What is a characteristic of expressionist wassily kandinsky's improvisation 31?

When the pressure is decreased from [tex]100.0 kPa[/tex] to [tex]90.0 kPa[/tex] at constant temperature, the volume of the gas in the balloon increases to [tex]3.67 L[/tex].

To solve this problem, we can use Boyle's Law, which states that for a given mass of gas at constant temperature, the volume of the gas is inversely proportional to its pressure. Mathematically, this can be expressed as:

[tex]\[ P_1V_1 = P_2V_2 \][/tex]

where [tex]\( P_1 \)[/tex] and [tex]\( V_1 \)[/tex] are the initial pressure and volume, and [tex]\( P_2 \)[/tex] and [tex]\( V_2 \)[/tex] are the final pressure and volume, respectively.

Given:

Initial volume [tex]\( V_1 = 3.3 \) L[/tex]

Initial pressure [tex]\( P_1 = 100.0 \) kPa[/tex]

Final pressure [tex]\( P_2 = 90.0 \) kPa[/tex]

Temperature is constant

We want to find the final volume [tex]\( V_2 \)[/tex]. Rearranging Boyle's Law to solve for [tex]\( V_2 \)[/tex], we get:

[tex]\[ V_2 = \frac{P_1V_1}{P_2} \][/tex]

Substituting the given values:

[tex]\[ V_2 = \frac{100.0 \text{ kPa} \times 3.3 \text{ L}}{90.0 \text{ kPa}} \][/tex]

[tex]\[ V_2 = \frac{330}{90} \text{ L} \][/tex]

[tex]\[ V_2 = 3.67 \text{ L} \][/tex]

The stable neutron-proton ratio in lighter elements is about 1:1, exemplified by Carbon-12. As element atomic numbers increase, the ratio tends to 1.5:1 to maintain nuclear stability, noticeable in heavier elements like lead-206. All elements with Z > 83 are inherently unstable and radioactive.

Among atoms with lower atomic numbers, the most stable nuclei typically have a neutron-proton ratio that approximates 1:1. This means that in lighter elements, the number of neutrons and protons are nearly equal, contributing to the stability of the nucleus.

A classic example is Carbon-12, which has six protons and six neutrons. As we examine heavier elements, the stable neutron-proton ratio increases, which can be attributed to the need to counterbalance the increased electrostatic repulsion between protons within the nucleus. For instance, heavy elements such as lead-206 have a neutron-proton ratio of about 1.5:1, with 124 neutrons to 82 protons.

Regardless of the number of neutrons, it should be noted that all elements with atomic number (Z) greater than 83 are unstable and radioactive. The balance in neutron-proton ratio is crucial as it determines the type of radioactive decay a nuclide may undergo, such as positron emission or electron capture, especially if the ratio is not within the stable range.

Answer: [tex]1s^22s^22p^63s^13p^2[/tex].

Explanation:

Electronic configuration is defined as the distribution of electrons in the energy levels around an atomic nucleus.

Atomic number helps in determining the electronic distribution  of an atom. We write electronic configuration according to Aufbau's principle in which shells are arranged in increasing energy levels.

Aluminium (Al) is a p block element and its atomic number is 13.

Electronic configuration of aluminium is [tex]1s^22s^22p^63s^23p^1[/tex].

Excite state is achieved when the electron moves to a higher energy level.The 3s electron moves to 3p orbital so that it can form three bonds.

Thus Electronic configuration of aluminium in an excited state is [tex]1s^22s^22p^63s^13p^2[/tex].

Answer:

Option c

Explanation:

Atomic number of helium is 2.

Electronic configuration of He = [tex]1s_2[/tex]

First energy shell of an atom is known as K shell. It has only one sub shell 's sub shell'.

K shell or energy level can accommodate maximum of 2 electrons. Helium has 2 electrons and these two electrons are filled in K shell. So, atom of helium has a full energy level.

Elements having full energy level or eight electrons in their valence shell is stable and therefore chemically inactive or inert.

As outer shell of helium is full, so it is chemically inactive.

Final answer:

To find the number of moles of neon in 14.3 L at STP, divide the volume by the molar volume of 22.4 L. The result is 0.638 moles of neon.

Explanation:

To determine the number of moles of neon that occupy a volume of 14.3 L at STP (standard temperature and pressure), you use the concept of molar volume. At STP, a mole of any gas occupies 22.4 L. Therefore, you can calculate the moles of neon using the volume and the molar volume as a conversion factor.

The formula for this calculation is:

Moles of neon = Volume of neon (L) / Molar volume (L/mol)

So as an equation:

Moles of neon = 14.3 L / 22.4 L/mol

This gives us:

Moles of neon = 0.638 moles

This is a conversion between moles and gas volume at STP and is a fundamental principle in chemistry.

Final answer:

The molality of a glucose solution with 257 g of glucose dissolved in 1.62 L of water is 0.880 mol/kg. This is determined by converting the mass of glucose to moles and then dividing by the mass of the water in kilograms.

Explanation:

To calculate the molality of the glucose solution, we need to know the amount of solute (glucose) in moles and the mass of the solvent (water) in kilograms. The molecular weight of glucose (C6H12O6) is 180.16 g/mol.

First, convert the mass of glucose to moles:

(257 g glucose) / (180.16 g/mol) = 1.426 mol glucose

Next, since the density of water is assumed to be 1.00 g/mL, we use that to find the mass of the water:

(1.62 L water) (1000 mL/L) (1.00 g/mL) = 1620 g water = 1.62 kg water

Now, we can calculate the molality (m):

m = mol solute / kg solvent = 1.426 mol / 1.62 kg = 0.880 mol/kg

The molality of the glucose solution is 0.880 mol/kg.

 There are 2 classifications of waves according to the media of propagation.

i think it is B) because Sound waves move by replacing one particle with another. Sound waves require a medium to propagate, or move. Light and electromagnetic waves do not require a medium. Electrostatic are not a type of wave.

hope this helps

AX5E0 - trigonal bipyramidal - zero lone pairs;
AX4E1 - seesaw - 1 lone pair;
AX3E2 - T-shaped - 2 lone pairs;
AX2E3 - linear - 3 lone pairs;

The only option that matches is trigonal bipyramidal.

Answer: it decreases the activation energy for a chemical reaction.

Explanation:

Activation energy is the extra energy that must be supplied to reactants in order to cross the energy barrier and thus convert to products.

A catalyst is a substance which increases the rate of a reaction by taking the reaction through a different path which involves lower activation energy and thus more molecules can cross the energy barrier and convert to products.

The catalyst itself does not take part in the chemical reaction and is regenerated as such at the end.

A catalyst plays a key role in reducing the activation energy for a chemical reaction by providing an alternative reaction pathway that requires less energy. Because of this reduction in energy, the reaction can proceed more rapidly. The catalyst itself is not consumed in the reaction and can be used again.

A catalyst works by providing an alternative reaction pathway that requires less energy, thus decreasing the activation energy for a chemical reaction. In other words, it helps to speed up the reaction by lowering the energy needed for it to occur.

Let's take the example of a hypothetical reaction, 'A + B → AB'. Without a catalyst, this reaction might require a high activation energy, prohibiting the reaction from occurring under typical circumstances. However, with a catalyst, the reaction might proceed with an intermediate step 'A+C → AC → AB + C'. In this example, 'C' is the catalyst and 'AC' is the intermediate step; each individual step needs less energy than the original reaction, thus lowering the overall activation energy.

It's important to note that catalysts do not change the total energy of the reactants or the product; they just make it quicker for the reaction to reach the product stage. After the reaction, the catalyst is not consumed and can be used again for the same reaction.

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To convert 115.0 g of ice at 0.0 ∘C to liquid water at 32 ∘C, 53.821 kJ of energy is required.

To determine how many kilojoules are required to convert 115.0 g of ice at 0.0 ∘C to liquid water at 32 ∘C, we need to account for both the phase change and the temperature increase.

Therefore, 53.821 kJ are required to convert 115.0 g of ice at 0.0 ∘C to liquid water at 32 ∘C.

Final answer:

To calculate the total change in mass for the fusion of two deuterium atoms into helium, we use Einstein's equation E = Δmc^2, which results in a mass change of approximately 4.258 × 10^-29 kg.

Explanation:

When two atoms of 2H deuterium fuse to form one atom of 4He helium, the energy evolved is 3.83 × 10^-12 joules. To find the total change in mass (Δm) for this reaction, we use Einstein's equation E = Δmc^2, where E is the energy released, c is the speed of light in a vacuum (approximately 3 × 10^8 m/s), and Δm is the change in mass. By rearranging the equation to Δm = E/c^2 and substituting the given values, we get Δm = (3.83 × 10^-12 joules) / (9 × 10^16 m^2/s^2) which results in a change in mass of approximately 4.258 × 10^-29 kg.

Answer:

Gravity helped to hold things in orbit and create the planets.

Explanation:

Scientist believe that the solar system started in a similar way to stars, from a nebula. They say that the it was a cloud of dust and gas called a nebula that contained mostly hydrogen and helium leftover from the "Big Bang"(which I have my arguments about.) They also say there were heavier elements. Gravity caused the nebula to shrink. As the nebula became smaller it had a rotation. As it got smaller it began to spin faster. The planets were formed by materials cooling off. As they were cooling off they began to clump together. Clumps collided with each other to make a bigger clump. Larger clumps would attract smaller clumps with their gravitational pull. Eventually the clumps started to form the planets and moons in today's solar system.

Answer:

350 mL

Explanation:

Given:

concentration of stock solution of HCl =6.00 M

Volume of stock solution of HCl = 175 mL

concentration of required solution = 2.00 M

total volume of required solution = to be determined

This is problem of dilution. We have to determine the total volume of required solution to be made, from the given stock solution.

We will use

M₁V₁=M₂V₂

Where

M₁=concentration of stock solution

V₁= volume of stock solution

M₂=concentration of required solution

V₂=volume of required solution

Putting values

6X175=2XV₂

V₂=525 mL

so total volume of required solution formed will be 525 mL

We have already 175 mL of solution in it. The water need is difference of these two volume.

water added = 525-175= 350 mL

Answer:

It must be vaporized is the answer

Explanation:

took thest

Final answer:

The bond angle in ozone is not exactly 120° due to electron pair repulsion and resonance structures, which cause deviations from the expected angle as explained by valence bond theory and hybridization.

Explanation:

The o-to-o-to-o bond angle in an ozone (O3) molecule is not exactly 120° because of the effects of electron pair repulsion and the molecule's resonance structure. Unlike a perfect equilateral triangle where angles are 120° due to identical bonding situations, in ozone, there are lone electron pairs on the central oxygen atom that push against the bonding pairs, causing a deviation from the expected angle. Additionally, the resonance structures contribute to an unequal distribution of electron density, further altering the bond angles.

Valence bond theory and hybridization explain that bonding in such molecules deviates from simple p-orbital overlap that would predict a 120° angle. Instead, these molecules adopt shapes that minimize the repulsion between electron pairs, which in case of water, leads to a bond angle of 104.5°, despite predictions of a 90° angle from unhybridized p-orbitals.

Answer:

I think the answer is Protons.

Protons are the positive subatomic particles in an atom. They reside in the nucleus of the atom and their number determines the type of the element. Normally, atoms maintain a balance of protons and electrons, resulting in a neutral overall charge.

In an atom, the positive subatomic particles are called protons. These particles are located in the nucleus, or center, of the atom. Protons are one of three main subatomic particles in an atom, along with neutrons (which have no charge) and electrons (which have a negative charge).

The number of protons in an atom's nucleus determines the type of element it is. For example, an atom with 1 proton is hydrogen, an atom with 6 protons is carbon, and so on. The balance of protons and electrons in an atom determines the atom's overall charge. Normally, atoms have an equal number of protons and electrons, so their charges balance out, resulting in a neutral charge overall.

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