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Category:Tetrapod unranked clades
Category:Timetarily ‘First Appearance’ organisms
Category:Early Cretaceous first appearancesAs we accelerate through the tail end of the expansion pack cycle, I find myself glued to two games that I would classify as ‘roguelikes’ or ‘videogames.’ The first is 8BitMMO, a social MMO (massively multiplayer) game that is based on the concepts of virtual world programming and Second Life. I have been a longtime fan of the game as I played 8BitMMO when it was known as Telepolis, and I have followed it and the fork in its development known as No One Is Online. As I write this, the game is now officially a standalone client but, as you will see if you scroll down to the bottom of this article, I am still playing an offline version. I am a bit bothered by the end game — the teleportation of players to a new game world — that has been developed to replace 1v1 PvP in the game. The other title is PlaneShift, a ‘videogame’ (or videogam, or vidgeam, depending on your preference and source) that is still in the early stages of development but, I hope, will eventually incorporate ideas gleaned from the development and usage of the other game I am playing, Voxatron.

PlaneShift

I think most, if not all, people who are familiar with the concept of Voxatron or 8BitMMO are aware of the video below that presents PlaneShift. I first published this video back in 2010, and I really should have gotten around to writing something about it. Anyway, suffice it to say that I’m doing it now.

8BitMMO

Like PlaneShift, 8BitMMO is a unique creature that has all the characteristics of a videogame but is also something else. It has a standalone client. It has a virtual world where individual users can build their own ‘independent’ cities, industries, stores, and other community-creating features. You can also download and run, and share, your own mini-games on the server. It is a little like Second Life, but unlike SL, user content gets built in from the ground up. It is a vidgame, but unlike PlaneShift, it doesn’

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By igniting a suddain burst of energy at the heart of a star, astronomers have found a dwarf star that has a record-breaking value of rotation in just one second.
The record-holding star is thought to be an unusual type of star, called a Wolf-Rayet star. These are stars that are very hot and very massive and we now believe that may be close to its final, nuclear-burning period.
Researchers at the University of Hertfordshire measured the rotation of this star and found it to be rotating around six times a second.
It is by far the fastest rotator ever discovered.
Stellar rotations provide valuable information about the internal structure and the history of the star, but methods used to measure these values are limited by the speed of the star’s rotation.
This was the team’s first measurement of rotation for a star that is so hot.
Anastasia Mikulski, of the University of Hertfordshire’s Astronomy Centre, said: “Measurement of rotation for stars with a temperature beyond 40 000 ‰K is notoriously difficult.
“Hotter stars rotate faster and thanks to new technology, we have been able to measure the rotation of a Wolf-Rayet star – and a very fast one at that.”
The star has an estimated mass of between 30 and 100 times that of our Sun, which sits at the size of a single Earth-mass planet.
It is between 20 and 30 light-years from Earth.
The name of the star is PHL 2227 (pronounced PHL – 22 – 27), a type of star known as a Wolf-Rayet star – shorthand for the type of star where the elements of nitrogen, oxygen and carbon fuse and give off powerful radiation.
Wolf-Rayet stars are common in the Universe and roughly the stars that are found among the stars of our own galaxy, The Milky Way.
All the stars in the Milky Way galaxy that we can see with telescopes are in this category.
This kind of star has been theorised to be a very short-lived phase in the life of a star.
This means that it will not last long in its current life as it is eating away the contents of its core.
As it burns away it first becomes a supergiant star, its luminosity and size increasing as the star loses mass.
A Wolf-Rayet star is believed to be a short
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