The Jupiter Trojans are two clusters of asteroids that orbit the sun about 60 degrees ahead, and 60 degrees behind, Jupiter. Those are the L4, L5 points and the two groups are called The Greek Camp and The Trojan Camp.
There are probably hundreds of millions of the things, approximately a million of which are greater than 1 km in diameter. Only about 7000 have been observed and described. Some of them are binaries or in even more complex systems.
They were first discovered some 100 years ago. The biggest of them is 624 Hektor, about 400 km long, situated at L4 (the so called Greek camp). I have no idea why “Hektor” is in the Greek camp. It has a satellite, about 100 km across.
617 Patroclus is also in the wrong camp, the Trojan camp. That’s the largest in that camp, and it also has a satellite.
The Jupiter Trojans are dark. Hektor for instance has an albedo of about 3%. That is, it reflects only 3% of light. They might be coated in tholins, a sticky organic goo.
Anyway, there is a mission called Lucy which is going to visit both camps. It will be the first mission to the Jupiter Trojans.
Lucy will launch in 2021, at arrive at L4 in 2027 where it will perform flyby encounters with four of these asteroids. It will then return to the vicinity of Earth, receive a little gravity kick to speed it towards L5, where it will run a flyby of 617 Patroclus in 2033.
So that’s nice.
There are only three pieces of science hardware:
high-res visible-light imager, based on the LORRI imager on New Horizons
colour imager and infrared spectrometer, based on the Ralph imager on New Horizons
thermal infrared spectrometer, based on that used by the OSIRIS-REX mission
