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Astrochemistry: Elements and Compounds

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H2O

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Water, an important molecule for life; exists on celestial bodies such as comets, moons, and exoplanets.

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He

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Helium, produced during Big Bang nucleosynthesis; the second most abundant element in the Universe.

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CO2

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Carbon dioxide, a molecule that can be found in the atmospheres of planets and as ice in molecular clouds.

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NaCl

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Sodium chloride, also known as table salt, has been detected in the atmosphere of an exoplanet.

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C2H2

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Acetylene, a hydrocarbon used in stellar atmosphere studies to understand carbon-based chemistry.

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H2CO

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Formaldehyde, an organic molecule found in the interstellar medium; involved in the synthesis of more complex molecules.

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CO

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Carbon monoxide, abundant in the interstellar medium; it is used as a tracer for molecular hydrogen.

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H2S

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Hydrogen sulfide, a toxic gas found in the interstellar medium; also known for its 'rotten egg' smell.

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Ca

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Calcium, a metal that forms dust in the interstellar medium; contributes to the spectrum of stars.

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Ni

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Nickel, an element produced in large stars and found in meteorites; contributes to the metal content of planetary cores.

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N2

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Nitrogen, makes up a significant portion of Earth's atmosphere and is found in the interstellar medium.

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P

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Phosphorus, a key element for life, found in the interstellar medium; plays a role in the formation of biomolecules.

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NH3

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Ammonia, found in the atmospheres of gas giant planets and in the interstellar medium; used in the synthesis of organic molecules.

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H3+

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Trihydrogen cation, plays a critical role in ionizing molecular clouds and initiating a chain of interstellar chemistry.

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Ar

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Argon, a noble gas found in planetary atmospheres and known for its lack of chemical reactivity.

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CH3OH

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Methanol, an organic molecule found in the interstellar medium; serves as a building block for more complex organic molecules.

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H

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Hydrogen, the most abundant element in the Universe, often forming molecular hydrogen (H2) which is essential in star formation.

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C2H6

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Ethane, a simple molecule found in the atmosphere of Titan and other celestial bodies; a hydrocarbon like methane.

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CH4

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Methane, a simple organic molecule found in planetary atmospheres, such as Titan's, and in the interstellar medium.

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H2SO4

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Sulfuric acid, detected in aerosol form in the atmosphere of Venus; its presence indicates volcanic or lightning activity.

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SiO2

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Silicon dioxide, a dust component in the interstellar medium; prevalent in rocky planets and meteoroids.

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S

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Sulfur, an element participating in sulfur-based chemistry in interstellar clouds; essential for some biological processes.

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Ne

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Neon, a noble gas with a distinct glow when ionized; found in stars and is used as a tracer for cosmic radiation.

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Fe

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Iron, a heavy element created in supernovae; plays a role in star formation and planet composition.

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C

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Carbon, a versatile element that is the backbone of organic chemistry and found throughout the Universe.

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O3

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Ozone, a form of oxygen that absorbs harmful ultraviolet radiation; found in the atmospheres of planets.

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O2

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Oxygen, in molecular form is essential for life on Earth, and it's present in low abundance in the interstellar medium.

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HCN

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Hydrogen cyanide, a compound detected in interstellar clouds; can give rise to amino acids and nucleotides.

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Si

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Silicon, found in cosmic dust and rocky planets; essential for silicate minerals in the Universe.

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Li

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Lithium, an element created during the Big Bang and within stars; its abundance helps to understand stellar processes.

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