,
Senin, 16 Maret 2015
New Poto Habib Lutfi Di Bekasi
Nilai Deklinasi matahari Dari Tahun Ke Tahun
DATE | OBSERVATION | OBLIQUITY | REMARKS |
B.C. 2045 | Karnak | 25° 09' 55" |
summer solstice, sunset orientation
|
B.C. 1570 | Karnak | 24° 32' 06" |
summer solstice, sunset orientation
|
B.C. 1100 | ancient Chinese | 24° 13' 56" |
ancient observation, derived from "Chou-Pei"
|
B.C. 1100 | ancient Chinese | 23° 54' 04" |
ascribed to Chou Kung, but corresponds to later date
|
B.C. 900 | ancient Hindu | 24° 11' 04" |
derived from Jaina Astronomical Treatise "Suryaprajnapti"
|
B.C. 700 | ancient Chinese | 24° 02' 06" |
derived from "Chou-Pei"
|
B.C. 700 | ancient Chinese | 24° 01' 50" |
derived from "Chou-Pei"
|
MEAN | 24° 01' 58" | ||
B.C. 558 | Thales | 24° 00' 56" |
observations at Miletus
|
B.C. 510 | ancient Hindu | 24° 00' 44" |
derived from the "Suryasiddhanta"
|
B.C. 326 | Pytheas | 23° 53' 46" |
observations at Marseilles
|
B.C. 326 | Pytheas | 23° 54' 53" |
observations at Marseilles
|
MEAN | 23° 54' 20" | ||
B.C. 230 | Eratosthenes | 23° 52' 04" |
observations at Alexandria
|
B.C. 230 | Eratosthenes | 23° 51' 47" |
observations at Syene at Summer Soltice
|
B.C. 230 | Eratosthenes | 23° 51' 59" |
observations at Syene at both Soltices
|
B.C. 230 | Eratosthenes | 23° 52' 12" |
observations of shadowless area at Summer Solstice
|
MEAN | 23° 52' 00" | ||
B.C. 135 | Hipparchus | 23° 52' 16" |
observations at Rhodes
|
B.C. 130 | ancient Chinese | 23° 54' 04" |
from figures given by Haui-Nan-Tzu (died B.C. 122)
|
B.C. 80 | ancient Chinese | 23° 53' 46" |
observations at Loyang. Figures given by Lieou Hiang
|
A.D. 80 | Chinese | 23° 54' 04" |
from figures given by the authors of the See-fen Astronomy, but result corresponds to earlier date of observation
|
A.D. 139 | Ptolemy | 23° 48' 16" |
observations at Alexandria
|
A.D. 521 | Chinese | 23° 40' 36" |
observations at Nanking (9 foot gnomon)
|
A.D. 521 | Chinese | 23° 41' 59" |
observations at Nanking (8 foot gnomon)
|
A.D. 521 | Chinese | 23° 41' 31" |
observations by Ouey Tartars at Kaifeng-fu, probably
|
MEAN | 23° 41' 22" | ||
A.D. 578 | Chinese | 23° 41' 12" |
observations at Sianfu
|
A.D. 579 | Chinese | 23° 41' 12" |
observations at Sianfu
|
A.D. 581 | Chinese | 23° 41' 12" |
observations at Sianfu
|
A.D. 584 | Chinese | 23° 41' 30" |
observations at Loyang
|
A.D. 596 | Chinese | 23° 42' 12" |
observations at Sianfu
|
A.D. 597 | Chinese | 23° 42' 12" |
observations at Sianfu
|
A.D. 629 | Chinese | 23° 40' 07" |
observations by Litchou-foung at Sianfu
|
A.D. 829 | Al Mamun | 23° 35' 00" |
observations at Bagdad
|
A.D. 880 | Al Battani | 23° 35' 54" |
observations at Rakka in Syria
|
A.D. 916 | Arab | 23° 35' 50" |
mean of numerous Arab observations from A.D.829-1019
|
A.D. 1000 | Ibn Junis | 23° 36' 11" |
observations at Cairo
|
A.D. 1049 - 1052 | Chinese | 23° 33' 40" |
observations as Kaifeng-fu
|
A.D. 1070 | Alzarkali | 23° 34' 42" |
observations at Toledo
|
A.D. 1100 | Chinese | 23° 34' 32" |
observations at Kaifeng-fu
|
A.D. 1130 | Chinese | 23° 31' 48" |
observations at Hang Chow
|
A.D. 1140 | Almaeon | 23° 34' 12" |
observations at Toledo
|
A.D. 1174 | Ben Maimon | 23° 31' 51" |
observations at Cordova
|
A.D. 1250 | Alphonsine Tables | 23° 33' 11" |
observations at Toledo
|
A.D. 1277-1280 | Chinese | 23° 33' 02" |
observations by Ko-Chou-King at Peking
|
A.D. 1290 | Nasar-Al-Din | 23° 31' 40" |
observations at Maragha (Persia)
|
A.D. 1290 | Guilliame de St. Cloud | 23° 34' 00" |
observation at Paris
|
A.D. 1328 | Prophatius Judaeus | 23° 32' 42" |
observations at Toledo
|
A.D. 1332 | Jean de Lignieres | 23° 33' 31" |
observations at Paris
|
A.D. 1363 | Ibn al Shatir | 23° 32' 32" |
observations at Cairo
|
A.D. 1437 | Ulugh Beigh | 23° 31' 44" |
observations at Samarkand
|
A.D. 1460 | Purbach and Regiomontanus | 23° 30' 37" |
observations at Erfurt, Nurnberg, and Vienna
|
A.D. 1468 | Toscanelli | 23° 31' 47" |
observations at Florence
|
A.D. 1491 | Walther | 23° 30' 50" |
observations at Nurnberg
|
A.D. 1491 | Novarra | 23° 30' 56" |
observations at Bologna
|
A.D. 1514 | Werner | 23° 30' 33" |
observations at Nurnberg
|
A.D. 1525 | Copernicus | 23° 30' 30" |
observations at Frauenberg
|
A.D. 1570 | Ignatius | 23° 29' 00" |
observations at Bologna (corrections uncertain)
|
A.D. 1570 | Dante Prince of Hess | 23° 31' 00" |
observations at Cassel (corrections uncertain)
|
A.D. 1570 | Rothmann & Byrge | 23° 30' 20" |
observations at Cassel (corrections uncertain)
|
MEAN | 23° 30' 07" | ||
A.D. 1587 | Tycho Brahe | 23° 29' 49" |
observations at Uraniborg
|
A.D. 1594 | Wright | 23° 30' 00" |
observations at Cambridge
|
A.D. 1616 | Wendelin | 23° 30' 16" |
observations at Forcalquier in the Basses Alpes
|
A.D. 1627 | Kepler | 23° 30' 30" |
observations at Linz (Upper Austria)
|
A.D. 1636 | Peiresc | 23° 30' 23" |
observations at Marseilles
|
A.D. 1636 | Gassendi | 23° 29' 58" |
observations at Marseilles
|
A.D. 1650 | Riccioli | 23° 29' 40" |
observations at Bologna
|
A.D. 1658 | Hevelius | 23° 29' 27" |
observations at Danzig
|
A.D. 1664 | Cassini | 23° 29' 08" |
observations at Bologna and Paris
|
A.D. 1686 | Wurzelbaur | 23° 28' 52" |
observations at Nurnberg
|
A.D. 1660 | Montons | 23° 29' 03" |
Hutton
|
A.D. 1672 | Richer | 23° 28' 52" |
Hutton
|
A.D. 1686 | La Hire | 23° 29' 28" |
Hutton
|
A.D. 1689.5 | Flamsteed | 23° 28' 56" |
Ball's Astronomy
|
A.D. 1690 | Flamsteed | 23° 28' 48" |
Encyclopaedia Britannica
|
A.D. 1690 | Flamsteed | 23° 29' 00" |
Hutton
|
MEAN | 23° 28' 55" | ||
A.D. 1703 | Bianchini | 23° 28' 35" |
Encyclopaedia Britannica
|
A.D. 1703 | Bianchini | 23° 28' 25" |
Hutton
|
MEAN | 23° 28' 30" | ||
A.D. 1706 | Roemer | 23° 28' 41" |
Hutton
|
A.D. 1715 | Louville | 23° 28' 24" |
Hutton
|
A.D. 1730 | Godin | 23° 28' 20" |
Hutton
|
A.D. 1736 | Condamine | 23° 28' 24" |
Encyclopaedia Britannica
|
A.D. 1743 | Cassini de Thury | 23° 28' 26" |
Encyclopaedia Britannica
|
A.D. 1750 | Lacaille | 23° 28' 19" |
Encyclopaedia Britannica
|
A.D. 1750 | Bradley | 23° 28' 18" |
Hutton
|
A.D. 1755 | Bradley | 23° 28' 15" |
Encyclopaedia Britannica
|
A.D. 1756 | Mayer | 23° 28' 16" |
Encyclopaedia Britannica and Hutton
|
A.D. 1769 | Maskelyne | 23° 28' 10" |
Encyclopaedia Britannica and Hutton
|
A.D. 1772 | Hornsby | 23° 28' 08" |
Hutton
|
A.D. 1779 | Nautical Almanac | 23° 28' 07" |
Hutton
|
A.D. 1780 | Cassini | 23° 27' 54" |
Encyclopaedia Britannica
|
A.D. 1795 | Maskelyne | 23° 27' 58" |
Ball's Astronomy
|
A.D. 1800 | Nautical Almanac | 23° 27' 50" |
Hutton
|
A.D. 1800 | Maskelyne | 23° 27' 57" |
Encyclopaedia Britannica and Hutton
|
A.D. 1800 | Piazzi | 23° 27' 56" |
Encyclopaedia Britannica and Hutton
|
A.D. 1800 | Pond | 23° 27' 56" |
Hutton
|
A.D. 1800 | Delambre | 23° 27' 57" |
Encyclopaedia Britannica and Hutton -- hundreds of observations
|
A.D. 1800 | Bessel | 23° 27' 55" |
Ball's Astronomy
|
A.D. 1812 | English and French Astronomers | 23° 27' 42" |
Hutton
|
A.D. 1813 | Pond | 23° 27' 49" |
Encyclopaedia Britannica
|
A.D. 1813 | Brinkley | 23° 27' 50" |
Ball's Astronomy
|
A.D. 1813 | Arago and Mathieu | 23° 27' 49" |
Grant (History of Physical Astronomy)
|
A.D. 1815 | Bessel | 23° 27' 48" |
Encyclopaedia Britannica
|
A.D. 1816 | Brinkley | 23° 27' 49" |
Encyclopaedia Britannica
|
A.D. 1825 | Pearson | 23° 27' 44" |
Encyclopaedia Britannica
|
A.D. 1835 | Airy | 23° 27' 40" |
Encyclopaedia Britannica
|
A.D. 1850 | Leverrier | 23° 27' 32" |
Encyclopaedia Britannica
|
A.D. 1868 | Airy | 23° 27' 22" |
Ball's Astronomy
|
A.D. 1880 | Nautical Almanac | 23° 27' 17.6" | |
A.D. 1900 | Nautical Almanac | 23° 27' 08" | |
A.D. 1920 | Nautical Almanac | 23° 26' 58.9" | |
A.D. 1940 | Nautical Almanac | 23° 26' 49.5" | |
A.D. 1949 | Nautical Almanac | 23° 26' 45.3" |
Beberapa Rumus Trigonometri Hasil Temuan Al Battani
Beliau sempat menulis tabel cotangen dari 0 derajat sampai 90 derajat
lewat rumus cotangen temuannya ini
dia juga tidak menggunakan rumus yang biasa dipakai matematikawan yunani
sebelumnya dalam mencari nilai m
tapi menciptakan rumus sendiri yakni
jadi dia berhasil menemukan nilai sudut x
dia juga menciptakan rumus lainnya
semisal rumus di bawah ini
saat mengukur tinggi matahari dia memiliki rumus temuan dengan cara
mengetahui tinggi h dan panjang permukaan m
copast:
Semesta Kapan Kau Berhenti Berkembang
Sampai Saat Ini Selalu Jadi Pertanyaan 'Besar' Mereka, Eksistensi ' Ruh ' ?
-----------------------
Saya jujur terkadang kumat berkhayal 'agak kelewat', seandainya manusia dilebur dalam bentuk paling kecil sekali lalu di percepat atau diperlambat tanpa terikat ruang dan waktu sebagaimana klaim para pengagum teori relativitasnya Simbah Albert Einstein [sori ya Mbah ane kritik], akankah tergambarkan eksistensi ruh ...
Sekali lagi kita pasti akan termenung karena memang ini salah satu rahasia 'Allah' yang dititipkan di dalam dada sebelah kiri insan [baca: hati], sengaja dirahasiakan karena memang para yahudi [cerdas] itu ingin bertanya lebih dalam tentang urusan yang paling rahasia tentang segala sesuatu yang paling rahasia di muka bumi ini [ehemmm serius amat bacanya sih, biasa aja kelesss]
Mestinya sebelum masuk, mereka harus mempercayai si empunya 'rumah tangga' kanjeng Nabi shollaallahu alaihi wasallam, baru setelah dijelaskan dan dipersilakan masuk akan tergambar jelas, isi 'rumah' tersebut.
tapi optimisme tetap ada, ilmu pengetahuan yang sedikit itu diharapkan bisa terungkap untuk mengenalkan iman, islam dan ihsan kepada para 'pemuja fisika'. Bisa mengungkap jati diri manusia sebenarnya karena [hakikatnya] di jagat ini tidak ada yang terjadi/muncul secara tiba. Kita [dipaksa] tunduk pada kuasa dan kehendak-Nya, dan karena 'ruh' yang dititipkan pada kita ini hendaklah kita berembah sujud kepada-Nya.
“Maka apabila telah Kusempurnakan penciptaannya dan Kutiupkan kepadanya roh (ciptaan)-Ku; maka hendaklah kamu tersungkur dengan bersujud kepadanya.” [Shad : 72]
#salam_zuperr_Gan
-----------------------
* ilustrasi [yg agak dipaksakan] benturan partikel terkecil untuk melihat sejauh mana partilkel lain terbentuk saat 'benturan pertama' di laboratorium super waaaaww CERN, swiss .. "ilmuwan lagi kesengsem sama Big Bang Theory"
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