<p>For an observer hovering [I say hover because by definition there are no orbits for an observer at the photon sphere] at the photon sphere for a non-maximal de Sitter-Schwarzschild black hole, a simple accelerometer will tell an observer which horizon is which. The reason for this is that in order to hover at the photon sphere the observer must take up a non-inertial local frame with a directional bias decided by the direction of the BH event horizon. </p>

<p>In the maximal de Sitter-Schwarzschild spacetime the BH singularity disappears and the observer will not be able to tell the difference between the two horizons as there is an automorphism of that spacetime which will map one horizon to the other.</p>

CC BY-SA 3.0
2014-10-10T21:29:10.243Z
Where can I read about maximal spacetimes.
Anixx
CC BY-SA 3.0
2014-10-11T01:56:21.080Z
http://en.wikipedia.org/wiki/De_Sitter%E2%80%93Schwarzschild_metric#Nariai_solution
John Davis
CC BY-SA 3.0
2014-10-09T21:56:30.037Z
2014-10-10T00:48:37.007Z
2014-10-10T00:48:37.007Z
John Davis
<p>A person at the <a href="http://en.wikipedia.org/wiki/Photon_sphere" rel="nofollow">photon sphere</a> of a black hole will observe the following:</p>

<ul>
<li><p>The black hole surface will cover exactly half of the visible sky (say, the left half), and cosmic horizon will cover the other half.</p></li>
<li><p>Looking in any direction between these hemispheres the person will see oneself.</p></li>
<li><p>The person will observe no centrifugal force however fast he moves. Any object the person thowing to the left will experience the centrifugal force pulling it further left, while any object thrown to the right also will experience the centrifugal force pulling it to the right. Approaching the black hole in such circumstances may look quite like actually escaping it to the crew.</p></li>
<li><p>The space to the right as well the space to the left seemingly includes objects of any length and dimensions, the further objects are, the more they are time-dilated and length-contracted.</p></li>
</ul>

<p>Is there any way for a spacecraft commander to decide (by an experiment conducted in a small$^1$ amount of time) which hemisphere is the sky and which hemisphere is black hole in such circumstances?</p>

<p>--</p>

<p>$^1$ Here <em>small</em> means small compared to characteristic time scales of the problem.</p>

<black-hole>
Can a person at a photon sphere of a black hole decide where the black hole is?
Anixx
# Can a person at a photon sphere of a black hole decide where the black hole is?

(Asked by: username_0 on 2014-10-09)

A person at the [photon sphere](http://en.wikipedia.org/wiki/Photon_sphere) of a black hole will observe the following:

* The black hole surface will cover exactly half of the visible sky (say, the left half), and cosmic horizon will cover the other half.
* Looking in any direction between these hemispheres the person will see oneself.
* The person will observe no centrifugal force however fast he moves. Any object the person thowing to the left will experience the centrifugal force pulling it further left, while any object thrown to the right also will experience the centrifugal force pulling it to the right. Approaching the black hole in such circumstances may look quite like actually escaping it to the crew.
* The space to the right as well the space to the left seemingly includes objects of any length and dimensions, the further objects are, the more they are time-dilated and length-contracted.

Is there any way for a spacecraft commander to decide (by an experiment conducted in a small$^1$ amount of time) which hemisphere is the sky and which hemisphere is black hole in such circumstances?

--

$^1$ Here *small* means small compared to characteristic time scales of the problem.

**Tags:** black-hole


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## 1 answers

### Answer by username_1 on 2014-10-09. Score: 4 | Accepted answer

For an observer hovering [I say hover because by definition there are no orbits for an observer at the photon sphere] at the photon sphere for a non-maximal de Sitter-Schwarzschild black hole, a simple accelerometer will tell an observer which horizon is which. The reason for this is that in order to hover at the photon sphere the observer must take up a non-inertial local frame with a directional bias decided by the direction of the BH event horizon.

In the maximal de Sitter-Schwarzschild spacetime the BH singularity disappears and the observer will not be able to tell the difference between the two horizons as there is an automorphism of that spacetime which will map one horizon to the other.

> **Comments:**
> **username_0**: Where can I read about maximal spacetimes.  
> **username_1**: http://en.wikipedia.org/wiki/De_Sitter%E2%80%93Schwarzschild_metric#Nariai_solution  

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