To be clear: to an astrophysicist, "dark" means "does not interact with electromagnetic radiation except through the curvature of space-time by gravity". It only interacts with normal matter in that it affects gravity. It is otherwise completely transparent.
It does no mean "is not currently reflecting or producing visible light". Your closet does not contain dark matter when you close the door.
Your closet probably has the same concentration of dark matter in it as everywhere else on the surface of Earth. But that quantity is unmeasurable at our current technology level, because any signal we might get is completely obscured by all the noise from bright matter around here.
Dark matter is not matter that does not emit light. A rogue asteroid far from any star is a dark object, but it is not dark matter. If you aimed a radar beam at it, the signal would bounce off, and you could detect the reflected/absorbed/re-emitted signal when it gets back to you. If you somehow found an aggregation of dark matter, your radar beam would not bounce. It would pass right through, like a flashlight beam shining through a crystal ball. Your beam might refract slightly due to the gravity, but it would not reflect. It would be similar to aiming a neutrino beam at the regular asteroid. Most of the beam just passes straight through without interacting.
Not even black holes are dark matter (or if they ever were, they aren't any more), because they absorb light. If one eclipses a known light source, you can see the black spot, along with the lensing around the outside. They interact with light.
Why not just go back to calling it The Æther? Or mayhap a form of non-luminiferous aether, if I may be so bold?
https://en.wikipedia.org/wiki/Aether_theories
a space-filling substance or field, thought
to be necessary as a transmission medium for
the propagation of [...] gravitational forces.
You say tomato, I say Tomato. Aether. Why not?There's also apparently decent evidence, based on things like irregularities in the cosmic microwave background, that most dark matter isn't any form of baryonic matter.
The sun is 99.86% of the mass of our solar system and is quite average. [1]
Dark matter is ~27% of the mass of the observable universe. [2]
Are you claiming that exoplanets and asteroids represent 27% of the mass of the universe when a typical G-type star (not particularly massive, by any means) is almost 100% of the mass of our entire solar system?
I'm confused by your assertion - you either have some data I am lacking, have entirely made up your post, or are, yourself, confused.
[1] https://en.wikipedia.org/wiki/Sun [2] https://en.wikipedia.org/wiki/Dark_matter
I'll let someone else be more precise:
http://cdms.berkeley.edu/Education/DMpages/FAQ/question36.ht...
Meanwhile, their gravity is now well known to induce wobble on their parent stars, which are much more luminous, and probably outshines any exoplanet in the infrared.
This method works best for
young planets *that emit infrared
light* and are far from the glare
of the star.
In other words, if they are still swirling balls of liquid magma. So, NOT dark matter.Furthermore, are you aware that you yourself are emitting infrared light right at this moment and are presumably not a swirling ball of liquid magma?
are you aware that you yourself are emitting
infrared light right at this moment [...] ?
WHAAATTT???!!!1oneThe hell you say!
Come on, man. You and I both know that exoplanets are a recent discovery (1988 being the earliest verified potential candidate for the real thing), and thus hard to detect in the visible spectrum. No one is looking at them with an ordinary telescope, tuned into the visible spectrum.
Last time I checked, anything not emitting visible light is commonly referred to as "dark." But wait, let me just check with my specialized visible light emission instrument.
Gee, when I turn off this incandescant light bulb, it goes... dark! Hypothesis verified! Is it still hot? Why yes! Yes, it is still hot. But also dark. Weird!
But hey, while we're being pedantic nerds, I'll just take a moment to correct you, regarding your correction of me.
Most of the examples in the impeccably cited link are measured in multiples of Jupiter's mass, which, you know, pretty much means they're certainly gas giants, and damn near brown dwarf classification, lending to their thermal activity.
So, the heat would likely not be owing to lava or magma.
There's no proof of material at all, thus not matter, thus no such thing as dark matter. I'd willingly accept other names such as Dark Question Marks. Or maybe Dark Mathematical Terms Yet To Be Named.
Here's a good one: Dark Unobservable Numerically Challenged Entities.
Matter isn't matter unless collisions prove it's occupancy of space. That's pretty much why matter is considered anything at all. You can't gloss over a significant lack of collisions.
Asteroid belts are also dark matter. If a remote star has an asteroid belt, it wouldn't be easily detectable, since it probably wouldn't elicit the kepler-style wobbles and flickers, or if it did, perhaps less obvious/detectable events.
Based on this, the astronomical fad terminology is flawed, since it seems to claim that only stars matter because only stars are matter (and the luminous gas of nebulae too, of course). The layperson finds intrigue in the term Dark Matter, because journalists are trying to sell a story.