The Persian war and many battles between Greeks and Persians shaped the circumstances in which the sculpture was created. The Greeks were winning and feeling good about themselves.
<h3>What is the sculpture and its representation?</h3>
Apollo with Battling Lapiths and Centaurs is the name of the sculpture. It comes from the west pediment of the Temple of Zeus in Olympia and is not documented in the city's Archaeological Museum.
It was created approximately 460 BCE and hence belongs to the Classical period of Greek history.
The sculpture depicts the legendary narrative of the Lapiths and Centaurs' combat, in which centaurs who were invited to the Lapiths' wedding became incapable and kidnapped the bride Hippodameia.
The wedding guests were abused by Centaurs, and a conflict ensued, in which Lapiths triumphed. Apollo is seen here peering down on the combat and exhibiting his might with a swiftly extending arm.
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Answer:
Explanation:
<u>1. Calculate the depreciation per unit produced:</u>
Depreciation can be established in terms of time or units produced.
In this case, since you know the number of units of products produced during the second year of machine's use, your are interested in establishing deprectiation in terms of the number of units produced.
You are given:
- useful life: 210,000 units
- salvage value: $7,000
- purchase cost: $103,000
<em>Straight-line depreciation:</em>
- Depreciation = [purchase cost - salvage value] / (number of units)
- Depreciation = [$103,000 - $7,000] / (210,000 untis)
- Depreciation = $16/(35units)
<em />
<em><u>2) Calculate the depreciation of 33,600 units</u></em>
<em>During its second year the machine produces 33,600 units of product</em>; thus, the corresponding depreciation is:
- Depreciation = 33,600 units × $16/(35 units) = $15,360
The closer the star the larger The Parallax angle.
The primary mechanism driving the X-ray emission in traditional supergiant high mass X-ray binaries and supergiant fast X-ray transients is the accretion of stellar wind material by a compact object.
We present the first simulation of the fast and dense massive star wind accretion onto a neutron star in this paper, taking into account the effects of the centrifugal and magnetic inhibition of accretion ("gating") caused by the spin and magnetic field of the compact object.
We modeled the nonstationary radiatively generated wind of an O-B supergiant star using a radiative hydrodynamical code, and then we positioned a neutron star with a fixed magnetic field and spin period at a specific distance from the massive companion.
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Answer:
A. Orthographic mode
Explanation:
Orthographic mode presents an orthographic projection that shows us detailed proportions of the object. It is used to present the three-dimensional proportions in two-dimensional settings.
The lines are parallel and the model presents the parallel projection. <u>This means that the lines which are parallel never cross, unlike in the perspective mode. </u>Using both of these and switching between them helps you get a better vision of the object while modeling it.
