), R. J. Wainscoat (Institute for Astronomy, University of Hawaii), R. Weryk (Department of Physics and Astronomy, University of Western Ontario), L. Fraga (Laboratório Nacional de Astrofísica LNA/MCTI), C. Briceño (Cerro Tololo Inter-American Observatory/NSF’s NOIRLab), and L. Conversi (ESA NEO Coordination Centre; ESA ESRIN).