Expert Voices

Asteroid sharing Earth's orbit discovered — could it help future space missions?

A graphic shows where Earth's Trojan asteroid 2020 XL5 would appear in the skies if it were visible without equipment.
A graphic shows where Earth's Trojan asteroid 2020 XL5 would appear in the skies if it were visible without equipment. (Image credit: NOIRLab/NSF/AURA/J. da Silva)

This article was originally published at The Conversation. (opens in new tab) The publication contributed the article to Space.com's Expert Voices: Op-Ed & Insights.

David Rothery (opens in new tab), Professor of Planetary Geosciences, The Open University

Research has shown that the Earth trails an asteroid barely a kilometer across in its orbit about the sun — only the second such body to have ever been spotted. It goes round the sun on average two months ahead of the Earth, dancing around in front like an excited herald of our coming.

This object, known as 2020 XL5, was first spotted in December 2020 using Pan-STARRS telescopes (opens in new tab) on the summit of Haleakala on the Hawaiian island of Maui. But determination of its orbit required follow-up observations using the 4.1-metre SOAR (Southern Astrophysical Research) telescope (opens in new tab) in Chile.

Related: The greatest asteroid missions of all time!

Based on this data, a team led by planetary scientist Toni Santana-Ros (opens in new tab) of the University of Alicante in Spain has now announced (opens in new tab) that 2020 XL5 is trapped for at least the next several thousand years in an orbit about one of the sun-Earth "Lagrange points." These are where the gravitational forces of the Earth and the sun balance to create stable locations. It means the object keeps pace with the Earth as it goes round the sun.

Lagrange points exist around other planets too, they are equilibrium points for any objects with small mass under the influence of any two much more massive bodies. There are three such points on the sun-Earth line (L1, L2 and L3, see image below), first discovered mathematically by the Swiss mathematician Leonhard Euler. Spacecraft, such as James Webb Space Telescope (at L2) and DSCOVR (opens in new tab) (at L1), can be maintained there with only a small expenditure of fuel.

A diagram shows the five Earth-sun Lagrange points. (Image credit: NOIRLab/NSF/AURA/J. da Silva/M. Zamani (NSF's NOIRLab))

Two other points, L4 and L5, were discovered in 1772 by Euler's student Joseph-Louis Lagrange (opens in new tab). Here, a small-mass object making an equilateral triangle with sun and Earth is in a stable equilibrium. These points are 60 degrees ahead of and 60 degrees behind the Earth, and because 60 degrees (see image above) is one-sixth of the Earth's orbit this amounts to two months separation.

If a small-mass object is perturbed so as to move away from L4 or L5, the combined gravity of the sun and Earth draws it back — bending its path into a stable orbit around the Lagrange point that looks kidney bean shaped relative to Earth.

XL5, but no fireball

2020 XL5 is being called a Trojan companion to the Earth by analogy with Jupiter's Trojan asteroids. Jupiter shares its orbit with nearly ten thousand known asteroids, half of them ahead of Jupiter, and half behind. The first of those, discovered in 1906, was named Achilles after a central character at the siege of Troy (opens in new tab) in Homer's Iliad.

A convention developed to name each one after a hero from the same story. Only those trailing Jupiter (clustered at the sun-Jupiter L5 position) are given Trojan names, such as Hektor, whereas those ahead of Jupiter (at L4) are give Greek names, such as Achilles. Collectively, whether at L4 or L5 they are all referred to as Trojans.

Asteroid positions, with Jupiter’s Trojans in green. (Image credit: Mdf at English Wikipedia, Public domain, via Wikimedia Commons)

Small numbers of Trojan asteroids have now been discovered associated with Neptune (23), Uranus (1) and Mars (9). But 2020 XL5 is only the second Trojan companion of Earth to have been found. The first, 2010 TK7, was discovered in 2010 (opens in new tab). That's only about 300 meters across, so 2020 XL5 considerably outmasses it at about 1.2km across.

There are probably many more Earth Trojans, but they are hard to discover from Earth because they can only ever be seen fairly low in the pre-dawn sky if at L4 like both 2010 TK7 and 2020 XL5, or just after sunset if at L5 (where none have yet been found). Their orbits are not stable over millions of years, so they can't be remnants that have been there ever since Earth's formation but must have drifted into place later.

However, the SOAR observations were able to show that 2020 XL5 appears to be a carbon-rich asteroid (called C-type). So it is a sample of what the solar system was built from, and it would be instructive to study Earth's Trojan companions in more detail as examples of unaltered material.

But could we mine them or use them in other ways? Santana-Ros notes that 2020 XL5 has an orbit that bobs above and below Earth's orbital plane. This means that to maneuver a spacecraft into a rendezvous (to orbit or land on it) would require considerable velocity change. That would probably need too much fuel to be practical. The same applies to 2010 TK7.

However, the study points out that if other Earth Trojans are found in orbits that are less tilted, these might make handy bases as staging posts for exploration of the solar system. They'd be much easier to take off from than from the Earth or moon because their gravity is so slight. They could even be a source of resources that we could mine.

This article is republished from The Conversation (opens in new tab) under a Creative Commons license. Read the original article (opens in new tab).

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David Rothery
Professor of Planetary Geosciences, The Open University

David Rothery is a professor of planetary geosciences at the Open University in Milton Keyes, England, where he studies volcanic activity with remote sensing, as well as volcanology and geoscience on other planets. He earned a Ph.D. on the applications of remote sensing from Open University in 1982 and has been a professor of planetary geosciences since 2013. Prior to that he had served as a senior lecturer since 1994. David is the U.K. lead co-investigator on the Mercury Imaging X-ray Spectrometer aboard the European Space Agency's BepiColombo mission to Mercury and chairs ESA's Mercury Surface and Composition Working Group. He is the author of several books on space geosciences, including his landmark Planet Mercury: From Pale Pink Dot to Dynamic World (Springer-Praxis, 2014). You can see David's latest updates by following him on Twitter (opens in new tab).