Stars essays
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Abstract One of the main problems in the world of astro-physics is differentiating between heavenly bodies such as stars and quasars which are distinct from each other. The main problem between scientists and researchers alike is that they have a hard time differentiating the two separate entities from the collected SDSS catalog data that comprises of the features and classification data. The current methods have proved to be inefficient and not up to par with modern expectations. Matching the recorded...
3 Pages
1419 Words
There is a huge difference between the three spectra. The first to use was the Testine Light Bulb, which gave us tremendous results. When the light bulb is lite passes through a colorful rainbow displayed with the whole number of colors, red, orange, yellow, green, blue, indigo and violet which were clearly separated. The second source was the Energy Efficient Light Bulb. The bulb on usual occasions shows a white light. When the light bulb’s light passes through the spectroscope,...
1 Page
485 Words
Several billion years after a star’s birth its life will eventually end. How a star will die is determined by its mass, age, and type. The sun and other stars shine as results of reactions in its core. This changes light elements to become heavier and release energy in the process, which creates the necessary pressure needed to keep stars from collapsing in on themselves. When a star’s core lacks hydrogen fuel it stops its flow of energy, therefore, disabling...
1 Page
492 Words
Helioseismology, simply put, is the study of the Sun’s core through the observation of wave propagation that is visible on the surface. This is possible due to both the continual movement of plasma to the sun’s surface, as well as the constant radiation from the heat, that forms convection cells resulting in the investigable convection currents or “waves”. As each cell and consequently current, have varying fluctuations in pressure, the Sun is left with its uneven surface. As well as...
4 Pages
1621 Words
The Sun, the centre of our solar system, an object in which without life on Earth would cease to exist. The Sun provides energy to Earth which allows many important chemical reactions to take place in order to facilitate life. Our Sun is relatively hot and immense, conducting physical investigations to obtain information is impossible, therefore safe and long-distance techniques have been developed in order to study our Sun and then extend these techniques further to study other stars in...
4 Pages
1809 Words
