Question: Scientists know that there must be more mass than what is visible in galaxies as
they manage to hold themselves together despite not being enough ordinary
matter, so they call it dark matter as it doesn't emit anything but is
observable through its gravity. Then if this dark matter can generate gravity
similar to ordinary matter then can it not interact with itself and make dark
matter clumps that are gravitationally detectable. Like a dark matter planet? If
this was true i imagine a dark matter planet would be detectable as it would
skew the orbits of ordinary matter planets? - Puzzled
Answer:
The conception of dark matter planets or solar systems for that matter is
dependent on how well we can distinguish exotic forms from ordinary forms. In
the latter case one might reference Fritz Zwicky's measurements of galaxy
clusters which highlighted a ‘missing mass’. He found that the mass needed to
bind a cluster of galaxies together gravitationally was at least ten times the
apparent mass visible. Around the same time there were observations of stellar
motions in the galactic plane by Dutch astronomer Jan Oort. He found there had
to be at least three times the mass visibly presenting in order for stars not to
escape the galaxy and fly off into space.
What exactly constituted
this 'missing mass'.? The short answer is we don't know but there a number of
candidates. By the late 1970s (with Cygnus X-1), astronomers realized there were
other forms of dark matter. Among the most discussed candidates were black
holes, marking the end stage of evolution for very massive stars. In the black
hole, the gravity is so strong that no light escapes and the mass typically is
much greater than that of the Sun.
Currently, we are aware of a super
black hole at the center of our galaxy with 9.7 billion times the mass of the
Sun. Can such an entity form planets? Hardly! It would more likely 'devour'
them.
Dark matter generally occurs in either baryonic or non-baryonic
forms, depending on whether the matter reacts with radiation or not. If it
doesn’t, it’s non-baryonic. Baryons include protons and neutrons, while
non-baryons include electrons and neutrinos.
Non-baryonic dark matter
further breaks down into cold dark matter and hot dark matter. The terms hot and
cold are not so much indicative of current temperatures, as the phase of the
early universe at which the particular dark matter ‘decoupled’ from the hot
radiation background. An early decoupling implies a higher ambient background
radiation temperature of the primeval cosmos. A later decoupling correlates to a
cooler temperature. Perhaps the most widely studied candidate of hot dark matter
is the neutrino.
By contrast, cold dark matter candidates tend to have
larger mass and amongst the most likely suspects are: gravitinos, magnetic
monopoles, and primordial black holes. However, there are a couple of exceptions
to this, which include: WIMPs and Axions.
How any of these entities could
leave specific gravity signatures that distinguish any one from their dark
counterparts is a matter of continued inquiry. Until such signatures are
identified and clarified there is little chance of even remotely confirming on
the existence of "dark matter planets". Especially if it is proposed that such a planet could orbit an ordinary matter (e.g. hot plasma) star.
It is certainly plausible that a dark matter object (like a small
black hole) could "skew the orbit" of an ordinary matter planet - or
star. But that a dark matter planet could exist within the confines of an ordinary matter solar system is another matter. And if such a solar system was entirely of dark matter, how would one detect it at all?
Your conjecture of dark matter clumps spinning off from a much larger dark matter mass (e.g. proto- star) evokes a takeoff on the nebular hypothesis of origin for our own solar system. The problem is that while such an entity (dark matter proto-planet) might be possible, there is no evidence whatsoever it exists. For example, all of the hundreds of exoplanets found thus far have all been ordinary matter objects - no 'dark matter'.
This is not to say such planets will never be found, but rather the investment of time, technology an resources may be much more than current cost-benefit analyses allow.
First, a bit of background: thanks to astronomer Edwin Hubble cosmology was put on a more secure observational footing on the basis of his "Hubble law". It is encapsulated by the graph shown below:

This relation between distance D to an extra-galactic object e.g. quasar, galaxy cluster) and its recessional velocity (v), has since come to be known as Hubble's law and is expressed:
v = cz = HD
where H is known as the Hubble constant, c is the speed of light and z is the red shift.
This quantity z measures the extent to which spectral lines, say L1 and L2, are shifted to the red (longer wavelengths) compared to the normal spectrum, say of an element like hydrogen. The greater this shift the higher the velocity of recession.
The image below illustrates this for two extragalactic objects:

In fact 'H' is more technically the Hubble "scale factor". The REAL Hubble constant (H o ) is the scale factor (a) divided by the distance in megaparsecs MPC (km) where 1 parsec = 3.26 light years.
If then currently MPC (km) = 3.08 x 10 19 km/ Mpc then:
H o = a / MPC(km) = 2.26 x 10 -18 s -1
Then the age of the cosmos can be obtained from: t o = 1 / H o =
(1 / 2.26 x 10 -18 s -1 ) = 4.4 x 10 17 s = 1.3 x 10 10 yrs. or 13 billion years in age
The scale factor a, called the "Hubble constant", is currently a » 70 km/ sec/Mpc. But as I reported last summer, e.g.
http://brane-space.blogspot.com/2016/06/arriving-at-hubble-constant.html
has since been refined to a = 72.8 km/ sec/Mpc.
Clearly then what we call the Hubble constant depends on the accuracy of a, and this in turn depends on the latest techniques to attain more exact values. As I noted in the preceding link the newer, more exact value has been based on refining the universe’s current expansion rate to unprecedented accuracy, reducing the uncertainty to only 2.4 percent.
However, an uncertainty of even just 2.4 percent means we cannot be talking about a real physical constant, but only an approximate factor that determines the proportionality value H in the Hubble law. This is important to process before continuing. My point is that the "discrepancy" with the standard model is a separate issue, because the standard model itself is still under scrutiny, although it's gained much more traction with the discovery of the Higgs boson.
This elicits the question of whether this small "mismatch" (Overbye's term) is truly an indicator of how well we know the cosmos. According to Wendy Freedman of the University of Chicago, who has spent most of her career charting the size and growth of the universe:
“If it is real, we will learn new physics,”
Perhaps. But I don't think the 'new physics' will enter until we also are able to incorporate the role of dark energy, which has been identified as the primary agent responsible for the accelerated expansion. Relevant to this we invoke what can be called a cosmological "equation of state" (think of something like the equation of state for an ideal gas, e.g. P = nkT) for the vacuum energy presumed to underlie most theories of dark energy . This is:
w = (Pressure/ energy density) = -1
One advantage is that this equation of state is consistent with Einstein's general theory of relativity - which one could say approaches the status of a 'basic law of physics'.
