Emission spectrometry is an old and largely known method for quantitative and qualitative analysis of elements.
It means the element which you need to detect.
Scientist have been sending rovers and astronauts to the other planets to detect life on other planets. (I think I'm not 100% sure,sorry)
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.
carbon is used in rat poison and is the title of a murder mystery
If you use high-end equipment such as electron microscopes, you can detect the amount of electrons are in an atom and therefore identify that element. Examples; 1 electron - Hydrogen 8 electrons - Oxygen 111 electrons - Roentgenium
It means the element which you need to detect.
Positron Emission Tomography (PET) scans are used in hospital mainly to detect cancers, especially cancers that have metastasised or spread into surrounding tissue.
phosphoros
The isotope iodine-131.
Cesium doesn't have a smell you need special equipment to detect Cesium.
Scientist have been sending rovers and astronauts to the other planets to detect life on other planets. (I think I'm not 100% sure,sorry)
to use the computer for research on a certain topic
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.
HPLC (high pressure liquid chromatography), hair samples and bodily fluids can be tested this way.
things like contents of atmosphere, heat, etc.
It is a faeces (poo) sample, which can be used by a biomedical scientist to determine the cause of diarrhoea for instance, or detect the presence of occult (hidden) blood.
All elements have their own discrete power spectra. To excite a hydrogen atom requires a different amount of energy than to excite a helium atom. The energy of a photon is proportional to its wavelength. So by looking at the wavelengths in the absorption or emission lines in the spectra and comparing them to known energy levels (empirical or quantum mechanic derived) of different elements, a great deal can be said about a stars outer layer.