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In a galaxy far far away... M6760 (I made it up) is an unusually massive neutron star billions of light years away and it is surrounded by a spherical Dyson sphere painted in new improved formula vantablack called Perfect Blackbody 2.0 (trademarked & copy rights) using alien tech of course (actually it is depleted carbon nanotube). So from Earth perspective, how can we tell that is it not a blackhole using modern day technology?

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    $\begingroup$ No accretion disc $\endgroup$
    – nzaman
    Commented Dec 30, 2019 at 12:18
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    $\begingroup$ Depleted carbon? $\endgroup$
    – T.J.L.
    Commented Dec 30, 2019 at 16:09
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    $\begingroup$ And what exactly Dyson sphere may be used for around a black hole or a neutron star? Both objects don't radiate much by themselves and whoever built the sphere probably took care about the acreting material, so no radiation inside at all. Your sphere will be (given time) probably in a thermal equilibrium with the microwave background, i.e. completely invisible. The only way we can know about the object is if it has some satellite stars. If they are of the right kind, we can deduce the mass of the unknown object. $\endgroup$
    – fraxinus
    Commented Dec 30, 2019 at 16:40
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    $\begingroup$ Anish Kapoor is stuck on earth, and so it can't possibly be ;) $\endgroup$ Commented Dec 30, 2019 at 17:28
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    $\begingroup$ @Matthew why do we need to know what the aliens were doing? We don't care. The asker just wishes to know if you can tell the two apart. Why the aliens made it black is arguably a tangentially relevant detail. They did it because they could and it looks cool. $\endgroup$
    – user64742
    Commented Jan 2, 2020 at 0:22

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When we “see” a black hole or neutron star, we don’t see the actual body itself — they’re much too small, as well as black holes being black. So there’s no point messing around with Dyson spheres and black paint, because none of that will change what we see. We detect both black holes and neutron stars from their effects on the nearby matter and light, and none of those will change because of what you’re planning.

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    $\begingroup$ Actually we do see at least some neutron stars, for instance pulsars: en.wikipedia.org/wiki/Pulsar Though of course a Dyson sphere around an active pulsar rather boggles the mind :-) $\endgroup$
    – jamesqf
    Commented Dec 30, 2019 at 17:46
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    $\begingroup$ @jamesqf depends. Pulsars are a powerful source of energy and they distribute it evenly along a pair of circles. Now, you need to feel comfortable powering your laptop from thunderstorms before even thinking of making any use of this beast,. but hey... Kardashev 3 is Kardashev 3 $\endgroup$ Commented Dec 30, 2019 at 20:15
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    $\begingroup$ @John Dvorak: Dyson sphere is a closed surface (by definition) which needs to be made of solid matter. So unless you know the way to the secret handwavium mines, where exactly are you going to find something that can withstand being hit by a relativistic particle jet. Your Dyson sphere immediately becomes a ring. Then, unless you have a really old, cool neutron star, its temperature is around a million K, so it's radiating in X-rays. Then there's the magnetic field... $\endgroup$
    – jamesqf
    Commented Dec 31, 2019 at 1:52
  • $\begingroup$ @jamesqf Don't really need handwavium, just a magnetic field strong enough to bend that particle jet and spread it across a bigger surface so you can absorb its energy to power your field. The generator necessary to bootstrap this process would be impressive though... $\endgroup$
    – Perkins
    Commented Dec 31, 2019 at 18:53
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    $\begingroup$ We study the wind by looking at the movement of the trees. $\endgroup$
    – Ink blot
    Commented Jan 1, 2020 at 11:52
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I'm surprised no one has mentioned this.

Your ultra-black Dyson sphere is easily distinguishable from a quiescent black hole or unnaturally cold neutron star by one major thing, if you're close enough to tell those two objects apart:

It blocks out too many background stars.

That is, your Dyson sphere, to avoid having surface gravity too great to support itself, will be many times larger than the neutron star, never mind the event horizon of a black hole. Whatever means you use to spot it (IR blackbody radiation, reflection at wavelengths your upgraded Vantablack doesn't absorb), by the time you can detect anything but gravity to know there's something odd, you'll easily be able to tell that, black as it is, it’s FAR larger than anything that should be that black.

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    $\begingroup$ This is an interesting idea. Given the distance to this galaxy, though (billions of light-years), I assume the angular size would be small enough that we wouldn't be able to observe any of these occultations. $\endgroup$
    – HDE 226868
    Commented Jan 1, 2020 at 16:05
  • $\begingroup$ This was actually mentioned before, in Cadence's comment to dspeyer's answer; of course your answer is still a good one $\endgroup$ Commented Jan 1, 2020 at 17:38
  • $\begingroup$ @FelixDombek I'm pretty sure my answer is older than that comment. $\endgroup$
    – Zeiss Ikon
    Commented Jan 2, 2020 at 12:04
  • $\begingroup$ @ZeissIkon One can hover the mouse over an inexact timestamp like "2 days ago" to see the exact time, which tells that the comment is 12h older if I read this correctly. $\endgroup$ Commented Jan 2, 2020 at 18:37
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Vantablack doesn't reflect light, but it'll still have black body radiation based on temperature. It may be far into the infrared, but the black body curve is a signature we can recognize from a distance.

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    $\begingroup$ Then of course people would be trying to figure out the intersection of less than 2.17 solar masses and a BBR spectrum of 500K. There's not a lot there $\endgroup$ Commented Dec 30, 2019 at 10:29
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    $\begingroup$ @VaradMahashabde You'd also have to factor in that (although extremely dim) it's visually much bigger around than 2.17 solar masses would imply. Whether the visible diameter makes it easier or harder to solve is beyond me, though. $\endgroup$
    – Cadence
    Commented Dec 30, 2019 at 12:06
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Fair chance this Dyson Sphere is larger than the Golden Gate Bridge. Once you're at that size, painting it is not an event so much as an ongoing activity. You start at the Presidio, and by the time you reach the Marin Headlands, the paint where you started is at End Of Life, and you must start over.

I don't know how big Dyson Spheres are, but probably big enough to probably warrant at least 5 or 6 paint gangs. So it won't look like a black hole, it'll look more like a black melon.

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    $\begingroup$ The GGB is subject to a lot more weathering than in space, however... $\endgroup$
    – Matthew
    Commented Dec 30, 2019 at 19:38
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    $\begingroup$ @Matthew but the weathering you do get in space is impressive.... $\endgroup$ Commented Dec 30, 2019 at 19:46
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    $\begingroup$ In some sense, that's a fair point... although scratching the paint is hardly the end of your worries w.r.t. asteroid impacts. I think this goes back to the point I was making, however, which is why is this thing painted with radiation-absorbing paint in the first place? As other answers note, it doesn't seem very useful as an attempt at stealth on something this size... $\endgroup$
    – Matthew
    Commented Dec 30, 2019 at 19:52
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    $\begingroup$ Obviously, there's a solar-system-sized paint sprayer being constructed concurrently with the Dyson sphere which somehow slipped OP's mind. $\endgroup$ Commented Dec 30, 2019 at 22:06
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    $\begingroup$ Dyson spheres are massive enough to accumulate their own atmosphere on the outside. They might very well have weather. $\endgroup$
    – SRM
    Commented Dec 31, 2019 at 7:54
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We mostly identify black holes by the effects of their gravity on surrounding bodies, and the behavior of accreted matter. We have an idea of where the limit is for the mass of a Neutron Star. If we assume the obscured Neutron Star is mostly isolated from enough dust and gas for the accretion to be noticeable[1], we'd suspect based on the apparent mass. I suspect we'd find it very interesting, even if it is the maximum mass allowable for a Neutron Star, and would search for it to be sure we don't need to change our models. At which point, the question becomes exactly how faint the enclosure can make any radiation that tries to escape, because it is highly unlikely it could be perfectly opaque to all wavelengths.

[1] What happens to the enclosure if an accretion disk does form? It depends on the size and other properties of the enclosure, but my guess is that it would eventually get hot enough to have a detectable infrared presence, so I have to assume it's relatively "clean" space, and we "only" have to worry about radiation from inside heating it to a detectable glow.

The main thing to worry about is that there will be heat, and it must go somewhere. Either your enclosure will radiate it, or it will be destroyed by it. There are also other things, like polar jets etc that Black Holes give off, which it might be able to fake, but in the end, you need a way to hide the heat, and obfuscate the mass.

Given the above, you need a very massive, very cool Neutron Star, without a lot of accretable matter in the vacinity, and to design your enclosure so as to make any remaining heat difficult to detect, and to deal with any other radio signatures that would distinguish Neutron Stars from Black Holes. Deviate from any of those, and astronomers can probably tell what's up. Infrared and weird behavior of accreted matter, combined with apparently having too low a mass for a Black Hole, will get speculation going. It'd be very difficult to get just the right mass, and hide the heat, and get any necessary radio shenanigans just right, and deal with accretion realistically. The more realistic you want the disguise, the more complex your enclosure becomes, and then you have the risk of someone seeing it from just the right angle to notice that something's off when it passes in front of a star.

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Curvature

Mass bends space.

A large dyson sphere encircling a neutron star at the high end of the mass spectrum will bend light differently to a black hole.

The dyson sphere would have to be constructed in such a way that its mass was uniform in all directions done the planck length. Otherwise one side of the sphere will curve light more than any other part of the circle seen from earth.

Jets

Black holes, and Neutron stars produce jets of accelerated matter at their poles. The energy imparted into the jet informs us of the strength of the thing accelerating the mater. Needless to say Neutron stars accelerate mater to very different energies compared to blackholes.

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The gravitational lensing creates a ring of light around the photon sphere of a black hole. A neutron star wrapped in a Dyson Sphere has less mass in larger volume, so it causes much less gravitational lensing and therefore won't create this effect. The distortion of background around it will also be much weaker.

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Vantablack absorbs visible light by trapping said light in its carbon nanotubes, and that light eventually dissipates into heat, so as @dspeyer said, infrared sensors could be used to detect this change in heat/temperature whereas a black hole would not be detected by this method/observation.

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    $\begingroup$ Good point. Perhaps Perfect Blackbody 2.0(tm)(R) is one of those tow-layer paints, with vantablack being the lower layer, and the upper layer being made entirely of Maxwell's Daemons. $\endgroup$ Commented Dec 31, 2019 at 3:09
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If you cover the black hole with a Dyson sphere you can't tell them apart. The Dyson sphere would have to be large enough to have the accretion disk inside. You are just left with the gravitational effects. At any reasonable distance, you only see the total mass because the stuff inside the sphere will be roughly spherically symmetric.

You could tell that it is not a neutron star if the mass were too large for it to be one.

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