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Kyousei High School RP 2~
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on 2008-01-24 17:49:37 |
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Previous Thread read rules and everything HERE |
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Re: Kyousei High School RP 2~
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on 2008-01-24 19:32:05 (edited 2008-01-24 19:38:52)
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@miko thanks for making the 2nd thread! [class 4-B student, username: kira7392 char name: Hiiragi Akira] [class 4-B] *sits down* Akira: weird...i said something that's not what i thought i wanted to say...hope it's not an illusion...  |
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Re: Kyousei High School RP 2~
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on 2008-01-24 19:42:18 |
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@thank you Miko ^^ [class 4-B] Ikuto: what do you mean weird Akira? I barely know what you just said dude...are you one of those advance students ._.? 
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Re: Kyousei High School RP 2~
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on 2008-01-25 05:34:37 |
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[Class 4A Student; Username: ayu_mia6; Character Name: Mia] *Hagino stopped and helped Mia up. She stared at the corpse* Now why would that be on you foot?! *She laughed and look at Mia* You O.K.? *reaches her hand* Mia: *laughs* I'm okay, we should report this body to our PE teacher when we come back... *jogs again*   |
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Re: Kyousei High School RP 2~
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on 2008-01-25 05:51:51 |
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[Class 4b Student, Username: kabluam, Character name: Zlatan Kachizky] saki~ Uwaaahhhhhh... Akira's answer was amazing. I don't get any of this.. Ack. That means. FAIL. x.x; -saki stares at Zlatan- Saki~ Well, at least I'm not the only one who's confused about this heh..heh.. *suddenly zlatan shivers, he feels like someone watching over him. then he looks back. as he sees saki is staring at him, he quickly turns his head to the board* zlatan: what the.... what is exactly she is doing *then zlatan looks at his book and convinced himself* zlatan: nah, she just looking at the board [note although zlatan is tall, he sits on the front row]  |
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Re: Kyousei High School RP 2~
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on 2008-01-25 10:57:25 |
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[Class 4-A, Username: icefiregal123, Character: Hagino] Mia: *laughs* I'm okay, we should report this body to our PE teacher when we come back... *jogs again* *Hagino started to job again* Yea we should..I still don't see why it would be attatched to you.  |
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Re: Kyousei High School RP 2~
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on 2008-01-25 11:06:57 |
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-Hospital- Aki: so i've been confined again in a hospital Butler: Aki-sama i suggest you should rest some more Aki: but i want to see that girl again  |
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Re: Kyousei High School RP 2~
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on 2008-01-25 13:07:17 (edited 2008-01-25 13:08:08)
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[4-B] *suddenly zlatan shivers, he feels like someone watching over him. then he looks back. as he sees saki is staring at him, he quickly turns his head to the board* zlatan: what the.... what is exactly she is doing *then zlatan looks at his book and convinced himself* zlatan: nah, she just looking at the board Saki~ Eh? What was that about? *strains to see the board* Ack. He is blocking the board.. Gawsh.. I hate being short. *falls out of her desk* Ahhh! -on the floor- Saki~ Owwie ow ow.. That huuuurt, gah, clumsy.  |
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Re: Kyousei High School RP 2~
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on 2008-01-25 13:49:02 |
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[Classroom 4-B] Saki~ Eh? What was that about? *strains to see the board* Ack. He is blocking the board.. Gawsh.. I hate being short. *falls out of her desk* Ahhh! -on the floor- Saki~ Owwie ow ow.. That huuuurt, gah, clumsy. Ikuto: Are you okay Saki? *reaches out and help her get back up* there you go *goes back sitting down and looks up what the teacher said and takes note of what the other students said* so many information.
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Re: Kyousei High School RP 2~
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on 2008-01-26 00:19:49 (edited 2008-01-26 00:20:14)
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[class 4-B student, username: kira7392 char name: Hiiragi Akira] [class 4-B] Ikuto: what do you mean weird Akira? I barely know what you just said dude...are you one of those advance students ._.? Akira: well...actually i didn't really know much detail...but i said it somehow...it was like...somebody else answered that...and i can't be an advance student...it's just...no way. *meanwhile* Saki: Eh? What was that about? *strains to see the board* Ack. He is blocking the board.. Gawsh.. I hate being short. *falls out of her desk* Ahhh! Saki: Owwie ow ow.. That huuuurt, gah, clumsy. Ikuto: Are you okay Saki? *reaches out and help her get back up* there you go Akira: Are you hurt anywhere Saki? |
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Re: Kyousei High School RP 2~
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![](http://i49.tinypic.com/2af097a.jpg")
on 2008-01-27 04:22:59 |
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[Class 4-A,username:kemg, char name:Kenji DelaCroix] ooc:The return of the trouble maker..*dun dun dun* heheh..What time is it in the RP? __________________________________________________________________ [Dorm] Kenji was typing on his PC on an RP forum(XD) while cutting class. "Hmm..I guess its time to eat.." he said to himself "Been gone for a while now..Somebodies bound to notice..." He turned off the PC and started to get his school things and proceeded to his next class.  |
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Re: Kyousei High School RP 2~
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on 2008-01-27 04:24:09 |
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10:45 AM! Yuuka : Thank you Ms. Tomokazu. Let's continue. Gravitation is a natural phenomenon by which all objects with mass attract each other. In everyday life, gravitation is most commonly thought of as the agency that gives objects weight. Weight, as stated by Ueki, is how one is and is computed by mass times the strength of gravity on your spot so it depends on where you are, or a measurement of the gravitational force acting on an object. While mass is the amount of matter in an object. That is the difference between Mass and weight. Now, let's tackle the history of the Gravitational theory. In the 4th century BC, the Greek philosopher Aristotle believed that there is no effect or motion without a cause. The cause of the downward motion of heavy bodies, such as the element earth, was related to their nature, which caused them to move downward toward the center of the universe, which was their natural place. Conversely, light bodies such as the element fire, move by their nature upward toward the inner surface of the sphere of the Moon. Thus in Aristotle's system heavy bodies are not attracted to the earth by an external force of gravity, but tend toward the center of the universe because of an inner gravitas or heaviness. Then, in the middle ages, The Indian astronomer Brahmagupta, in his Brahmasphuta Siddhanta, recognized gravity as a force of attraction. Brahmagupta followed the heliocentric solar system of gravitation, earlier developed by Aryabhata in 499, and understood that there was a force of attraction between the Sun and the Earth. Now, what is the meaning of Brahmasphuta Siddhanta and what is the meaning of heliocentric? Akira : I'll answer that. *stands up* Brahmasphuta-siddhanta (The Opening of the Universe) is the main work of Brahmagupta, written in the year 628. hmm...it contains some remarkably advanced ideas, including a good understanding of the mathematical role of zero, rules for manipulating both negative and positive numbers, a method for computing square roots, methods of solving linear and some quadratic equations, and rules for summing series, Brahmagupta's identity, and the Brahmagupta’s theorem. The book was written completely in verse. *stops* then...heliocentrism, that come from the Greek (Helios = Sun and kentron = Center) is the theory that the sun is at the center of the Universe and/or the Solar System. I can only think of those at the moment...*sits down* Yuuka : Very good, thank you Mr. Akira. The class became wild and the other students kept on chatting. Yuuka pretended not to care, she just continued discussing. Yuuka : We will study about heliocentrism in the latter pat of our discussion. So, modern work on gravitational theory began with the work of Galileo Galilei in the late 16th century and early 17th century. In his famous (though probably apocryphal) experiment dropping balls from the Tower of Pisa, and later with careful measurements of balls rolling down inclines, Galileo showed that gravitation accelerates all objects at the same rate. This was a major departure from Aristotle's belief that heavier objects are accelerated faster. (Galileo correctly postulated air resistance as the reason that lighter objects may fall more slowly in an atmosphere.) Galileo's work set the stage for the formulation of Newton's theory of gravity. Ms. Yamada, since you and your friends are getting noisy, can you please tell the class what is Isaac Newton's universal theory of gravitation?  |
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Re: Kyousei High School RP 2~
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on 2008-01-27 05:54:54 |
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[Class 4b Student, Username: kabluam, Character name: Zlatan Kachizky] *zlatan straightens his sitting position* Saki~ Eh? What was that about? *strains to see the board* Ack. He is blocking the board.. Gawsh.. I hate being short. *falls out of her desk* Ahhh! -on the floor- Saki~ Owwie ow ow.. That huuuurt, gah, clumsy. *as he hears the a noise from behind, zlatan looks behind. there he sees saki is on the floor, while ikuto and akira helps her* zlatan: bah... girls are always the main source of noises and troubles *then zlatan turns his head to ms yuuka and starts listening* Yuuka : We will study about heliocentrism in the latter pat of our discussion. So, modern work on gravitational theory began with the work of Galileo Galilei in the late 16th century and early 17th century. In his famous (though probably apocryphal) experiment dropping balls from the Tower of Pisa, and later with careful measurements of balls rolling down inclines, Galileo showed that gravitation accelerates all objects at the same rate. This was a major departure from Aristotle's belief that heavier objects are accelerated faster. (Galileo correctly postulated air resistance as the reason that lighter objects may fall more slowly in an atmosphere.) Galileo's work set the stage for the formulation of Newton's theory of gravity. Ms. Yamada, since you and your friends are getting noisy, can you please tell the class what is Isaac Newton's universal theory of gravitation? zlatan: who, glad that question doesn't come to me... |
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Re: Kyousei High School RP 2~
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on 2008-01-27 13:52:10 (edited 2008-01-27 13:55:18)
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[character name: Saki Yamada, class: 4-B, username: sakura_kiss94] [4-B] -Stands up- Saki~ Gawsh.. Thanks Ikuto... Nah, I'm fine Akira. Yuuka : We will study about heliocentrism in the latter pat of our discussion. So, modern work on gravitational theory began with the work of Galileo Galilei in the late 16th century and early 17th century. In his famous (though probably apocryphal) experiment dropping balls from the Tower of Pisa, and later with careful measurements of balls rolling down inclines, Galileo showed that gravitation accelerates all objects at the same rate. This was a major departure from Aristotle's belief that heavier objects are accelerated faster. (Galileo correctly postulated air resistance as the reason that lighter objects may fall more slowly in an atmosphere.) Galileo's work set the stage for the formulation of Newton's theory of gravity. Ms. Yamada, since you and your friends are getting noisy, can you please tell the class what is Isaac Newton's universal theory of gravitation? Saki~ Owh.. Ah! Gomen teacher! Issac Newton's universal theory of gravitation is that every point mass attracts every other point mass by a force pointing along the line intersecting both points. The force is proportional to the product of the two masses and inversely proportional to the square of the distance between the point masses: F=G(m1 x m2)/r² where * F is the magnitude of the gravitational force between the two point masses, * G is the gravitational constant, * m1 is the mass of the first point mass, * m2 is the mass of the second point mass, * r is the distance between the two point masses. Please tell me that was right... T 3T; *pokes Zlatan* You're too tall to be in the front row.. I can't see >w>; |
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Re: Kyousei High School RP 2~
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on 2008-01-27 22:04:35 |
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[Class 4A Student; Username: ayu_mia6; Character Name: Mia] *Hagino started to jog again* Yea we should..I still don't see why it would be attatched to you. Mia: I dunno... *looks back* but the worst part isthe corpse is standing and following us kyaaaaaaa! *runs faster* >.< |
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Re: Kyousei High School RP 2~
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on 2008-01-28 04:34:32 (edited 2008-01-28 04:36:55)
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@miko ahahahaha... (Hope I still remember what to do XDDD) PE Teacher kicks corpse and head falls off... PE Teacher : Stop worrying about that corpse and run! Run! Run! Run! *checks clock* PE Teacher : OK! That's enough! Rest for 30 seconds and then, tell me if you want to try for the standing long jump!  |
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Re: Kyousei High School RP 2~
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OOC: Sorry that i've been inactive for so long, my mum went for an operation and i had to find a parttime job, gomen!! >.< Hope my character hasn't been deleted for being inactive... Class 4-C student, username: invisible0403 character name: Saya Yamada [4-C] -------------------------------------------------------- Renma : *Is Writing something on the Board* Phew... Finally... I Managed to get into the class... *Put down the marker, He Look back and he Look at his writing* The writing Says "Values Education Class" So, Class... Firstly.. I Wanted to know.. What do you know about Values Education? *Renma Look around, and He sees that There're a lot of Confused face and also, He noticed that Few of them are Hesitating to raise their Hand and answer the question, Looking at them, he smile* I Won't Reduce your Grade to F Or Fail you on this class if you're wrong, So Let's hear some of your Answers shall we? Anyone wants to Volunteer? -------------------------------------------------------- Saya: *snapped out from daydreaming* (Values Ed? The hell is that? Somebody had better answer it before he calls me...) *looks around and notice noone dares to make response* *sighs* How about giving us some clues, sensei? |
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Re: Kyousei High School RP 2~
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on 2008-01-29 10:59:22 (edited 2008-01-29 11:13:03)
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[Class 4-B Student, Usersname:jc-kun, Character name : Ikuto Tohoin] Yuuka : We will study about heliocentrism in the latter pat of our discussion. So, modern work on gravitational theory began with the work of Galileo Galilei in the late 16th century and early 17th century. In his famous (though probably apocryphal) experiment dropping balls from the Tower of Pisa, and later with careful measurements of balls rolling down inclines, Galileo showed that gravitation accelerates all objects at the same rate. This was a major departure from Aristotle's belief that heavier objects are accelerated faster. (Galileo correctly postulated air resistance as the reason that lighter objects may fall more slowly in an atmosphere.) Galileo's work set the stage for the formulation of Newton's theory of gravity. Ms. Yamada, since you and your friends are getting noisy, can you please tell the class what is Isaac Newton's universal theory of gravitation? Saki~ Owh.. Ah! Gomen teacher! Issac Newton's universal theory of gravitation is that every point mass attracts every other point mass by a force pointing along the line intersecting both points. The force is proportional to the product of the two masses and inversely proportional to the square of the distance between the point masses: F=G(m1 x m2)/r² where * F is the magnitude of the gravitational force between the two point masses, * G is the gravitational constant, * m1 is the mass of the first point mass, * m2 is the mass of the second point mass, * r is the distance between the two point masses. Please tell me that was right... T 3T; *pokes Zlatan* You're too tall to be in the front row.. I can't see >w>; Ikuto: well you are right Saki, but here's my answer to that question Ms.Yuuka *ahem* The equation for the force of gravity for all objects relatively close to the Earth is: F = mg where * F is the force pulling objects toward the Earth; it is also the weight of the object * m is the mass of the object * g is the acceleration due to gravity; this number is a constant for all masses of matter * mg is the product of m times g. The weight of an object is the measurement of the force of gravity on that object. You weigh something on a scale, according to the force that the Earth pulls it down. Thus the weight is actually the force of gravity on that object: w = mg where * w is weight * m is mass * g is acceleration due to gravity which makes Newton realized that in the planet-Sun system, the planet does not orbit around a stationary Sun. Instead, Newton proposed that both *brings out an Apple and a Orange for a little show and tell ^^;* the planet (the apple) and the Sun (Orange) orbited around the common center of mass for the planet-Sun system. He then modified Kepler's 3rd Law so that the mass M used is now the sum of the mass of the Sun plus the planet @_@(oh my god my head hurts after saying all that in the class X_x)
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Re: Kyousei High School RP 2~
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on 2008-01-29 17:36:44 (edited 2008-01-30 15:37:59)
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[Class 4b Student, Username: kabluam, Character name: Zlatan Kachizky] Saki~ Owh.. Ah! Gomen teacher! Issac Newton's universal theory of gravitation is that every point mass attracts every other point mass by a force pointing along the line intersecting both points. The force is proportional to the product of the two masses and inversely proportional to the square of the distance between the point masses: F=G(m1 x m2)/r² where * F is the magnitude of the gravitational force between the two point masses, * G is the gravitational constant, * m1 is the mass of the first point mass, * m2 is the mass of the second point mass, * r is the distance between the two point masses. Please tell me that was right... T 3T; *he writes something on his note and he mumbles to himself* zlatan: check.. i think that's correct Ikuto: well you are right Saki, but here's my answer to that question Ms.Yuuka *ahem* The equation for the force of gravity for all objects relatively close to the Earth is: F = mg where * F is the force pulling objects toward the Earth; it is also the weight of the object * m is the mass of the object * g is the acceleration due to gravity; this number is a constant for all masses of matter * mg is the product of m times g. The weight of an object is the measurement of the force of gravity on that object. You weigh something on a scale, according to the force that the Earth pulls it down. Thus the weight is actually the force of gravity on that object: w = mg where * w is weight * m is mass * g is acceleration due to gravity which makes Newton realized that in the planet-Sun system, the planet does not orbit around a stationary Sun. Instead, Newton proposed that both *brings out an Apple and a Orange for a little show and tell ^^;* the planet (the apple) and the Sun (Orange) orbited around the common center of mass for the planet-Sun system. He then modified Kepler's 3rd Law so that the mass M used is now the sum of the mass of the Sun plus the planet @_@(oh my god my head hurts after saying all that in the class X_x) *zlatan writes something on his note and he mumbles again* zlatan: wait, althought that statement is correct, i think that's to far from what ms yuuka asked *pokes Zlatan* You're too tall to be in the front row.. I can't see >w>; *zlatan looks back at saki* zlatan: yep, so you want me to move from this spot?? why don't just you move to the front row, so you can see better? |
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Re: Kyousei High School RP 2~
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on 2008-01-29 22:08:51 |
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[4-B] Ikuto: well you are right Saki, but here's my answer to that question Ms.Yuuka *ahem* The equation for the force of gravity for all objects relatively close to the Earth is: F = mg where * F is the force pulling objects toward the Earth; it is also the weight of the object * m is the mass of the object * g is the acceleration due to gravity; this number is a constant for all masses of matter * mg is the product of m times g. The weight of an object is the measurement of the force of gravity on that object. You weigh something on a scale, according to the force that the Earth pulls it down. Thus the weight is actually the force of gravity on that object: w = mg where * w is weight * m is mass * g is acceleration due to gravity which makes Newton realized that in the planet-Sun system, the planet does not orbit around a stationary Sun. Instead, Newton proposed that both *brings out an Apple and a Orange for a little show and tell ^^;* the planet (the apple) and the Sun (Orange) orbited around the common center of mass for the planet-Sun system. He then modified Kepler's 3rd Law so that the mass M used is now the sum of the mass of the Sun plus the planet @_@(oh my god my head hurts after saying all that in the class X_x) Ueki: (whispers to Ikuto) Wow... Nice going, buddy. That was one heck of an explanation. |