Showing posts with label Moon. Show all posts
Showing posts with label Moon. Show all posts

Tuesday, October 15, 2013

moon's orbit is gradually enlarging

I've read that the moon's (the Earth's that is) orbit is gradually enlarging, i.e. the moon is gradually moving away from Earth. The rate at which this is ocurring, I read, was about 2 inches per year. I know that the moon's orbit is an ellipse and that this figure must be an average rate. 1. Is it true that the moon is moving away from Earth?, and 2) if so what is causing the moon to move away from the Earth? I know it is the Earth's gravitational attraction that holds the moon in orbit. If the Earth's mass remains constant the gravitational attraction must remain the same. I also read that the Earth gains more mass than it losses due to the bombardment of space debris (asteroids and what not) and since the Earth is bigger than the moon it must be gaining mass more rapidly than the moon therefore Earth's gravitational influence to hold the moon in orbit must be increasing thereby 'gluing' the two bodies more tightly together. Please explain.

It's not a question of mass, but of energy! The tidal force exerted by the Moon on the Earth causes the oceans to bulge. The Earth rotates about its axis faster than the Moon revolves around the Earth, and this rapid rotation carries the tidal bulge of the oceans forward of the Moon in its orbit. So the tidal bulge on the Earth is always slightly ahead of the Moon's own position. This bulge is continuously tugging the Moon forward, increasing the Moon's total energy. Imagine a cowboy's lasso. As the cowboy spins the lasso faster and faster (increasing its total energy), the loop gets wider. The same thing essentially happens to the Moon. The tugging of the Earth's bulge lifts it into a wider orbit around the Earth. The cowboy has to put some energy into the lasso to make the loop wider. In the Moon's case, the energy comes from the Earth's rotation. Friction between the oceans and the Earth's surface is slowing the Earth's rotation by 0.002 seconds every 100 years. The Earth's rotation will continue to slow, losing energy, until it's rotating so that a solar day equals a lunar month. The Earth's tidal bulge will point directly at the Moon, and the Moon will stop spiraling away from the Earth. The Earth will then keep its same side facing the Moon, just as the Moon presently keeps the same side facing the Earth. This has already happened to Pluto and its Moon, Charon, and is very common in the solar system.


Submitted by Peter (age 43, New Jersey, USA)
(May 29, 1998)

Saturday, October 12, 2013

Moon



---------------------------------------------------------
Taken from: Wikipedia
---------------------------------------------------------


Designations
Adjective lunar, selenic
Orbital characteristics
Perigee 363,295 km
(0.0024 AU)
Apogee 405,503 km
(0.0027 AU)
Semi-major axis 384,399 km
(0.00257 AU)[1]
Eccentricity 0.0549[1]
Orbital period 27.321582 d (27 d 7 h 43.1 min[1])
Synodic period 29.530589 d (29 d 12 h 44 min 2.9 s)
Average orbital speed 1.022 km/s
Inclination 5.145° to the ecliptic[2] (between 18.29° and 28.58° to Earth's equator)[1]
Longitude of ascending node regressing by one revolution in 18.6 years
Argument of perigee progressing by one revolution in 8.85 years
Satellite of Earth
Physical characteristics
Mean radius 1,737.10 km  (0.273 Earths)[1][3]
Equatorial radius 1,738.14 km (0.273 Earths)[3]
Polar radius 1,735.97 km  (0.273 Earths)[3]
Flattening 0.00125
Circumference 10,921 km (equatorial)
Surface area 3.793 × 107 km2  (0.074 Earths)
Volume 2.1958 × 1010 km3  (0.020 Earths)
Mass 7.3477 × 1022 kg  (0.012300 Earths[1])
Mean density 3.3464 g/cm3[1]
Equatorial surface gravity 1.622 m/s2 (0.165 4 g)
Escape velocity 2.38 km/s
Sidereal rotation period 27.321582 d (synchronous)
Equatorial rotation velocity 4.627 m/s
Axial tilt 1.5424° (to ecliptic)
6.687° (to orbit plane)[2]
Albedo 0.136[4]
Surface temp. min mean max
equator 100 K 220 K 390 K
85°N[5] 70 K 130 K 230 K
Apparent magnitude −2.5 to −12.9[a]
−12.74 (mean full moon)[3]
Angular diameter 29.3 to 34.1 arcminutes[3][b]
Atmosphere[6]
Surface pressure 10−7 Pa (day)
10−10 Pa (night)[c]
Composition Ar, He, Na, K, H, Rn