Solat Itu Tiang Agama Islam

1. Dibaca 21 kali sebelum masuk tidur Insya Allah akan dijaga oleh Allah Subhanahu wa Ta’ala daripada gangguan makhluk halus, jin, syaitan, pencuri, mati mengejut dan perkara yang tidak diingini berlaku termasuk sihir.

2. Dibaca 786 kali pada air di waktu malam (seeloknya malam Juma’at) lalu diberi minum pada orang yang bodoh, lemah ingatan, bebal, diberi minum pada waktu pagi (waktu terbit matahari) insya Allah akan diterangkan hati oleh Allah Subhanahu wa Ta’ala (diulang selama 7 hari).

3. Dibaca 50 kali dihadapan orang yang zalim insya Allah akan dihinakan orang zalim itu oleh Allah Subhanahu wa Ta’ala.

4. Ditulis 135 kali lalu diletakkan di depan pintu rumah, insya Allah rumah itu akan terhindar dari jin dan syaitan.

5. Ditulis 101 kali lalu dimasukkan ke dalam botol dan ditutup/disumbat agar tidak masuk air ditanam di tempat sawah insya Allah akan terselamat dari binatang perosak dan penyakit tanaman.

Source: Amalan Rahsia dan Kehebatan Ayat Al-Quran (2008)

Untuk mendengar dan menghayati al-quran bolehlah melayari
laman web :www.quranexplorer.com

1. Dibaca 41 kali bersama dengan surah Al-Ikhlas, Al-Falaq dan An-Naas sebelum tidur insya Allah akan dijaga dari sekalian bahaya kecuali mati.

2. Dibaca 41 kali setelah qabliah subuh (sebelum fardhu Subuh) akan dikurniakan oleh Allah Subhanahu wa Ta'ala:

a. Dimudahkan naik pangkat
b. Diluaskan rezeki
c. Dimudahkan membayar hutang
d. Disembuhkan dari penyakit
e. Orang yang lemah akan dikuatkan oleh Allah serta digalati, disegani dan dihormati
f. Disayangi oleh semua makhluk
g. Percakapan didengar orang
h. Selamat dari bala bencana

3. Diamalkan 7 kali selepas solat fardhu akan dikurniakan oleh Allah Subhanahu wa Ta'ala:

a. Berkat dalam kehidupan
b. Dihilangkan kesusahan di dunia dan akhirat.

4. Diamalkan 20 kali selepas solat fardhu tanpa berkata-kata akan diluaskan rezeki dan dikurniakan rezeki tanpa diduganya.

5. Jika dibaca 40 kali di air maka air itu akan menjadi ubat dari segala penyakit kecuali mati.

6. Ditulis dan dilebur dengan air dengan izin Allah akan hilang segala kerisauan, kesusahan dan ketidaktenangan hati dan jiwa.

7. Jika dibaca 121 kali oleh orang yang diikat / dipasung dengan khusyuk dan penuh keyakinan dan ditiup sebanyak 10 kali pada ikatan itu dengan izin Allah akan terlepas.

8. Jika ditulis kalimah pada kenderaan dan rumah akan terhindar dari perkara yang tidak baik termasuk kecurian.

9. Dibaca مَـٰلِكِ يَوۡمِ ٱلدِّينِ pada sebiji batu atau apa sahaja melainkan najis kemudian diletakkan pada kenderaan, insya Allah kenderaan tersebut tidak akan diganggu, dikacau atau dicuri dengan syarat selepas meletakkan batu tadi pada kenderaan tidak boleh menoleh lagi pada kenderaan tersebut (kita serahkan bulat-bulat penjagaannya kepada Allah Subhanahu wa Ta'ala).

10. Dibaca وَإِيَّاكَ نَسۡتَعِينُ tiga kali senafas ditiup pada binatang garang atau orang zalim dengan izin Allah tidak akan dapat memudharatkan kita.

Jika ditulis ayat ini dan dilebur dengan air kemudian diminum oleh orang yang lemah hafalan, lemah ingatan, kurang cerdas dalam berfikir, lemah dalam pelajaran Insya Allah akan dikuatkan dan dicerdaskan otaknya.

Untuk mengelakkan kenderaan daripada berlanggar atau menemui kemalangan, sila lakukan seperti berikut:

1) Sediakan air di dalam satu bekas.

2) Setelah disediakan air, bacalah Al-Fatihah 3 kali, ayat Qul huAllahu Ahad (al-Ikhlas) 3 kali, Qul a'udzubirobbinnas (An-Nas) 3 kali. Setiap 3 kali dibaca ayat yang diterangkan, hendaklah ditiupkan ke dalam air.

3) Setelah melakukan perkara yang disebutkan di atas, siramkanlah air itu ke atas kereta anda dengan memulakannya dari arah berikut:

a. Mulakan dari sebelah kanan pemandu hingga ke depan.

b. Dari depan ke kiri.

c. Dari kiri ke belakang.

d. Dari belakang pusing sehingga sampai ke tempat duduk pemandu.

Apabila anda lakukan seperti yang ditunjukkan di atas, InsyaAllah, kenderaan anda tidak akan mengalami kemalangan yang besar.

Perhatian:
Perkara yang disebutkan di atas hanya perlu dilakukan sekali sahaja pada awal anda membeli kenderaan itu. Bagi yang sudah memiliki kenderaan boleh memulakannya dari sekarang. Cukup dengan sekali sahaja.

A star is a massive, luminous ball of plasma that is held together by its own gravity. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth. Other stars are visible in the night sky, when they are not outshone by the Sun. For most of its life, a star shines due to thermonuclear fusion in its core releasing energy that traverses the star's interior and then radiates into outer space. Almost all elements heavier than hydrogen and helium were created by fusion processes in stars.

Astronomers can determine the mass, age, chemical composition and many other properties of a star by observing its spectrum, luminosity and motion through space. The total mass of a star is the principal determinant in its evolution and eventual fate. Other characteristics of a star are determined by its evolutionary history, including the diameter, rotation, movement and temperature. A plot of the temperature of many stars against their luminosities, known as a Hertzsprung-Russell diagram (H–R diagram), allows the age and evolutionary state of a star to be determined.

A star begins as a collapsing cloud of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. Once the stellar core is sufficiently dense, some of the hydrogen is steadily converted into helium through the process of nuclear fusion.^[1] The remainder of the star's interior carries energy away from the core through a combination of radiative and convective processes. The star's internal pressure prevents it from collapsing further under its own gravity. Once the hydrogen fuel at the core is exhausted, those stars having at least 0.4 times the mass of the Sun^[2] expand to become a red giant, in some cases fusing heavier elements at the core or in shells around the core. The star then evolves into a degenerate form, recycling a portion of the matter into the interstellar environment, where it will form a new generation of stars with a higher proportion of heavy elements.^[3]

Binary and multi-star systems consist of two or more stars that are gravitationally bound, and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution.^[4] Stars can form part of a much larger gravitationally bound structure, such as a cluster or a galaxy.

The Sun (Latin: Sol), a yellow dwarf, is the star at the center of the Solar System. The Earth and other matter (including other planets, asteroids, meteoroids, comets, and dust) orbit the Sun,^[9] which by itself accounts for about 98.6% of the Solar System's mass. The mean distance of the Sun from the Earth is approximately 149,600,000 kilometers, or 92,960,000 miles, and its light travels this distance in 8 minutes and 19 seconds. Energy from the Sun, in the form of sunlight, supports almost all life on Earth via photosynthesis,^[10] and drives the Earth's climate and weather.

The surface of the Sun consists of hydrogen (about 74% of its mass, or 92% of its volume), helium (about 24% of mass, 7% of volume), and trace quantities of other elements, including iron, nickel, oxygen, silicon, sulfur, magnesium, carbon, neon, calcium, and chromium.^[11] The Sun has a spectral class of G2V. G2 means that it has a surface temperature of approximately 5,780 K (5,500 °C) giving it a white color that often, because of atmospheric scattering, appears yellow when seen from the surface of the Earth. This is a subtractive effect, as the preferential scattering of shorter wavelength light removes enough violet and blue light, leaving a range of frequencies that is perceived by the human eye as yellow. It is this scattering of light at the blue end of the spectrum that gives the surrounding sky its color. When the Sun is low in the sky, even more light is scattered so that the Sun appears orange or even red.^[12]

The Sun's spectrum contains lines of ionized and neutral metals as well as very weak hydrogen lines. The V (Roman five) in the spectral class indicates that the Sun, like most stars, is a main sequence star. This means that it generates its energy by nuclear fusion of hydrogen nuclei into helium. There are more than 100 million G2 class stars in our galaxy. Once regarded as a small and relatively insignificant star, the Sun is now known to be brighter than 85% of the stars in the galaxy, most of which are red dwarfs.^[13]

The Sun orbits the center of the Milky Way galaxy at a distance of approximately 24,000 to 26,000 light years from the galactic center, moving generally in the direction of Cygnus and completing one revolution in about 225–250 million years (one Galactic year). Its orbital speed was thought to be 220±20 km/s, but a new estimate gives 251 km/s.^[14] This is equivalent to about one light-year every 1,190 years, and about one AU every 7 days. These measurements of galactic distance and speed are as accurate as can be, given current knowledge, but this may change as more is learned.^[15] Since our galaxy is moving with respect to the cosmic microwave background radiation (CMB) in the direction of Hydra with a speed of 550 km/s, the sun's resultant velocity with respect to the CMB is about 370 km/s in the direction of Crater or Leo.^[16]

The Sun is currently traveling through the Local Interstellar Cloud in the low-density Local Bubble zone of diffuse high-temperature gas, in the inner rim of the Orion Arm of the Milky Way Galaxy, between the larger Perseus and Sagittarius arms of the galaxy. Of the 50 nearest stellar systems within 17 light-years (1.6×10¹⁴ km) from the Earth, the Sun ranks 4th in absolute magnitude as a fourth magnitude star (M=4.83).^{[citation needed]}

SOLAT ITU TIANG AGAMA