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Mice21 [21]
3 years ago
6

Which statement best explains the relationship between satellite technology and the Internet?

History
2 answers:
trasher [3.6K]3 years ago
5 0
Pretty sure it's A because you can cross out the other three but I think it's A
expeople1 [14]3 years ago
5 0

Answer:

<h2><em>D. People in less-developed nations use satellites to access the Internet, greatly increasing the number of Internet users.</em></h2>

Explanation:

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Movement of a group of people
Dimas [21]

The movement of a group of people is called migration.


6 0
4 years ago
Beginning in the nineteenth century, industrializing lands experienced a social change known as the demographic transition when?
natta225 [31]

Answer:

When fertility rates fell.

Explanation:

The demographic transition consists in the change of the demographic profile of the population of a city or country. Demographic transitions are usually triggered by industrialization and urbanization.

Pre-industrial, agrarian societies have a demographic profile of very high fertility rates, very high child mortality, and very low life expectancy.

In other words, in agrarian societies, women have many children, only a few of those children survive into adulthood, and because life expenctacy is low, the average person is young, and there are very few old people.

As the agrarian society becomes more industrial and more urban, women start having fewer children, and more of those children survive, because the increased wealth generated by the industrial economy allows better medical care and nutrition.

Life expectancy rises as well, leading to an general aging of society. For example, in Japan, a highly industrialized, and very urban country, the average age is 46 years.

5 0
3 years ago
The Frank's were allies with Rome.<br> 1.true<br> 2.false
Lesechka [4]
Im gunna go with true

6 0
3 years ago
Read 2 more answers
13. What movement
Alinara [238K]

Answer:

i think you're talking about the propaganda the US had going around about Japanese immigrants being seen as evil or untrustworthy. if not could you please put options for the answer?

Explanation:

5 0
3 years ago
1 plus 1 is 2 very easy
Bumek [7]

Answer:

indeed it is

Explanation:

Whitehead and Russell's Principia Mathematica is famous for taking a thousand pages to prove that 1+1=2. Of course, it proves a lot of other stuff, too. If they had wanted to prove only that 1+1=2, it would probably have taken only half as much space.

Principia Mathematica is an odd book, worth looking into from a historical point of view as well as a mathematical one. It was written around 1910, and mathematical logic was still then in its infancy, fresh from the transformation worked on it by Peano and Frege. The notation is somewhat obscure, because mathematical notation has evolved substantially since then. And many of the simple techniques that we now take for granted are absent. Like a poorly-written computer program, a lot of Principia Mathematica's bulk is repeated code, separate sections that say essentially the same things, because the authors haven't yet learned the techniques that would allow the sections to be combined into one.

For example, section ∗22, "Calculus of Classes", begins by defining the subset relation (∗22.01), and the operations of set union and set intersection (∗22.02 and .03), the complement of a set (∗22.04), and the difference of two sets (∗22.05). It then proves the commutativity and associativity of set union and set intersection (∗22.51, .52, .57, and .7), various properties like &#x03B1;&#x2229;&#x03B1;=&#x03B1;" role="presentation" style="display: inline; font-style: normal; font-weight: normal; line-height: normal; font-size: 16px; text-indent: 0px; text-align: left; text-transform: none; letter-spacing: normal; word-spacing: normal; overflow-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; padding: 0px; margin: 0px; position: relative;">α∩α=αα∩α=α (∗22.5) and the like, working up to theorems like ∗22.92: &#x03B1;&#x2282;&#x03B2;&#x2192;&#x03B1;&#x222A;(&#x03B2;&#x2212;&#x03B1;)" role="presentation" style="display: inline; font-style: normal; font-weight: normal; line-height: normal; font-size: 16px; text-indent: 0px; text-align: left; text-transform: none; letter-spacing: normal; word-spacing: normal; overflow-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; padding: 0px; margin: 0px; position: relative;">α⊂β→α∪(β−α)α⊂β→α∪(β−α).

Section ∗23 is "Calculus of Relations" and begins in almost exactly the same way, defining the subrelation relation (∗23.01), and the operations of relational union and intersection (∗23.02 and .03), the complement of a relation (∗23.04), and the difference of two relations (∗23.05). It later proves the commutativity and associativity of relational union and intersection (∗23.51, .52, .57, and .7), various properties like &#x03B1;&#x2229;&#x02D9;&#x03B1;=&#x03B1;" role="presentation" style="display: inline; font-style: normal; font-weight: normal; line-height: normal; font-size: 16px; text-indent: 0px; text-align: left; text-transform: none; letter-spacing: normal; word-spacing: normal; overflow-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; padding: 0px; margin: 0px; position: relative;">α∩˙α=αα∩˙α=α (∗22.5) and the like, working up to theorems like ∗23.92: &#x03B1;&#x2282;&#x02D9;&#x03B2;&#x2192;&#x03B1;&#x222A;&#x02D9;(&#x03B2;&#x2212;&#x02D9;&#x03B1;)" role="presentation" style="display: inline; font-style: normal; font-weight: normal; line-height: normal; font-size: 16px; text-indent: 0px; text-align: left; text-transform: none; letter-spacing: normal; word-spacing: normal; overflow-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; padding: 0px; margin: 0px; position: relative;">α⊂˙β→α∪˙(β−˙α)α⊂˙β→α∪˙(β−˙α.

4 0
3 years ago
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