EXPLANATION TEXT SUN SET.docx

 Nama : Nides Prianda Ginting Kelas : XII IPS 1 Task

: English (Expalanation Text)

Sunset Or Sundowsn

Sunset or sundown, is the daily disappearance of the Sun  below the western

horizon as a result of  Earth's  Earth's rotation. The three phases of twilight after sunset :

The time of sunset is defined in astronomy as the moment when the trailing edge of the Sun's disk disappears below the horizon. Near to the horizon, atmospheric refraction causes the ray path of light from the Sun to be distorted to such an extent that geometrically the Sun's disk is already about one diameter  below the horizon when sunset is observed. observed. The spinning Earth lit by the Sun as seen from far above the North Pole. All along the terminator, the rays from the sun hit Earth horizontally, neglecting any atmospheric effects and Earth's orbital motion. Sunset is distinct from twilight, from twilight, which  which has three phases, the first being civil  twilight, which begins once the Sun has disappeared below the horizon, and

continues until it descends to 6 degrees below the horizon; the second phase is nautical   twilight,

between 6 and 12 degrees below the horizon; and the third is

astronomical   twilight,

which is the period when the Sun is between 12 and 18

degrees below the horizon.[1]  Dusk  is at the very end of astronomical twilight, and is the darkest moment of twilight just before night.[2]  Night occurs when the Sun reaches 18 degrees below the horizon and no longer illuminates the sky, Locations north of the Arctic Circle and south of the Antarctic Circle experience no sunset or sunrise on at least one day of the year, when the  polar day or the  polar night persists continuously for 24 hours. Sunset creates unique atmospheric conditions such as the often intense orange and red colors of the Sun and the surrounding sky.

General Structure Sunset Or Sundowsn

a. General Statement Sunset or sundown, is the daily disappearance of the Sun below the western

horizon as a result of  Earth's rotation.

 b. Sequenced statement The time of sunset is defined in astronomy as the moment when the trailing edge of the Sun's disk disappears below the horizon. Near to the horizon, atmospheric refraction causes the ray path of light from the Sun to be distorted to such an extent that geometrically the Sun's disk is already about one diameter below the horizon when sunset is observed.

The spinning Earth lit by the Sun as seen from far above the North Pole. All along the terminator, the rays from the sun hit Earth horizontally, neglecting any atmospheric effects and Earth's orbital motion.

Sunset is distinct from twilight, which has three phases, the first being civil  twilight, which begins once the Sun has disappeared below the horizon, and continues until it descends to 6 degrees below the horizon; the second phase is nautical  twilight,

between 6 and 12 degrees below the horizon; and the third is

astronomical  twilight,

which is the period when the Sun is between 12 and 18

degrees below the horizon.[1]  Dusk  is at the very end of astronomical twilight, and is the darkest moment of twilight just before night.[2]  Night occurs when the Sun reaches 18 degrees below the horizon and no longer illuminates the sky,

c. Close Statement Sunset creates unique atmospheric conditions such as the often intense orange and red colors of the Sun and the surrounding sky.

PASSIVE VOICE 

The time of sunset is defined in astronomy as the moment when the trailing edge of the Sun's disk disappears below the horizon.



 Near to the horizon,  atmospheric refraction causes the ray path of light from the Sun to be distorted to such an extent that geometrically the Sun's disk is already about one diameter below the horizon when sunset is observed.

Source : https://en.wikipedia.org/wiki/Sunset

Terjemahan MATAHARI TERBENAM

Sunset atau matahari terbenam, adalah hilangnya harian Matahari di bawah ufuk  barat sebagai akibat dari rotasi bumi.

Tiga fase senja setelah matahari terbenam: Waktu matahari terbenam didefinisikan dalam astronomi sebagai saat ketika trailing edge dari disk matahari menghilang di bawah cakrawala. Dekat cakrawala, refraksi atmosfer menyebabkan jalur sinar cahaya dari Matahari yang akan terdistorsi sedemikian rupa bahwa geometris disk Matahari sudah sekitar satu diameter di bawah cakrawala saat matahari terbenam diamati.

Bumi berputar diterangi Matahari seperti yang terlihat dari jauh di atas Kutub Utara. Sepanjang terminator, sinar dari matahari menghantam bumi secara horizontal, mengabaikan efek atmosfer dan gerakan orbital bumi.

Sunset berbeda dari senja, yang memiliki tiga tahap, yang pertama senja sipil, yang dimulai setelah Matahari telah menghilang di bawah cakrawala, dan terus sampai turun ke 6 derajat di bawah cakrawala; tahap kedua adalah senja bahari, antara 6 dan 12 derajat di bawah cakrawala; dan yang ketiga adalah senja astronomi, yang merupakan periode ketika matahari berada antara 12 dan 18 derajat di bawah cakrawala. [1] Senja adalah di akhir senja astronomi, dan saat  paling gelap senja sebelum malam. [2 ] Malam terjadi ketika matahari mencapai 18

derajat

di

bawah

cakrawala

dan

tidak

lagi

menerangi

langit,

Lokasi utara Lingkaran Arktik dan selatan dari pengalaman Lingkaran Antartika tidak ada sunset atau sunrise pada setidaknya satu hari dalam setahun, ketika hari  polar atau malam kutub berlanjut terus menerus selama 24 jam.

Sunset menciptakan kondisi atmosfer yang unik seperti jeruk sering intens dan warna merah dari Matahari dan langit sekitarnya.