No.
285nm is ultraviolet, and I think with a spectroscope you actually look with your eye to see the emission - you would not be able to see this wavelength. If you put some kind of a film that reacts to UV light in the spectroscope, you could then "see" it as a mark on the film.
Depending on the method many chemical or physical properties can be used. Examples: spectra of emission, color of ions in solution, formation of some precipitates, melting point, density, etc.
The mass number can be found by multiplying the mass of a single atom by Avogadro's number, that is 6.022 X 1023. In this instance, the product is 23.0, and the element is probably sodium, which has this gram atomic mass. mass number is less than 1, which does not correspond to any real, stable atom. The element could conceivably be a rare isotope of neon or magnesium.
The study of line spectra was useful in the discovery of new elements because each element has a unique line spectrum that can help identify and distinguish it from others. By examining the line spectra of unknown substances, scientists could match their patterns with known elements, revealing the presence of new elements with distinct spectral signatures. This technique played a crucial role in the discovery and characterization of many new elements in the periodic table.
honestly what kind of question is this? what do you mean? could they identify different cola cans? flavor? what?
Yes, the optical spectrum of sunlight contains absorption or emission lines that can be used to identify the elements present in the sun. Each element produces a unique pattern of lines in the spectrum, allowing astronomers to determine the composition of the sun and other celestial bodies.
In atomic spectroscopy, each element has a unique spectrum. The atomic spectrum obtained from a sample is a combination of the spectra of each elemental component. We take the strongest line from the sample spectrum and determine which elements could have caused it (we call these "candidates"). We then look at the full spectrum from each candidate and see whether or not every major line is present in the sample spectrum. If so, we say that element is present.Then we subtract the spectrum (or spectra) of the element(s) we have determined to be present from the sample spectrum and repeat the same process with the next strongest line in the (leftover) sample spectrum. We continue repeating this process until all lines in the sample spectrum are accounted for.
This could have many names such as 'decay', 'radioactive decay', or 'radiation.
Not necessarily. The absence of specific spectral lines could be due to factors like the star's temperature, composition, or magnetic fields affecting the spectral lines. It could also be that the element is present in trace amounts that are not detectable in the spectrum.
The presence of the nitrate ion in solution typically does not have a direct effect on color emission. Nitrate ions are typically colorless and do not absorb visible light that would result in color emission. However, in some cases, nitrate ions can indirectly affect color emission by participating in complex chemical reactions that result in color changes.
Helium, the second most abundant element in the universe, was discovered on the sun before it was found on the earth. Pierre-Jules-César Janssen, a French astronomer, noticed a yellow line in the sun's spectrum while studying a total solar eclipse in 1868. Sir Norman Lockyer, an English astronomer, realized that this line, with a wavelength of 587.49 nanometers, could not be produced by any element known at the time. It was hypothesized that a new element on the sun was responsible for this mysterious yellow emission. This unknown element was named helium by Lockyer.
Spectra is the plural of spectrum. You could discuss the spectrum generated by an element in a star, and comparing more than one element, you would be comparing spectra. (Latin -um words form plurals like this, so you cannot refer to them as spectrums. Another example is datum, singular, and data, plural.)
identify and define the elements of the communication process
285nm is ultraviolet, and I think with a spectroscope you actually look with your eye to see the emission - you would not be able to see this wavelength. If you put some kind of a film that reacts to UV light in the spectroscope, you could then "see" it as a mark on the film.
Identifying an unknown element is helpful in various scientific and industrial applications, such as determining the composition of a material, investigating pollution sources, or developing new technologies. It can also be crucial in fields like forensic science, environmental monitoring, and quality control.
The visible spectrum
Depending on the method many chemical or physical properties can be used. Examples: spectra of emission, color of ions in solution, formation of some precipitates, melting point, density, etc.