Introduction In this two-part lab you build spectroscopy using the components included in the lab kit and visualize and analyze the spectra of multiple light sources. In the second half of the experiment, I will create a pinhole viewer. Then use the pinhole viewer to measure the sun and moon diameters. After completing the two parts of the lab, there are some problems that need to be addressed. This article looks at these questions and answers. Spectrometer In order to understand this week's experiment, you first need to understand what the spectrometer is and what it does.
There are two types of investigation: imaging and spectroscopy. Dark energy measurement and the atmospheric meteorological telescope (LSST) are image surveys, the baryon vibration spectrum measurement (part of Sloan Digital Sky Survey), eBOSS and dark energy spectrometer are spectral measurements. In the image survey, we take pictures of the night sky using a huge camera - a car of a certain size. The more distant you are, the longer the distance the light will reach. When you shoot galaxies, galaxies, supernovae at various distances, you can see the temporal distribution of substances. The dark energy survey began data collection in 2013 and shot more than 300 million galaxies. By the end of 2018, it takes about one eighth of the total night sky. LSST will further expand what we know
From distance triangle and spectral parallax. Determining the distance of a star is a way to calculate the scale of objects in the galaxy and it is important to understand stars. It is because you can calculate the energy generated and emitted using the inverse square law method and the apparent brightness of the star for dimming. Distant. A star visible to the naked eye at night is a corner of the iceberg. Even though we go out on a sunny summer evening, the lights in the city are not too bright and we can see the light in the sky. This is the "Galaxy" - the light from thousands of unresolved stars in the Milky Way (the galaxy with the capital "G" is the galaxy where we live)