Dark Matter: How Do We Know It's Not Just Invisible Planets?

In summary, astronomers often locate planets orbiting other stars by detecting the "wobble" of a star. They can't actually see the planet right? Isn't it true that dark matter is also detected by it's gravitational influence on nearby objects? Maybe this is a dumb question, but how do we know that the dark matter isn't just stuff like planets that we can't see because stars are in the way, or are too bright?Look at it this way. In our solar system, planets and such only make up about 1/10 of 1% of the mass. The rest is the Sun. Assuming that dark matter is made up of particles that we currently don't understand, we should expect there to be about
  • #1
AdkinsJr
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I understand that astronomers often locate planets orbiting other stars. They do this by detecting the "wobble" of a star. They can't actually see the planet right? Isn't it true that dark matter is also detected by it's gravitational influence on nearby objects? Maybe this is a dumb question, but how do we know that the dark matter isn't just stuff like planets that we can't see because stars are in the way, or are too bright?
 
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  • #2
Look at it this way. In our solar system, planets and such only make up about 1/10 of 1% of the mass. The rest is the Sun.

There should be 5 times as much Dark matter as regular matter to explain the observations. That's the equivalent of our Solar system having 5000 times as much matter than it does now in the way of planets and such.

That much extra normal matter should be noticeable even if just by the dimming effect it would have on the light we see from the stars.
 
  • #3
I think there is more to AdkinsJr question than what Janus responded to.

In principle Dark Matter (DM) could be in the form of planets or dim stars (e.g. brown dwarfs) or black holes. Because the average distance between these objects would be so large,you won't always see starlight dim (unless a DM object eclipses a star).

My guess is that people have ruled out brown dwarfs and planets as being DM for two possible reasons. First off, planetary and stellar formation theories don't allow for most of the matter in a galaxy to collapse into brown dwarfs and planets. Second, someone may have done a direct search for brown dwarves that showed there aren't enough to explain dark matter.

A much more respectable possibility is that massive compact objects (e.g. neutron star or black hole) comprise DM. Astronomers can search for these compact objects through microlensing effects. When a compact object passes in front of a star the compact object's gravity can act like a lens and magnify the stars light for us. So by keeping our eye (i.e. telescope) on a bunch of stars we can look for spikes in their brightness which could be these compact objects. This type of survey has been carried out and has ruled out DM being black holes with a mass of [itex] 10^{-8}M_{sun}[/itex] (according to the http://en.wikipedia.org/wiki/Massive_compact_halo_object" on this subject).

Thus, most astronomers think that DM is comprised of particles that lie outside our current understanding of particle physics.
 
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  • #4
One additional factor against dark matter being baryonic is the observed ratio (big bang origin) of H1, H2, He3, He4, Li6, Li7 is consistent with the known baryonic density in the universe. Dark matter, if baryonic, would increase the density by a factor of six, therefore not consistent with the ratios describe above.
 
  • #5
Mathman,

If dark matter were comprised of primordial black holes that were present before the time of big bang nucleosynthesis, this would not contradict the primordial elemental abundance results. Right?
 
  • #6
Most scientists seem to accept dark matter, but there are some skeptics. I have heard about an alternative to general relativity, called the "asymmetric theory of gravity," which does away with dark matter and results in dramatically different cosmological model.
However, if general relativity holds, and dark matter behaves accordingly, wouldn't dark matter bend light? Has this ever been detected?
 
  • #7
Yes, dark matter does bend light. In fact that is one of the primary ways we have detected it. This http://blogs.discovermagazine.com/cosmicvariance/2006/08/21/dark-matter-exists/" * provides the best explanation I have ever read that explains why general relativity + dark matter is far superior to modified general relativity.

*This links to a blog post by the Caltech cosmologist Sean Carroll. The post explains why the Bullet Cluster dramatically confirms Dark Matter and disproves modified gravity.
 
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Related to Dark Matter: How Do We Know It's Not Just Invisible Planets?

1. What is dark matter?

Dark matter is a type of matter that does not emit or interact with light, making it invisible to traditional telescopes and detectors. It is believed to make up about 85% of the total matter in the universe.

2. How do we know that dark matter is not just invisible planets?

Scientists have studied the motion of stars and galaxies in the universe and have found that their movements cannot be fully explained by the presence of visible matter, such as planets. Additionally, dark matter does not emit or interact with light, making it unlikely that it is composed of planets.

3. What evidence do we have for the existence of dark matter?

There is a significant amount of evidence for dark matter, including the observed gravitational effects on the rotation of galaxies, the bending of light in gravitational lensing, and the large-scale structure of the universe. Additionally, simulations of the universe's evolution also support the existence of dark matter.

4. Can we directly detect dark matter?

Currently, scientists have not been able to directly detect dark matter. However, there are ongoing experiments using various methods, such as underground detectors and particle accelerators, in an attempt to detect and study dark matter particles.

5. How does the study of dark matter contribute to our understanding of the universe?

Studying dark matter is crucial in understanding the formation and evolution of the universe. It helps explain the observed structures and movements of galaxies and provides insight into the nature of gravity and the fundamental laws of physics. It also plays a role in the search for new particles and potential alternative theories to the standard model of physics.

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