Category: CR 2: Modeling Conservation of Mass (MS)

Develop and use a model to describe how the total number of atoms does not change in a chemical reaction and thus mass is conserved

Chemical Reactions, CR 1: Determining Chemical Reactions (MS), CR 1: Predicting Reactions (HS), CR 2: Energy in Reactions (HS), CR 2: Modeling Conservation of Mass (MS), CR 3: Evidence of Reactions (HS), CR 3: Testing Endo/Exothermic Reactions (MS), CR 4: Driving Reactions (HS), Non-NGSS Articles, Physical Science, S&P 1: Atoms & Molecules (MS), S&P 1: Periodic Table Patterns (HS), S&P 3: Heat & Reactions (MS), S&P 4: Molecule Traits (HS), Structure & Properties of Matter, W 1: Graphing Waves (MS), W 1: Wave Relationships (HS), W 2: Wave Behavior (MS), Waves & Electromagnetic Radiation

Beaming Pyrimidines Part 2

GwynneL.

Thymine and Other Prebiotic Molecules Produced from the Ultraviolet Photo-Irradiation of Pyrimidine in Simple Astrophysical Ice Analogs(NOT OPEN ACCESS) SUMMARY: In the second edition of beaming pyrimidines, instead of using ammonia, scientists beamed pyrimidines with methanol, water and methanol, methane, and water and methane. As with “Beaming Pyrimidines Part 1”, the gases were cooled way… Continue reading Beaming Pyrimidines Part 2

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Chemical Reactions, CR 2: Energy in Reactions (HS), CR 2: Modeling Conservation of Mass (MS), CR 3: Evidence of Reactions (HS), CR 3: Testing Endo/Exothermic Reactions (MS), CR 4: Driving Reactions (HS), CR 5: Conservation of Mass (HS), Physical Science, S&P 4: Molecule Traits (HS), Structure & Properties of Matter, W 1: Graphing Waves (MS), W 1: Wave Relationships (HS), W 2: Digital Info (HS), W 2: Wave Behavior (MS), W 3: Digital vs Analog (MS), W 3: Modeling Electromagnetic Radiation (HS), W 5: Devices (HS), Waves & Electromagnetic Radiation

Beaming Simulated Space Ice

GwynneL.

Enantiomeric separation of complex organic molecules produced from irradiation of interstellar/circumstellar ice analogs(NOT OPEN ACCESS) SUMMARY: To simulate conditions in space and in asteroids and meteorites, scientists put simple gases (water, carbon dioxide, ammonia, and methanol) into a low temperature and low pressure chamber. Then, using UV light, they irradiated these gases (which at the… Continue reading Beaming Simulated Space Ice