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astronomy

J002E3

J002E3 is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand J002E3 rather than just read about it. In short: J002E3 is an object in space which is thought to be the S-IVB third stage of the Apollo 12 Saturn V rocket. It was discovered on September 3, 2002, by amateur astronomer Bill Yeung.

J002E3 — main illustration
J002E3 — illustration

Key takeaways

  • J002E3 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect J002E3 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of J002E3 from memory before moving on to harder problems.

Reference excerpt

J002E3 is an object in space which is thought to be the S-IVB third stage of the Apollo 12 Saturn V rocket. It was discovered on September 3, 2002, by amateur astronomer Bill Yeung. Initially thought to be an asteroid, it has since been tentatively identified as the third stage of Apollo 12 Saturn V based on spectrographic evidence consistent with the titanium dioxide in the paint used on the rockets. The stage was intended to be injected into a permanent heliocentric orbit in November 1969, but is now believed instead to have gone into an unstable high Earth orbit which left Earth's proximity in 1971 and again in June 2003, with an approximately 40-year cycle between heliocentric and geocentric orbit.

Discovery When it was first discovered, it was quickly found that the object was in an orbit around Earth. Astronomers were surprised at this, as the Moon is the only large object in orbit around the Earth, and anything else would have been ejected long ago due to perturbations with the Earth, the Moon and the Sun. Therefore, it probably entered into Earth orbit very recently, yet there was no recently launched spacecraft that matched the orbit of J002E3. One explanation could have been that it was a 30 meter-wide piece of rock, but University of Arizona astronomers found that spectral observations of the object indicated a strong correlation of absorption features with a combination of human-made materials including white paint, black paint, and aluminum, consistent with Saturn V rockets. Back-tracing its orbit showed that the object had been orbiting the Sun for 31 years and had last been in the vicinity of the Earth in 1971. This seemed to suggest that it was a part of the Apollo 14 mission, but NASA knew the whereabouts of all hardware used for that mission; the third stage, for instance, was deliberately crashed into the Moon for seismic studies. The most likely explanation appears to be the S-IVB third stage for Apollo 12. Photometric observations of J002E3 made in February 2003 from the Air Force Maui Optical and Supercomputing Site (AMOS) matched an S-IVB light curve model consisting of a diffuse cylinder tumbling with a period of 63.46 seconds and a precession of 79 ± 10°. NASA had originally planned to direct the S-IVB into a solar orbit, but an extra long burn of the ullage motors meant that venting the remaining propellant in the tank of the S-IVB did not give the rocket stage enough energy to escape the Earth–Moon system, and instead the stage ended up in a semi-stable orbit around the Earth after passing by the Moon on 18 November 1969. It is thought that J002E3 left Earth orbit in June 2003, and that it may return to orbit the Earth in the mid-2040s.

Potential impact with Earth or Moon The object's Earth orbital paths occasionally take it within the radius of the Moon's orbit, and could result in eventual entry into Earth's atmosphere, or collision with the Moon. The Apollo 12 empty S-IVB, Instrument Unit, and spacecraft adapter base, had a mass of about 14 tonnes; 15 short tons (30,000 lb). This is less than one-fifth of the 77.1-tonne; 85.0-short-ton (169,900 lb) mass of the Skylab space station, which was constructed from a similar S-IVB and fell out of orbit on 11 July 1979. Objects with a mass of about 10 tonnes (22,000 lb; 11 short tons) enter Earth's atmosphere approximately 10 times a year, one of which impacts the Earth's surface approximately once every 10 years. Ten essentially similar empty S-IVB stages from Apollo, Skylab and Apollo-Soyuz Test Project missions have re-entered the atmosphere from 1966 to 1975. In all cases (including the Skylab station), the objects burned in the atmosphere and broke into relatively small pieces, rather than striking the Earth as a single mass. On the other hand, these objects entered from low Earth orbit or a ballistic trajectory, with less energy than J002E3 might possibly have if it were to enter from solar orbit.

See also 6Q0B44E, space debris originally thought to be a meteoroid 2006 RH120, a meteoroid originally thought to be space debris 2007 VN84, an asteroid designation mistakenly given to the Rosetta spacecraft 3753 Cruithne 2020 SO Space debris

Notes

References

External links J002E3 Animations, CNEOS Mystery Object J002E3 Gallery, NASA Mystery Object Orbits Earth, NASA Astronomers Discover That Earth's Second Moon Wears Apollo Paint at the Wayback Machine (archived 20 August 2007), University of Arizona

Illustrations

J002E3 illustration
J002E3 illustration
J002E3: S-IVB stage of Apollo 17. The one used for Apollo 12 is of identical type.
S-IVB stage of Apollo 17. The one used for Apollo 12 is of identical type.

Worked examples

Example 1 — a first encounter with J002E3

Start with the simplest possible case. Write down what J002E3 claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to J002E3 before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about J002E3 ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of J002E3

In research
J002E3 appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses J002E3 in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
J002E3 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Apollo 12, Apollo program, Artificial objects mistaken for near-Earth objects, so understanding it makes those chapters shorter.
In everyday life
Look for J002E3 outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study J002E3 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what J002E3 means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain J002E3 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is J002E3 in simple terms?

J002E3 is an object in space which is thought to be the S-IVB third stage of the Apollo 12 Saturn V rocket. It was discovered on September 3, 2002, by amateur astronomer Bill Yeung.

Why does J002E3 matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study J002E3?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on J002E3.

Tags

  • Apollo 12
  • Apollo program
  • Artificial objects mistaken for near-Earth objects
  • Astronomical objects discovered in 2002
  • Claimed moons of Earth
  • Derelict satellites in heliocentric orbit
  • Individual rockets
  • Near-Earth objects in 2002
  • Space archaeology

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