Expansion of space: Earth - Moon

Click For Summary
SUMMARY

The discussion centers on the calculation of the Moon's recession from Earth using Hubble's law, which is deemed inappropriate for local astronomical distances. The Moon is indeed receding at approximately 38 mm per year due to tidal friction, while gravitational forces dominate over cosmic expansion at short distances. The "Big Rip" scenario, suggesting that cosmic expansion could eventually tear apart atoms, is largely speculative and not supported by evidence. The general-relativistic effects on local systems, such as the Earth's orbit, are minimal, comparable to the size of an atomic nucleus.

PREREQUISITES
  • Understanding of Hubble's law and its application limits
  • Basic knowledge of gravitational forces and tidal friction
  • Familiarity with general relativity concepts
  • Awareness of astronomical measurement techniques, such as laser ranging
NEXT STEPS
  • Research the implications of Hubble's law on cosmic scales
  • Explore tidal friction effects on celestial bodies
  • Study general relativity and its impact on local gravitational systems
  • Investigate the "Big Rip" hypothesis and current scientific consensus
USEFUL FOR

Astronomers, astrophysicists, and students of cosmology interested in the dynamics of celestial bodies and the effects of cosmic expansion on local gravitational systems.

Michel_vdg
Messages
107
Reaction score
1
Hi,

I made a (rough) calculation of how far the Moon would be moving away from Earth according to Hubble's law = 72.6 (km/s)/Mpc

--

1 megaParsec = 3.08 × 1022 m ≈ 4 × 1022 m

Distance between Moon and Earth ≈ 4 x 108 m

Expansion rate ≈ 7.2 104 (m/s)/4 × 1022 m = 7.2 (m/s)/4 × 1018 m

Thus expansion for Earth - Moon ≈ 7.2 x 10-10 m/s

--

Is this calculation correct? If so, than that it would be about one picometer per second, or is Earth's gravity force simply keeping the Moon in it place?

Thanks,

m.
 
Astronomy news on Phys.org
Hubble's law applies to intergalactic distances. It does not apply to stars within our own galaxy, much less distance between planets in a single solar system not distance between a planet and it moons.
 
ok, thanks.

Than how can we calculate the expansion of the Universe on a local scale, or is there no expansion locally because gravity keeps it all together?
 
Correct. Gravitational bound objects are essentially immune to the effects of expansion. The force of expansion is overwhelmed by gravity over 'short' distances. By 'short' distances we are talking the level of galactic clusters.
 
FWIW, the Moon *is* receding, but due tidal friction, currently ~ 38 mm / yr.
http://en.wikipedia.org/wiki/Orbit_of_the_Moon

IIRC, this is measured by laser ranging using the retro-reflector panels positioned by Apollo astronauts or mounted on Russian rover.
 
Why do I keep hearing that the expansion of space will eventually rip even atoms apart, if it's too weak to affect anything below intergalactic distances?
 
Lsos said:
Why do I keep hearing that the expansion of space will eventually rip even atoms apart, if it's too weak to affect anything below intergalactic distances?

The so-called "Big Rip" scenario that you describe is hypothetical and not widely believed to be likely. There is no evidence for it, just speculation.

I SEEM to recall (sorry I can't give a link, so this is hearsay) that it has even been disproven, but that may be a stretch. Call it unlikely.
 
The influence of the cosmological expansion on local systems
F. I. Cooperstock, V. Faraoni, D. N. Vollick
http://arxiv.org/abs/astro-ph/9803097v1

They calculate this kind of thing. The effect is extremely small. The predicted general-relativistic effect on the radius of the Earth's orbit since the time of the dinosaurs is calculated to be about as big as the diameter of an atomic nucleus.
 
phinds said:
The so-called "Big Rip" scenario that you describe is hypothetical and not widely believed to be likely. There is no evidence for it, just speculation.

I SEEM to recall (sorry I can't give a link, so this is hearsay) that it has even been disproven, but that may be a stretch. Call it unlikely.

Here's an interesting blogpost by a theoretical astrophysicist on this topic, and somewhere on it there is also a link to that paper:

http://astrokatie.blogspot.co.uk/2012/07/you-dont-have-to-blow-up-universe-to-be.html
 
  • #10
bcrowell said:
The influence of the cosmological expansion on local systems
F. I. Cooperstock, V. Faraoni, D. N. Vollick
http://arxiv.org/abs/astro-ph/9803097v1

They calculate this kind of thing. The effect is extremely small. The predicted general-relativistic effect on the radius of the Earth's orbit since the time of the dinosaurs is calculated to be about as big as the diameter of an atomic nucleus.

Thanks, this was the kind of information I was curious about.
 

Similar threads

  • · Replies 5 ·
Replies
5
Views
1K
  • · Replies 13 ·
Replies
13
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 14 ·
Replies
14
Views
8K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 13 ·
Replies
13
Views
2K