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Immersion At first I thought the inherent lack of haptic feedback would stymie the game and make it less fun than a similar controller-based game like Rock Band VR on Rift. If hand-tracking were more solid I would put it nearly equal to a controller-based rhythm game in the amount of fun and skill you can build. Simply put: when it works, Unplugged is awesome. And although haptics would undeniably help the game, Unplugged does a good job filling in the gaps with its array of expressive visuals.
Strumming on the other hand no pun intended is a binary action that has to be done with a enough force to register. It feels a bit like having a button on your controller that works 90 percent of the time. Here I go through finger counting on both hands just to show how off Quest can be at times. She spends her time conveying astronomy to people outside the university walls, and additionally she helps current Astronomy Professors getting their research out in public.
Majken has her own company called Astronomicca, where she also runs a blog about astronomy. I also love to read so, when combining the two, you get love to read about astronomy. I like learning about things that I like so I will pay close attention to anything astronomy related.
Abstract In this article we explain the process of star formation for regular Sun-like stars. Stars form from an accumulation of gas and dust, which collapses due to gravity and starts to form stars. The process of star formation takes around a million years from the time the initial gas cloud starts to collapse until the star is created and shines like the Sun. The leftover material from the star's birth is used to create planets and other objects that orbit the central star.
Observing star formation is difficult, because the dust is not transparent to visible light. It is, however, possible to observe these dark stellar nurseries using radio waves, because radio waves travel freely down to us and our radio telescopes. Stars, like our own Sun, have not always been around. Stars are born and die over millions or even billions of years. Stars form when regions of dust and gas in the galaxy collapse due to gravity.
Without this dust and gas, stars would not form. The Dusty Nuseries of Stars A galaxy contains not only billions of stars, but also large amounts of gas and dust. These regions of gas and dust in the galaxy lie in the space between the stars. If the galaxy were a street, the houses would be stars and the regions of gas and dust would be the gardens in between the houses.
The space between the stars in a galaxy is called the interstellar medium , because it is the medium, or substance, that makes up the space between stellar objects. The regions of gas and dust are called molecular clouds , because of their content. Molecular clouds are made of a mix of atoms, molecules, and dust. Atoms are the small building blocks of all the stuff around us. Molecules consist of two or more atoms joined together. The molecules present in molecular clouds are typically molecular hydrogen, H2 , but can also be more complex molecules, such as methanol, which consists of six atoms, or water, which consists of three atoms.
Dust grains are even larger clumps of matter and they can be up to a few millimeters in size, which is huge compared with atoms or molecules. Molecular clouds in the interstellar medium are large. In fact, a single molecular cloud can be hundreds of thousands of times heavier than the Sun. Their volumes also vary: a molecular cloud can be the same size as, or many times bigger than, our entire solar system.
These enormous molecular clouds undergo turbulent motion. This means that the gas and dust within the clouds do not stay in the same place as time passes. These substances move around in all directions, like children running around in a school yard. This turbulent motion of the gas and dust distributes the atoms and molecules unevenly, so that some regions of the molecular cloud will have more matter in them than other regions Figure 1A. If the gas and dust pile up to a very high level in a certain region, that region starts to collapse due to the pull from its own gravity.
The region is smaller than the molecular cloud and lives inside the molecular cloud. Figure 1 - The process of star formation. The illustration shows the six steps of star formation for Sun-like stars. The process starts on A , where gas and dust in the space between stars also called the interstellar medium, ISM collapse into a dense ball of gas called a prestellar core B that eventually will become the sun.
During the collapse a disk C forms around the core, while two jets are emitted at the poles. At some point the star stops growing, but gas still fall onto the disk D. After a few million years this process also halts. The star is now born E , while the planets are being formed from the left-over material, which will eventually become a solar system F.
A solar system typically lives 10 billion years after the formation process. But, when gas and dust start to collapse in a region within the molecular cloud, it slowly heats up. This is a consequence of a law of physics, which tells us that, when matter is squeezed together, the density of the matter will increase and the matter will start to heat up.
When the collapsing region has reached a size of nearly 10, AU, it is called a pre-stellar core Figure 1B and is officially a star in-the-making. Also, this pre-stellar core will later become the interior core of the star. Over the next 50, years or so, the pre-stellar core contracts.
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