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Nature

Chem

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Protons, Neutrons, and Electrons Practice Worksheet Fill in the blanks in the following worksheet. Please keep in mind that the isotope represented by each space may NOT be the most common isotope or the one closest in atomic mass to the value on the periodic table. Atomic symbol Atomic number Protons Neutrons Electrons Atomic mass B 6 11 24 31 37 39 89 29 35 43 100 Pb 207 102 70 89 225 Mo 53 81 206 100 159 No 261 Yb 172 106 159 Finding Protons, Neutrons, and Electrons of Elements

Metabolic rate in selected invertebrates.

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Practical 2: Metabolic rate in selected invertebrates. Ayman Shaik Abstract In this experiment was designed to determine the metabolic rate of three small invertebrates in relation to the animal?s body mass. The hypotheses for this experiment would be that the animal with the highest Oxygen consumption, would have the highest metabolic rate. The above hypothesis is accepted. The cockroach of the mass 1,07g, has an Oxygen consumption of 4,8ml and the highest metabolic rate of Introduction

The effect of UV light on bacteriophage

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Introduction: A bacteriophage is a virus which infects bacteria and have been of particular interest to scientists as vectors of horizontal gene transfer as well as the drivers of bacterial evolution, including as sources of diagnostic and genetic tools and novel therapeutic agents (Clokie et al., 2011). Just as with all viruses, bacteriophages are highly specific with regards to it?s host bacterium or it may only infect one species of bacteria (Kasman and Whitten, 2018).

Chemistry 101 exam 3 key

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Chemistry 101 - Exam II Name ______________________ 11 April 2018 Show all work for credit. State any assumptions made to solve a problem. Give all numerical answers with the correct number of significant figures. All answers in scientific notation must be in correct scientific notation (i.e., 6.022?1023 not 6.022E23 or 6.022e23). All instances of incorrect scientific notation will result in the loss of 3 points each. All numbers that require units should have the units written. All instances of numbers without units will result in the loss of 3 points each. 1. (32 points) Textbook Problem 7.107 ? Some of the butane, C4H10?, in a 200.0 L cylinder at 26.0 ?C is withdrawn and burned at a constant pressure in an excess of air. As a result, the

Chemistry 101 exam 2 key

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Chemistry 101 - Exam II Name ______________________ 26 October 2016 Show all work for credit. State any assumptions made to solve a problem. Give all numerical answers with the correct number of significant figures. All answers in scientific notation must be in correct scientific notation (i.e., 6.022?1023 not 6.022E23 or 6.022e23). All instances of incorrect scientific notation will result in the loss of 3 points each. All numbers that require units should have the units written. All instances of numbers without units will result in the loss of 3 points each. 1. (26 points) Cetane, C16H34, is a typical petrodiesel with a standard enthalpy of combustion of ?10 699.1 kJ mol?1. Methyl linoleate, C19H34O2, is a biodiesel with a standard enthalpy of

carbohydrate biofact sheet

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Carbohydrates: Revision Summary B io F actsheet January 1999 Number 39 1 Carbohydrates contain 3 elements: Carbon (C), Hydrogen (H) and Oxygen (O). Thus, if we remove water from carbohydrates, all that remains is carbon. Carbohydrates can be divided into 3 categories; monosaccharides, disaccharides and polysaccharides (Table 1). Monosaccharides and Disaccharides Monosaccharides and disaccharides are sugars. They all have the basic formula (CH2O)n and can be classified according to how many carbon atoms they contain. 3C = triose sugars e.g. glyceraldehyde C3H5O2 5C = pentose sugars e.g. ribose C5H10O5 6C = hexose sugars e.g. glucose C6H12O6 Formation of disaccharides - typical exam questions Common exam questions include:

Radioactivity and Nuclear Energy Notes

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Radioactive Decay Activation Energy (Ea): The threshold energy that must be overcome to produce a chemical reaction Electromagnetic Radiation: Radiant energy that exhibits wavelike behavior and travels through space at the speed of light in a vacuum Radioisotope: a radioactive isotope Many nuclei are radioactive Radioactive: Refers to a nucleus that spontaneously decomposes to form a different nucleus Over 85% of all known nuclides are radioactive Nuclear Equation: an equation representing radioactive decay Types of Radioactive (Nuclear) Decay (The spontaneous decomposition of a nucleus to form a different nucleus): Alpha Decay Alpha () particle shoots out from nucleus equivalent to helium-4 Beta Decay Beta () particle shoots out from nucleus equivalent to an electron Gamma Decay

Holt Earth Science Chapter 18, Section 18.1

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Water?s Changes of State Water exists in all 3 states of matter and is made of hydrogen and oxygen atoms. In all 3 stages of matter, these molecules are in constant motion (higher temperature: more movement). Difference between 3 states is the arrangement of the water molecules. A. Ice, Liquid Water, and Water Vapor Ice is made of water molecules held together by mutual molecular attractions.They form a tight, orderly network and don?t move - they vibrate in a fixed position. When ice is heated, the molecules vibrate more, and when the rate of movement increases enough, the bonds between the molecules break, resulting in melting In the liquid state, the molecules are still tightly packed but move fast enough to slide past each other (this causes liquid water to be fluid)

Holt Earth Science Chapter 17, Section 17.4

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Heating the Atmosphere A. What Happens to Incoming Solar Radiation? When radiation strikes an object, 3 things happen: some of the energy is absorbed by the object (converted to heat+temperature rises), some substances (water+air) are transparent to certain radiation wavelengths + transmit energy, and some radiation is bounced off the object without absorption/transmission. Reflection + scattering are responsible for redirected solar radiation. Out of the total solar radiation from the sun, 50% is absorbed by the land/sea, 20% is absorbed by the atmosphere/clouds, 5% is reflected from the land/sea surface, 5% is backscattered to space by the atmosphere, 20% is reflected by the clouds (in total, 30% is lost to space by reflection/scattering). B. Reflection and Scattering

Holt Earth Science Chapter 17, Section 17.3

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Earth-Sun Relationships The Sun is the source from almost all of the Earth?s weather and climate. Earth intercepts 12000000000 (one two-billionth) of all the energy given off by the sun (this is several hundred thousand times the energy generation of the US). Solar energy isn?t evenly distributed; the amount of energy varies with latitude, time of day, and season. Unequal heating of Earth creates winds and ocean currents, which transport heat to balance energy inequalities; the consequences of these processes are called weather. If the Sun died, global winds and currents would stop; but if the Sun shines, the winds will blow and weather will exist. Variations in solar heating are caused by the motions of the Earth relative to the Sun and variations in the Earth?s land-sea surface.

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