Physics, 29.02.2020 04:15 carolyntowerskemp

The_method is the safest turning technique to use as it does not
expose your hands to the airbag's deployment area.

A. push/pull
B. secured turn
C. hand over hand
D. three point

Answers: 3

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Answers

Answer from: yoongnzl

The correct answer is A. The push/pull also known as hand-to-hand technique

Explanation:

A. PUSH/ PULL STEERING (HAND-TO-HAND)

This is the correct answer. The push/pull turn is also known as the hand-to-hand can be done such that your hands never cross over the steering wheel. Since the hands do not cross over the steering wheel, there is less chance of an injury to the face, hands or arms induced by your hands or arms in the event of a frontal crash due to an airbag. This technique has three methods;

The 10 and 2 position

The 9 and 3 position

The 8 and 4 position

Of the three methods, the 9 and 3 position is the preferred method of steering. Two and 10 o’clock is not recommended because it can be dangerous in vehicles with smaller steering wheels and equipped with airbags.

B. SECURE TURN

This option is wrong. It is not safe as regards to airbag deployment

C. HAND-OVER-HAND STEERING

This option is wrong. This method of steering is used when turning at low speeds with limited visibility at an intersection or when parking the vehicle or recovering from a skid. In hand-over-hand steering, the driver’s arms will pass across the airbag deployment zone. In the event of an airbag deployment, the driver arms will be thrown back into his face.

D. THE THREE POINT TURN

This option is wrong. It is a method you use when you want to execute a U-turn and you can only do it in limited place when the road is free of traffic. It should not be done near a main road, near a short curve, near an intersection or near the crest of a hill

Answer from: Quest

you go to your settings preference and in the end youll see sth that says "i want to delete my acc" click on it and u'll acc will be deleted but u have to wait.

Answer from: Quest

sequence is a continuous and distinctive band of stars that appears on plots of stellar color versus brightness. these color-magnitude plots are known as hertzsprung–russell diagramsafter their co-developers, ejnar hertzsprungand henry norris russell. stars on this band are known as main-sequence stars or dwarf stars. these are the most numerous true stars in the universe, and include the earth's sun.after condensation and ignition of a star, it generates thermal energy in its dense core region through nuclear fusion of hydrogen into helium. during this stage of the star's lifetime, it is located on the main sequence at a position determined primarily by its mass, but also based upon its chemical composition and age. the cores of main-sequence stars are in hydrostatic equilibrium, where outward thermal pressure from the hot core is balanced by the inward pressure of gravitational collapse from the overlying layers. the strong dependence of the rate of energy generation on temperature and pressure to sustain this balance. energy generated at the core makes its way to the surface and is radiated away at the photosphere. the energy is carried by either radiation or convection, with the latter occurring in regions with steeper temperature gradients, higher opacity or both.the main sequence is sometimes divided into upper and lower parts, based on the dominant process that a star uses to generate energy. stars below about 1.5 times the mass of the sun (1.5 m☉) primarily fuse hydrogen atoms together in a series of stages to form helium, a sequence called the proton–proton chain. above this mass, in the upper main sequence, the nuclear fusion process mainly uses atoms of carbon, nitrogen and oxygen as intermediaries in the cno cycle that produces helium from hydrogen atoms. main-sequence stars with more than two solar masses undergo convection in their core regions, which acts to stir up the newly created helium and maintain the proportion of fuel needed for fusion to occur. below this mass, stars have cores that are entirely radiative with convective zones near the surface. with decreasing stellar mass, the proportion of the star forming a convective envelope steadily increases. main-sequence stars below 0.4 m☉undergo convection throughout their mass. when core convection does not occur, a helium-rich core develops surrounded by an outer layer of hydrogen.in general, the more massive a star is, the shorter its lifespan on the main sequence. after the hydrogen fuel at the core has been consumed, the star evolves away from the main sequence on the hr diagram, into a supergiant, red giant, or directly to a white dwarf.