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Guru Granth Sahib
Composition, Arrangement & Layout
ਜਪੁ | Jup
ਸੋ ਦਰੁ | So Dar
ਸੋਹਿਲਾ | Sohilaa
ਰਾਗੁ ਸਿਰੀਰਾਗੁ | Raag Siree-Raag
Gurbani (14-53)
Ashtpadiyan (53-71)
Gurbani (71-74)
Pahre (74-78)
Chhant (78-81)
Vanjara (81-82)
Vaar Siri Raag (83-91)
Bhagat Bani (91-93)
ਰਾਗੁ ਮਾਝ | Raag Maajh
Gurbani (94-109)
Ashtpadi (109)
Ashtpadiyan (110-129)
Ashtpadi (129-130)
Ashtpadiyan (130-133)
Bara Maha (133-136)
Din Raen (136-137)
Vaar Maajh Ki (137-150)
ਰਾਗੁ ਗਉੜੀ | Raag Gauree
Gurbani (151-185)
Quartets/Couplets (185-220)
Ashtpadiyan (220-234)
Karhalei (234-235)
Ashtpadiyan (235-242)
Chhant (242-249)
Baavan Akhari (250-262)
Sukhmani (262-296)
Thittee (296-300)
Gauree kii Vaar (300-323)
Gurbani (323-330)
Ashtpadiyan (330-340)
Baavan Akhari (340-343)
Thintteen (343-344)
Vaar Kabir (344-345)
Bhagat Bani (345-346)
ਰਾਗੁ ਆਸਾ | Raag Aasaa
Gurbani (347-348)
Chaupaday (348-364)
Panchpadde (364-365)
Kaafee (365-409)
Aasaavaree (409-411)
Ashtpadiyan (411-432)
Patee (432-435)
Chhant (435-462)
Vaar Aasaa (462-475)
Bhagat Bani (475-488)
ਰਾਗੁ ਗੂਜਰੀ | Raag Goojaree
Gurbani (489-503)
Ashtpadiyan (503-508)
Vaar Gujari (508-517)
Vaar Gujari (517-526)
ਰਾਗੁ ਦੇਵਗੰਧਾਰੀ | Raag Dayv-Gandhaaree
Gurbani (527-536)
ਰਾਗੁ ਬਿਹਾਗੜਾ | Raag Bihaagraa
Gurbani (537-556)
Chhant (538-548)
Vaar Bihaagraa (548-556)
ਰਾਗੁ ਵਡਹੰਸ | Raag Wadhans
Gurbani (557-564)
Ashtpadiyan (564-565)
Chhant (565-575)
Ghoriaan (575-578)
Alaahaniiaa (578-582)
Vaar Wadhans (582-594)
ਰਾਗੁ ਸੋਰਠਿ | Raag Sorath
Gurbani (595-634)
Asatpadhiya (634-642)
Vaar Sorath (642-659)
ਰਾਗੁ ਧਨਾਸਰੀ | Raag Dhanasaree
Gurbani (660-685)
Astpadhiya (685-687)
Chhant (687-691)
Bhagat Bani (691-695)
ਰਾਗੁ ਜੈਤਸਰੀ | Raag Jaitsree
Gurbani (696-703)
Chhant (703-705)
Vaar Jaitsaree (705-710)
Bhagat Bani (710)
ਰਾਗੁ ਟੋਡੀ | Raag Todee
ਰਾਗੁ ਬੈਰਾੜੀ | Raag Bairaaree
ਰਾਗੁ ਤਿਲੰਗ | Raag Tilang
Gurbani (721-727)
Bhagat Bani (727)
ਰਾਗੁ ਸੂਹੀ | Raag Suhi
Gurbani (728-750)
Ashtpadiyan (750-761)
Kaafee (761-762)
Suchajee (762)
Gunvantee (763)
Chhant (763-785)
Vaar Soohee (785-792)
Bhagat Bani (792-794)
ਰਾਗੁ ਬਿਲਾਵਲੁ | Raag Bilaaval
Gurbani (795-831)
Ashtpadiyan (831-838)
Thitteen (838-840)
Vaar Sat (841-843)
Chhant (843-848)
Vaar Bilaaval (849-855)
Bhagat Bani (855-858)
ਰਾਗੁ ਗੋਂਡ | Raag Gond
Gurbani (859-869)
Ashtpadiyan (869)
Bhagat Bani (870-875)
ਰਾਗੁ ਰਾਮਕਲੀ | Raag Ramkalee
Ashtpadiyan (902-916)
Gurbani (876-902)
Anand (917-922)
Sadd (923-924)
Chhant (924-929)
Dakhnee (929-938)
Sidh Gosat (938-946)
Vaar Ramkalee (947-968)
ਰਾਗੁ ਨਟ ਨਾਰਾਇਨ | Raag Nat Narayan
Gurbani (975-980)
Ashtpadiyan (980-983)
ਰਾਗੁ ਮਾਲੀ ਗਉੜਾ | Raag Maalee Gauraa
Gurbani (984-988)
Bhagat Bani (988)
ਰਾਗੁ ਮਾਰੂ | Raag Maaroo
Gurbani (889-1008)
Ashtpadiyan (1008-1014)
Kaafee (1014-1016)
Ashtpadiyan (1016-1019)
Anjulian (1019-1020)
Solhe (1020-1033)
Dakhni (1033-1043)
ਰਾਗੁ ਤੁਖਾਰੀ | Raag Tukhaari
Bara Maha (1107-1110)
Chhant (1110-1117)
ਰਾਗੁ ਕੇਦਾਰਾ | Raag Kedara
Gurbani (1118-1123)
Bhagat Bani (1123-1124)
ਰਾਗੁ ਭੈਰਉ | Raag Bhairo
Gurbani (1125-1152)
Partaal (1153)
Ashtpadiyan (1153-1167)
ਰਾਗੁ ਬਸੰਤੁ | Raag Basant
Gurbani (1168-1187)
Ashtpadiyan (1187-1193)
Vaar Basant (1193-1196)
ਰਾਗੁ ਸਾਰਗ | Raag Saarag
Gurbani (1197-1200)
Partaal (1200-1231)
Ashtpadiyan (1232-1236)
Chhant (1236-1237)
Vaar Saarang (1237-1253)
ਰਾਗੁ ਮਲਾਰ | Raag Malaar
Gurbani (1254-1293)
Partaal (1265-1273)
Ashtpadiyan (1273-1278)
Chhant (1278)
Vaar Malaar (1278-91)
Bhagat Bani (1292-93)
ਰਾਗੁ ਕਾਨੜਾ | Raag Kaanraa
Gurbani (1294-96)
Partaal (1296-1318)
Ashtpadiyan (1308-1312)
Chhant (1312)
Vaar Kaanraa
Bhagat Bani (1318)
ਰਾਗੁ ਕਲਿਆਨ | Raag Kalyaan
Gurbani (1319-23)
Ashtpadiyan (1323-26)
ਰਾਗੁ ਪ੍ਰਭਾਤੀ | Raag Prabhaatee
Gurbani (1327-1341)
Ashtpadiyan (1342-51)
ਰਾਗੁ ਜੈਜਾਵੰਤੀ | Raag Jaijaiwanti
Gurbani (1352-53)
Salok | Gatha | Phunahe | Chaubole | Swayiye
Sehskritee Mahala 1
Sehskritee Mahala 5
Gaathaa Mahala 5
Phunhay Mahala 5
Chaubolae Mahala 5
Shaloks Bhagat Kabir
Shaloks Sheikh Farid
Swaiyyae Mahala 5
Swaiyyae in Praise of Gurus
Shaloks in Addition To Vaars
Shalok Ninth Mehl
Mundavanee Mehl 5
ਰਾਗ ਮਾਲਾ, Raag Maalaa
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Moon’s Rich Surface Contains Silver, Carbon Dioxide
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<blockquote data-quote="spnadmin" data-source="post: 135723" data-attributes="member: 35"><p>The surface of the moon contains not just water, but a rich mix of elements, including silver and carbon dioxide, astronomers said Thursday.</p><p></p><p>The findings to be published in the journal Science come from an analysis of data from the Lunar Crater Observation and Sensing Satellite (LCROSS) experiment that crashed into the moon last year.</p><p></p><p>Data from the experiment had already shown water is even more abundant on the moon’s craters than expected.</p><p></p><p>Scientists said Thursday they had found light hydrocarbons, traces of sulphur and carbon dioxide in the plume of dust kicked up by the crashing craft.</p><p></p><p>They have also been able to estimate more thoroughly the amount of water in the crater, which they believe makes up about 5.6 per cent of the mass in the crater. There’s enough water in the form of pure ice crystals to be useful for humans, both as pure water or separated into parts for fuel, the scientists found.</p><p></p><p>Silver was found in trace amounts among the light metals that also included sodium and mercury.</p><p></p><p>The dramatic experiment in 2009 crashed the LCROSS spacecraft into the moon’s Cabeus crater, sending a huge plume of dust 10 kilometres upward to gather data about ice that was suspected to be hidden in the perpetually dark lunar craters.</p><p></p><p>The components of the dust were analysed by another space craft called Lunar Reconnaissance Orbiter (LRO) that followed closely behind, gathering data. Major telescopes around the world were also aimed at the Cabeus crater on the moon’s south pole to capture data from the dust plume.</p><p></p><p>The analysis shows how rich the moon is in useful minerals and that it remains chemically active and has a water cycle, NASA scientists said.</p><p></p><p>“Seeing mostly pure water ice grains in the plume means water ice was somehow delivered to the moon in the past, or chemical processes have been causing ice to accumulate in large quantities,” said Anthony Colaprete, LCROSS project scientist and principal investigator at NASA’s Ames Research Centre in California.</p><p></p><p>“Also, the diversity and abundance of certain materials called volatiles in the plume suggest a variety of sources, like comets and asteroids, and an active water cycle within the lunar shadows.” The rocket’s impact was designed to replicate that of the large, natural asteroids that slam into the moon several times a month.</p><p></p><p>The NASA probe targeted a 100-kilometre wide, four-kilometre deep crater and was timed to strike when lighting conditions are ideal for observing the impact. The 585-kg craft created an impact crater about two metres deep. </p><p></p><p><a href="http://www.thehindu.com/sci-tech/science/article842838.ece?homepage=true" target="_blank">http://www.thehindu.com/sci-tech/science/article842838.ece?homepage=true</a></p></blockquote><p></p>
[QUOTE="spnadmin, post: 135723, member: 35"] The surface of the moon contains not just water, but a rich mix of elements, including silver and carbon dioxide, astronomers said Thursday. The findings to be published in the journal Science come from an analysis of data from the Lunar Crater Observation and Sensing Satellite (LCROSS) experiment that crashed into the moon last year. Data from the experiment had already shown water is even more abundant on the moon’s craters than expected. Scientists said Thursday they had found light hydrocarbons, traces of sulphur and carbon dioxide in the plume of dust kicked up by the crashing craft. They have also been able to estimate more thoroughly the amount of water in the crater, which they believe makes up about 5.6 per cent of the mass in the crater. There’s enough water in the form of pure ice crystals to be useful for humans, both as pure water or separated into parts for fuel, the scientists found. Silver was found in trace amounts among the light metals that also included sodium and mercury. The dramatic experiment in 2009 crashed the LCROSS spacecraft into the moon’s Cabeus crater, sending a huge plume of dust 10 kilometres upward to gather data about ice that was suspected to be hidden in the perpetually dark lunar craters. The components of the dust were analysed by another space craft called Lunar Reconnaissance Orbiter (LRO) that followed closely behind, gathering data. Major telescopes around the world were also aimed at the Cabeus crater on the moon’s south pole to capture data from the dust plume. The analysis shows how rich the moon is in useful minerals and that it remains chemically active and has a water cycle, NASA scientists said. “Seeing mostly pure water ice grains in the plume means water ice was somehow delivered to the moon in the past, or chemical processes have been causing ice to accumulate in large quantities,” said Anthony Colaprete, LCROSS project scientist and principal investigator at NASA’s Ames Research Centre in California. “Also, the diversity and abundance of certain materials called volatiles in the plume suggest a variety of sources, like comets and asteroids, and an active water cycle within the lunar shadows.” The rocket’s impact was designed to replicate that of the large, natural asteroids that slam into the moon several times a month. The NASA probe targeted a 100-kilometre wide, four-kilometre deep crater and was timed to strike when lighting conditions are ideal for observing the impact. The 585-kg craft created an impact crater about two metres deep. [url]http://www.thehindu.com/sci-tech/science/article842838.ece?homepage=true[/url] [/QUOTE]
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Moon’s Rich Surface Contains Silver, Carbon Dioxide
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