Science of Sunlight and Stars

This paper will attempt to explain how the astronomical instruments help astronomers as him or her are determining temperature, rotation rate, distance, and composition of objects. The paper will attempt to explain the understanding on the properties on stars in the Hertz sprung-Russell Diagram of the Cosmic Perspective. The paper will attempt also to explain and summarize a complete lifecycle of the sun, and the suns nature, and properties. The paper will also attempt to explain, and explore for a determination on where the sun is in the lifecycle. The paper will also attempt to explain the elements of the sunlight and stars. The paper will also briefly explain Newtons version of measurement of the suns radius.

The spectroscope is the simplest, and is consistency with the quartz or the glass of the prism, and is more common to have an understanding of today's solar system. To have an understanding there can be a diffracting of grate that could be an addiction for the front of the spectroscope lens. Therefore, the sum of light is a collection through the telescope may pass within the prism and the grate. This may happen at the split of each component, and can produce a spectrum of characteristic.

Astronomer that has the use of scopes, and graphs can enable a depth detail of his or her information collecting on the bodies of the celestial. The astronomer can collect more information using both spectrograph, and the spectroscope than any other astronomer. Astronomers that use a measurement for the displacement for the Doppler shift, and spectral line he or she could have a determination for velocity of the moving star, and the star could be moving toward earth or moving away from the earth.

The spectral lines, and the displacement can perhaps provide astronomers with information on the binaries of the spectroscopic. The data may also be on the double stars, and these double stars will not be resolve by the use of the telescope. Therefore, coming from information, the profile, intensity, and the lines of spectral is what the stars obtain such as the pressure, temperature, the chemical composition, and the stratification.

The Earth's atmosphere, and the opacities is a range of narrow path of the electromagnetic of wave length, and this can be a study within the ally of spectroscopic, and this allows any person to study from the surface of earth. Astronomer's may use balloons of high-altitude, rockets for researching, and the satellites that may carry the equipment of spectroscopic, and allowing the astronomers to extend the ranges of the X-ray's, gamma-ray's, infrared, and the ultraviolet portion of region (2. worldsite).

The H-R Diagram is a graph at the stars position at the axis, it tells the temperature. The temperature is in relation to the color, and also to the spectral type. The luminous is a location of the vertical. The axis will indicate that the sun is along