Crime & Punishment

You could have at least left some magazines for us to read whilst we wait.

I'm particularly partial to 'Horse & Rider' and a little known alternative fetish publication called 'Goldfish Girls'.

Reserved for the bureau of reservational withholdings for parties that called ahead, a division of the redundancy department of redundancy.

reserved for bumping

Reserved for femmy eyeliner wearing pirates to spout recycled overused disney pirate jargon......

My freighter is awaiting the arrival of your Kraken.

So it's been what 5 days now? Slow start I guess...

He said all freighter would die. No reason to choose a target.

But you always have to start with a bang, otherwise you're no better than other freighter-ganks.

Ah...that would explain the sudden spike in Catalyst sales.

Posting on an internet forum.

Also, the idea of a body so massive that even light could not escape was first put forward by geologist John Michell in a letter written to Henry Cavendish in 1783 of the Royal Society:

If the semi-diameter of a sphere of the same density as the Sun were to exceed that of the Sun in the proportion of 500 to 1, a body falling from an infinite height towards it would have acquired at its surface greater velocity than that of light, and consequently supposing light to be attracted by the same force in proportion to its vis inertiae, with other bodies, all light emitted from such a body would be made to return towards it by its own proper gravity.
—John Michell

In 1796, mathematician Pierre-Simon Laplace promoted the same idea in the first and second editions of his book Exposition du système du Monde (it was removed from later editions). Such "dark stars" were largely ignored in the nineteenth century, since it was not understood how a massless wave such as light could be influenced by gravity.

Furthermore!

The no-hair theorem states that, once it achieves a stable condition after formation, a black hole has only three independent physical properties: mass, charge, and angular momentum. Any two black holes that share the same values for these properties, or parameters, are indistinguishable according to classical (i.e. non-quantum) mechanics.

These properties are special because they are visible from outside a black hole. For example, a charged black hole repels other like charges just like any other charged object. Similarly, the total mass inside a sphere containing a black hole can be found by using the gravitational analog of Gauss's law, the ADM mass, far away from the black hole. Likewise, the angular momentum can be measured from far away using frame dragging by the gravitomagnetic field.

Food for thought.