What is cyber bullying???

Cyber bullying is when the Internet, cell phones or other devices that are used to send or post text/images that are intended to hurt or embarrass another person.

Why is cyber bullying  Dangerous???

Cyber bullying would hurt and embarrass another person and also cause  infringement on internet safety.

How to stop cyber bullying???

1)Tell your friends not to pass along harmful or cruel messages or images.

2)Tell students to delete all the suspicious email messages when they don’t know who is the user sending the E-Mail.

3)If you know friends who are cyber bullys, step up to them and tell them to stop.

4)Teach your friends how to use technology to block communication with cyberbullies/ people you don’t know.

5)During MSN, add contacts only the  people you know. Do not add strangers.

IS THIS TRUTH???

The term eclipse is most often used to describe either a solar eclipse, when the Moon’s shadow crosses the Earth’s surface, or a lunar eclipse, when the Moon moves into the shadow of Earth. However, it can also refer to such events beyond the Earth-Moon system: for example, a planet moving into the shadow cast by one of its moons, a moon passing into the shadow cast by its host planet, or a moon passing into the shadow of another moon. A binary star system can also produce eclipses if the plane of their orbit intersects the position of the observer.

An eclipse of the Sun by the Moon is termed a solar eclipse. The type of solar eclipse event depends on the distance of the Moon from the Earth during the event. A total solar eclipse occurs when the Earth intersects the umbra portion of the Moon’s shadow. When the umbra does not reach the surface of the Earth, the Sun is only partially occluded, resulting in an annular eclipse. Partial solar eclipses occur when the viewer is inside the penumbra.

The eclipse magnitude is the fraction of the Sun’s diameter that is covered by the Moon. For a total eclipse, this value is always greater than or equal to one. In both annular and total eclipses, the eclipse magnitude is the ratio of the angular sizes of the Moon to the Sun.

Solar eclipses are relatively brief events that can only be viewed in totality along a relatively narrow track. Under the most favorable circumstances, a total solar eclipse can last for 7 minutes, 31 seconds, and can be viewed along a track that is up to 250 km wide. However, the region where a partial eclipse can be observed is much larger. The Moon’s umbra will advance eastward at a rate of 1,700 km/h, until it no longer intersects the Earth.

During a solar eclipse, the Moon can sometimes perfectly cover the Sun because its apparent size is nearly the same as the Sun when viewed from the Earth. A solar eclipse is actually a misnomer; the phenomenon is more correctly described as an occultation of the Sun by the Moon or an eclipse of the Earth by the Moon.

Aaron lim .

From; Joshua.. x333

by:kong wei keong

Aaron lim