High-Level Project Summary
This Presentation was done by the Team " MASTER MIND ". We illustrate the diversity Lucy Mission to the Trojan Asteroids that will explored by our Art work.These Asteroids ( Trojan ) will survey eight Asteroids in Six independent orbits around the Sun to help resolve the past of the Solar System .Trojans, are a large group of asteroids that share the planet Jupiter's orbit around the Sun. Relative to Jupiter, each Trojan librates around one of Jupiter's stable Lagrange points: either L4, existing 60° ahead of the planet in its orbit, or L5, 60° behind.The total number of Jupiter trojans larger than 1 km in diameter is believed to be about 1 million, approximately equal to the number of
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Detailed Project Description
This Presentation was done by the Team " MASTER MIND ". We illustrate the diversity Lucy Mission to the Trojan Asteroids that will explored by our Art work.
These Asteroids ( Trojan ) will survey eight Asteroids in Six independent orbits around the Sun to help resolve the past of the Solar System .
Trojans, are a large group of asteroids that share the planet Jupiter's orbit around the Sun. Relative to Jupiter, each Trojan librates around one of Jupiter's stable Lagrange points: either L4, existing 60° ahead of the planet in its orbit, or L5, 60° behind.
The total number of Jupiter trojans larger than 1 km in diameter is believed to be about 1 million, approximately equal to the number of asteroids larger than 1 km in the asteroid belt.
As of 2004, many Jupiter trojans showed to observational instruments as dark bodies with reddish, featureless spectra.
Jupiter trojans do not maintain a fixed separation from Jupiter. They slowly librate around their respective equilibrium points, periodically moving closer to Jupiter or farther from it.
Jupiter trojans generally follow paths called tadpole orbits.
Jupiter trojans have orbits with radii between 5.05 and 5.35 AU (the mean semi-major axis is 5.2 ± 0.15 AU), and are distributed throughout elongated, curved regions around the two Lagrangian points;each swarm stretches for about 26° along the orbit of Jupiter, amounting to a total distance of about 2.5 AU. The width of the swarms approximately equals two Hill's radii, which in the case of Jupiter amounts to about 0.6 AU.
Many of Jupiter trojans have large orbital inclinations relative to Jupiter's orbital plane—up to 40°.
Space Agency Data
This Presentation was done by the Team " MASTER MIND ". We illustrate the diversity Lucy Mission to the Trojan Asteroids that will explored by our Art work.
These Asteroids ( Trojan ) will survey eight Asteroids in Six independent orbits around the Sun to help resolve the past of the Solar System .
Trojans, are a large group of asteroids that share the planet Jupiter's orbit around the Sun. Relative to Jupiter, each Trojan librates around one of Jupiter's stable Lagrange points: either L4, existing 60° ahead of the planet in its orbit, or L5, 60° behind.
The total number of Jupiter trojans larger than 1 km in diameter is believed to be about 1 million, approximately equal to the number of asteroids larger than 1 km in the asteroid belt.
As of 2004, many Jupiter trojans showed to observational instruments as dark bodies with reddish, featureless spectra.
Jupiter trojans do not maintain a fixed separation from Jupiter. They slowly librate around their respective equilibrium points, periodically moving closer to Jupiter or farther from it.
Jupiter trojans generally follow paths called tadpole orbits.
Jupiter trojans have orbits with radii between 5.05 and 5.35 AU (the mean semi-major axis is 5.2 ± 0.15 AU), and are distributed throughout elongated, curved regions around the two Lagrangian points;each swarm stretches for about 26° along the orbit of Jupiter, amounting to a total distance of about 2.5 AU. The width of the swarms approximately equals two Hill's radii, which in the case of Jupiter amounts to about 0.6 AU.
Many of Jupiter trojans have large orbital inclinations relative to Jupiter's orbital plane—up to 40°
Hackathon Journey
Theme : I'd get a chance to learn more about " TROJAN SUPERNOVA " . Wonderful Opportunity to learn and study about our Space.
References
Yosida,F. Nakamura(2005) Size distribution of faint L4 Trojan aateroids
Trojan Minor Planets
Tags
art
Global Judging
This project has been submitted for consideration during the Judging process.