Explanation:
1. Watch a ship sail off to sea
Without being in the sky, it is impossible to see the curvature of the Earth. However, you can always see a demonstration of this if you visit a harbor or any place with a wide-open view of the water.
2. Watch a lunar eclipse
Solar eclipses get all the attention, but if you are able to catch a glimpse of a lunar eclipse, you can see evidence that the Earth is, indeed, round. Here's how it works: Earth passes between the moon and sun, so that the sun projects Earth’s shadow onto the Moon in the night sky
3. Climb a tree
Imagine a vast plane with but one tree smack in the middle. If the earth were flat, your vision would extend exactly as far while standing at the base of the tree as it would when at the top of the tree
4.Measure shadows across the country
Pick two locations that are some distance apart (at least a couple hundred miles from each other and on the same meridian). Grab two sticks or dowels (or other objects) of equal length, two tape measures, and a friend. Each of you will take one stick/dowel/object and one tape measure to your location, stick the object into the ground, and measure the shadow. (For accuracy, you should both take your measurements at the same time of day.)
5. Watch a sunset
Pick a nice spot from which you can watch a sunset (we'll call this point A). Ideally, you'd have a clear horizon in front of you, and behind you would be some sort of elevated point that you can quickly access (a hill, a building with at least two floors, or perhaps the aforementioned tree; we'll call this point B).
The blue graph is a horizontal translation of the red graph to the left. To horizontally translate the red graph for the function F(x) = x², we substitute x - h for x in the given function. Since the blue graph shifts one unit to the left, h is equal to -1.
Replacing F(x) with F(x - h), we get the equation G(x) of the blue graph:
F(x - h) = (x - (-1))² = (x + 1)² = G(x)
Therefore, the answer is D. G(x) = (x + 1)².
<span>The Greenhouse Effect:
The greenhouse effect is a natural phenomenon, which, helps maintain the
relatively stable, livable, range of temperatures that we find on
earth. To better understand how this phenomenon works, scientists have
used the analogy of the greenhouse. In a greenhouse, the glass (the
atmosphere) allows the radiant energy (light) of the sun to enter. As
the radiant energy strikes various plants, gases, and objects in the
greenhouse, they heat up. Their heat is then released back into the air
of the greenhouse as infrared radiation (heat). This infrared radiation
cannot travel through the glass and remains inside the greenhouse,
increasing the temperature inside the greenhouse. Temperatures can be
controlled, or kept in balance, by allowing some of the heat to remain
inside and some to be vented to the outside. Under normal conditions,
the earth's atmosphere works in a similar manner. Solar radiation enters
the atmosphere and heats up the air molecules, the surface of the
earth, buildings, plants, and other objects. These objects in turn,
radiate infrared radiation back out into the atmosphere, where some of
this radiation is absorbed by the greenhouse gases, and some is radiated
out into space. As some of the heat stays in the atmosphere and some
escapes into spaces, a balance is maintained allowing our planet to have
a relatively stable range of temperatures. Scientists believe that as
the greenhouse gases become more abundant in the atmosphere, due mainly
to the burning of fossil fuels, they retain more and more infrared
radiation, allowing less and less to escape into space, tipping the
balance toward heating up the atmosphere, resulting in a changing and
warmer climate, planet-wide. This is the accelerated greenhouse effect.
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Answer:
exosphere is the space outside the atmosphere
Explanation:
and this is because mcdonald's new chilli sauce is tasty
The Earth lithosphere thicker in the vicinity of trenches.