Answer:
Hi! I don't know exactly what you want, but I can give you some tips and points to use.
POTENTIAL ARGUMENT POINTS:
- Safety : it is easy and fast to call emergency services
- Time-saving : being able to surf the web without a computer saves a lot of time, and time is money!
- Communication : cell phones keep us in touch with friends and loved ones
-World Access : We have the whole world at our fingertips and can connect to people around the globe.
TIPS:
- DO NOT FORGET A COUNTER ARGUMENT!!! For example, if you were arguing for the safety aspect, you could say something like, "Although it can be argued that cell phone use can cause harm to teens, cell phones contribute to a lot of kids' and teens' safety because ....blah blah blah."
- USE STATISTICS! Teachers eat that stuff up. Do not be afraid to just throw them into a paragraph to back something up.
That is pretty much all I can think of rn. Good luck! :)
True.
Figures of speech such as metaphors, similes, and allusions go beyond the literal meanings of the words
Standard news stories are organized with the most important facts first. This is done so that people who only read the first couple of paragraphs get the gist of the story.
Also -- people tend to remember what they heard or read first -- when they are more alert and interested.
Answer:At a particular instant roughly 15 billion years ago, all the matter and energy we can observe, concentrated in a region smaller than a dime, began to expand and cool at an incredibly rapid rate. By the time the temperature had dropped to 100 million times that of the sun’s core, the forces of nature assumed their present properties, and the elementary particles known as quarks roamed freely in a sea of energy. When the universe had expanded an additional 1,000 times, all the matter we can measure filled a region the size of the solar system.
At that time, the free quarks became confined in neutrons and protons. After the universe had grown by another factor of 1,000, protons and neutrons combined to form atomic nuclei, including most of the helium and deuterium present today. All of this occurred within the first minute of the expansion. Conditions were still too hot, however, for atomic nuclei to capture electrons. Neutral atoms appeared in abundance only after the expansion had continued for 300,000 years and the universe was 1,000 times smaller than it is now. The neutral atoms then began to coalesce into gas clouds, which later evolved into stars. By the time the universe had expanded to one fifth its present size, the stars had formed groups recognizable as young galaxies.
Explanation:
