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

Solar system details







Solar System





The Sun and planets of the Solar System. Sizes are to scale. Distances not to scale.









Distance from Sun
Radius
Orbital speed
Equatorial radius
Inclination to ecliptic
Polar radius
Mass
Sidereal rotation period
Sun
0
700,000 km(.0047 AU)






Mercury
0.4 AU







Venus
0.723 327 AU



3.394 58°



Earth
1 AU(150,000,000 km)







Mars
1.5 AU

24.077 km/s
3,396.2 ± 0.1 km

3,376.2 ± 0.1 km
6.4185×1023 kg
24.622 9 h
Jupiter
5.2 AU(780,000,000 km)
71,000 km(0.00047 AU)






Saturn
9.5 AU







Uranus
19.2







Neptune
30 AU(4.5×109 km)







Pluto












Earth to the Sun is 1 astronomical unit (150,000,000 km)



Age 4.568 billion years
Location Local Interstellar Cloud, Local Bubble, Orion–Cygnus Arm, Milky Way
System mass 1.0014 solar masses
Nearest star Proxima Centauri (4.22 ly), Alpha Centauri system (4.37 ly)
Nearest known planetary system Alpha Centauri system (4.37 ly)
Planetary system
Semi-major axis of outer planet (Neptune) 30.10 AU (4.503 billion km)
Distance to Kuiper cliff 50 AU
No. of stars 1
Sun
No. of planets 8
Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune
No. of known dwarf planets 5 (IAU)
Ceres, Pluto, Haumea, Makemake, Eris
hundreds of other possibilities[1]
No. of known natural satellites 421 (173 of planets[2] and 248 of minor planets[3])
No. of known minor planets 620,276 (as of 2013-07-23)[4]
No. of known comets 3,218 (as of 2013-07-23)[4]
No. of identified round satellites 19
Orbit about the Galactic Center
Inclination of invariable plane to the galactic plane 60.19° (ecliptic)
Distance to Galactic Center 27,000±1,000 ly
Orbital speed 220 km/s
Orbital period 225–250 Myr
Star-related properties
Spectral type G2V
Frost line ≈5 AU[5]
Distance to heliopause ≈120 AU
Hill sphere radius ≈1–2 ly




Neptune

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Taken from: Wikipedia
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Neptune Astronomical symbol for Neptune.
Neptune from Voyager 2
Neptune from Voyager 2 with Great Dark Spot at left and Small Dark Spot at lower right. White clouds are composed of methane ice; overall blue coloration is due at least in part to methane absorption of red light.
Discovery
Discovered by
Discovery date 23 September 1846[1]
Designations
Pronunciation Listeni/ˈnɛptjn/[2]
Adjective Neptunian
Orbital characteristics[7][a]
Epoch J2000
Aphelion 4,553,946,490 km
30.44125206 AU
Perihelion 4,452,940,833 km
29.76607095 AU
Semi-major axis 4,503,443,661 km
30.10366151 AU
Eccentricity 0.011214269
Orbital period 60,190.03[3] days
164.79 years
89,666 Neptune solar days[4]
Synodic period 367.49 days[5]
Average orbital speed 5.43 km/s[5]
Mean anomaly 267.767281°
Inclination 1.767975° to Ecliptic
6.43° to Sun’s equator
0.72° to Invariable plane[6]
Longitude of ascending node 131.794310°
Argument of perihelion 265.646853°
Satellites 14
Physical characteristics
Equatorial radius 24,764 ± 15 km[8][b]
3.883 Earths
Polar radius 24,341 ± 30 km[8][b]
3.829 Earths
Flattening 0.0171 ± 0.0013
Surface area 7.6183×109 km2[3][b]
14.98 Earths
Volume 6.254×1013 km3[5][b]
57.74 Earths
Mass 1.0243×1026 kg[5]
17.147 Earths
5.15×10−5 Suns
Mean density 1.638 g/cm3[5][b]
Equatorial surface gravity 11.15 m/s2[5][b]
1.14 g
Escape velocity 23.5 km/s[5][b]
Sidereal rotation period 0.6713 day[5]
16 h 6 min 36 s
Equatorial rotation velocity 2.68 km/s
9,660 km/h
Axial tilt 28.32°[5]
North pole right ascension 19h 57m 20s[8]
299.3°
North pole declination 42.950°[8]
Albedo 0.290 (bond)
0.41 (geom.)[5]
Surface temp. min mean max
1 bar level
72 K[5]
0.1 bar (10 kPa)
55 K[5]
Apparent magnitude 8.02 to 7.78[5][9]
Angular diameter 2.2–2.4[5][9]
Atmosphere[5]
Scale height 19.7 ± 0.6 km
Composition
80±3.2% hydrogen (H2)
19±3.2% helium (He)
1.5±0.5% methane (CH4)
~0.019% hydrogen deuteride (HD)
~0.00015% ethane (C2H6)
Ices:

Saturn


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Taken from: Wikipedia
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Saturn Astronomical symbol for Saturn
The planet Saturn
Saturn in natural color, photographed by Cassini, 2004
Designations
Pronunciation Listeni/ˈsætərn/[1]
Adjective Saturnian, Cronian
Orbital characteristics[5][a]
Epoch J2000.0
Aphelion 1,513,325,783 km (10.11595804 AU)
Perihelion 1,353,572,956 km (9.04807635 AU)
Semi-major axis 1,433,449,370 km (9.5820172 AU)
Eccentricity 0.055723219
Orbital period
Synodic period 378.09 days[3]
Average orbital speed 9.69 km/s[3]
Mean anomaly 320.346 750°
Inclination
Longitude of ascending node 113.642 811°
Argument of perihelion 336.013 862°
Satellites 62 with formal designations; innumerable additional moonlets.[3]
Physical characteristics
Equatorial radius
  • 60 268 ± 4 km[6][b]
  • 9.4492 Earths
Polar radius
  • 54 364 ± 10 km[6][b]
  • 8.5521 Earths
Flattening 0.097 96 ± 0.000 18
Surface area
  • 4.27×1010 km²[b][7]
  • 83.703 Earths
Volume
  • 8.2713×1014 km3[3][b]
  • 763.59 Earths
Mass
  • 5.6846×1026 kg[3]
  • 95.152 Earths
Mean density 0.687 g/cm3[3][b]
(less than water)
Equatorial surface gravity
Escape velocity 35.5 km/s[3][b]
Sidereal rotation period 10.57 hours[8]
(10 hr 34 min)
Equatorial rotation velocity
  • 9.87 km/s[b]
  • 35 500 km/h
Axial tilt 26.73°[3]
North pole right ascension
  • 2h 42m 21s
  • 40.589°[6]
North pole declination 83.537°[6]
Albedo
Surface temp. min mean max
1 bar level
134 K[3]
0.1 bar
84 K[3]
Apparent magnitude +1.47 to −0.24[9]
Angular diameter 14.5"–20.1"[3]
(excludes rings)
Atmosphere[3]
Scale height 59.5 km
Composition
~96% hydrogen (H2)
~3% helium (He)
~0.4% methane (CH4)
~0.01% ammonia (NH3)
~0.01% hydrogen deuteride (HD)
0.0007% ethane (C2H6)
Ices:

Venus

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Taken from: Wikipedia
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Venus The Venusian symbol, a circle with a small equal-armed cross beneath it
Venus in approximately true colour, a nearly uniform pale cream, although the image has been processed to bring out details.[1] The planet's disc is about three-quarters illuminated. Almost no variation or detail can be seen in the clouds.
Venus processed from two filters. The surface is obscured by a thick blanket of clouds.
Designations
Pronunciation Listeni/ˈvnəs/
Adjective Venusian or (rarely) Cytherean, Venerean
Orbital characteristics[2][4]
Epoch J2000
Aphelion
  • 108,939,000 km
  • 0.728 213 AU
Perihelion
  • 107,477,000 km
  • 0.718 440 AU
Semi-major axis
  • 108,208,000 km
  • 0.723 327 AU
Eccentricity 0.0067
Orbital period
Synodic period 583.92 days[2]
Average orbital speed 35.02 km/s
Mean anomaly 50.115°
Inclination
Longitude of ascending node 76.678°
Argument of perihelion 55.186°
Satellites None
Physical characteristics
Mean radius
  • 6,051.8 ± 1.0 km[5]
  • 0.949 9 Earths
Flattening 0[5]
Surface area
  • 4.60×108 km2
  • 0.902 Earths
Volume
  • 9.28×1011 km3
  • 0.866 Earths
Mass
  • 4.8676×1024 kg
  • 0.815 Earths
Mean density 5.243 g/cm3
Equatorial surface gravity
Escape velocity 10.36 km/s
Sidereal rotation period −243.018 5 day (Retrograde)
Equatorial rotation velocity 6.52 km/h (1.81 m/s)
Axial tilt 177.36°[2]
North pole right ascension
  • 18 h 11 min 2 s
  • 272.76°[6]
North pole declination 67.16°
Albedo
Surface temp. min mean max
Kelvin
737 K[2]
Celsius
464 °C
Apparent magnitude
  • brightest −4.9[8][9] (crescent)
  • −3.8[10] (full)
Angular diameter 9.7"–66.0"[2]
Atmosphere
Surface pressure 92 bar (9.2 MPa)
Composition