Saved Papers

Save papers so you can find them more easily...


Join Now

Get instant access to our database of over 100,000 papers.

Join Now!

Halley's Orbit


Join Now
Credit Card
Join Now
PayPal
 

The average period of Halley's orbit is 76 years but you cannot calculate the dates of its reappearances by simply subtracting multiples of 76 years from 1986. The gravitational pull of the major planets alters the orbital period from revolution to revolution. Nongravitational effects (such as the reaction from gasses boiled off during its passage near the Sun) also play an important, but smaller, role in altering the orbit. Between the years 239 BC and 1986 AD the orbital period has varied from 76.0 years (in 1986) to 79.3 years (in 451 and 1066). The closest perihelion passage to the time of Jesus are 11 BC and 66 AD; neither event took place in Jesus' lifetime. Its most famous appearance was in 1066 when it was seen at the Battle of Hastings, an event commemorated in the Bayeux Tapestry.
Comet Halley was visible in 1910 and again in 1986. Its next perihelion passage will be in early 2062.
Halley's orbit is retrograde and inclined 18 degrees to the ecliptic. And, like all......

Join Now or Login to view the rest of this paper.

Approximate Word Count: 366
Approximate Pages: 2 (260 words per double-spaced page)

Why should you join TermPapersMonthly?
- It's secure and completely anonymous.
- You get instant access to over 100,000 papers.
- Prompt and helpful customer support.

Credit Card
PayPal