buduhamuduruwo kiyala thiyanawane aasawan atharinna kiyala ...ehemanan ay hamuduruwo benz car wala yanne?
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Question 6: Ay Hamuduruwo Benz car wala yanne?
- Thread starter ExBuddhist Nishantha
- Start date
allah kiyala thiyenawa haram mas kanna epa kiyala. ehema thiyeddi ay samahara muslimla haram mas kanne?
Oka hambayekgen ahapan...matath hamyanta denna prashna tikak thiyenawa...mage buddhist prashna walata passe mama unta ewa denawa...dan kiyapank mekata uththare
Ithin umba ex-buddhist nam umba dannawa athine.. ekawath nodanada umba agama athariye?? dan balapan ahemed. u ex-muslim. u islam gana hama reddama dannawa palli ehema gihin typical widihata hadapu hinda. u ewa okkoma danagena wadak naha kiyala thama ee agama (thrastha waadaya) atha arala thamnge nuwanata galapena aagamak thora gatte. umba buddagama gana melo deyak nodana eka paattama man atharino kiyala atha arala apita gon kama pradarshanaya karanawa...
Ithin umba ex-buddhist nam umba dannawa athine.. ekawath nodanada umba agama athariye?? dan balapan ahemed. u ex-muslim. u islam gana hama reddama dannawa palli ehema gihin typical widihata hadapu hinda. u ewa okkoma danagena wadak naha kiyala thama ee agama (thrastha waadaya) atha arala thamnge nuwanata galapena aagamak thora gatte. umba buddagama gana melo deyak nodana eka paattama man atharino kiyala atha arala apita gon kama pradarshanaya karanawa...
machan mama megana hondata hoyala balala thamai me theerane gaththe...ko ithin mage prashnawalata umbala uththara denne nane? oya prashna tika nisa thamai mama buddhagama atha ariye..
appe ehenam loku deyak ehenam umba atharapu eka. dan ithin oya prashna nisama umba buddagama ata ariyanam ithin aye ewata uttara deela wadak nahane...
Kaatawath Wadak nathi thread walin wadak gamu.
Supernova
From Wikipedia, the free encyclopedia
This article is about the astronomical event. For other uses, see Supernova (disambiguation).
Multiwavelength X-ray, infrared, and optical compilation image of Kepler's Supernova Remnant, SN 1604. (Chandra X-ray Observatory)
A supernova (plural supernovae) is a stellar explosion that is more energetic than a nova. Supernovae are extremely luminous and cause a burst of radiation that often briefly outshines an entire galaxy, before fading from view over several weeks or months. During this short interval a supernova can radiate as much energy as the Sun is expected to emit over its entire life span.[1] The explosion expels much or all of a star's material[2] at a velocity of up to 30,000 km/s (10% of the speed of light), driving a shock wave[3] into the surrounding interstellar medium. This shock wave sweeps up an expanding shell of gas and dust called a supernova remnant.
Several types of supernovae exist. Types I and II can be triggered in one of two ways, either turning off or suddenly turning on the production of energy through nuclear fusion. After the core of an aging massive star ceases generating energy from nuclear fusion, it may undergo sudden gravitational collapse into a neutron star or black hole, releasing gravitational potential energy that heats and expels the star's outer layers. Alternatively a white dwarf star may accumulate sufficient material from a stellar companion (either through accretion or via a merger) to raise its core temperature enough to ignite carbon fusion, at which point it undergoes runaway nuclear fusion, completely disrupting it. Stellar cores whose furnaces have permanently gone out collapse when their masses exceed the Chandrasekhar limit, while accreting white dwarfs ignite as they approach this limit (roughly 1.38[4] times the mass of the sun). White dwarfs are also subject to a different, much smaller type of thermonuclear explosion fueled by hydrogen on their surfaces called a nova. Solitary stars with a mass below approximately nine solar masses, such as the Sun, evolve into white dwarfs without ever becoming supernovae.
On average, supernovae occur about once every 50 years in a galaxy the size of the Milky Way.[5] They play a significant role in enriching the interstellar medium with higher mass elements.[6] Furthermore, the expanding shock waves from supernova explosions can trigger the formation of new stars.[7][8][9]
Nova (plural novae) means "new" in Latin, referring to what appears to be a very bright new star shining in the celestial sphere; the prefix "super-" distinguishes supernovae from ordinary novae, which also involve a star increasing in brightness, though to a lesser extent and through a different mechanism. The word supernova was coined by
Swiss astrophysicist and astronomer Fritz Zwicky,[10][11] and was first used in print in 1926.[12]
Supernova
Supernova
From Wikipedia, the free encyclopedia
This article is about the astronomical event. For other uses, see Supernova (disambiguation).
Multiwavelength X-ray, infrared, and optical compilation image of Kepler's Supernova Remnant, SN 1604. (Chandra X-ray Observatory)
A supernova (plural supernovae) is a stellar explosion that is more energetic than a nova. Supernovae are extremely luminous and cause a burst of radiation that often briefly outshines an entire galaxy, before fading from view over several weeks or months. During this short interval a supernova can radiate as much energy as the Sun is expected to emit over its entire life span.[1] The explosion expels much or all of a star's material[2] at a velocity of up to 30,000 km/s (10% of the speed of light), driving a shock wave[3] into the surrounding interstellar medium. This shock wave sweeps up an expanding shell of gas and dust called a supernova remnant.
Several types of supernovae exist. Types I and II can be triggered in one of two ways, either turning off or suddenly turning on the production of energy through nuclear fusion. After the core of an aging massive star ceases generating energy from nuclear fusion, it may undergo sudden gravitational collapse into a neutron star or black hole, releasing gravitational potential energy that heats and expels the star's outer layers. Alternatively a white dwarf star may accumulate sufficient material from a stellar companion (either through accretion or via a merger) to raise its core temperature enough to ignite carbon fusion, at which point it undergoes runaway nuclear fusion, completely disrupting it. Stellar cores whose furnaces have permanently gone out collapse when their masses exceed the Chandrasekhar limit, while accreting white dwarfs ignite as they approach this limit (roughly 1.38[4] times the mass of the sun). White dwarfs are also subject to a different, much smaller type of thermonuclear explosion fueled by hydrogen on their surfaces called a nova. Solitary stars with a mass below approximately nine solar masses, such as the Sun, evolve into white dwarfs without ever becoming supernovae.
On average, supernovae occur about once every 50 years in a galaxy the size of the Milky Way.[5] They play a significant role in enriching the interstellar medium with higher mass elements.[6] Furthermore, the expanding shock waves from supernova explosions can trigger the formation of new stars.[7][8][9]
Nova (plural novae) means "new" in Latin, referring to what appears to be a very bright new star shining in the celestial sphere; the prefix "super-" distinguishes supernovae from ordinary novae, which also involve a star increasing in brightness, though to a lesser extent and through a different mechanism. The word supernova was coined by
Swiss astrophysicist and astronomer Fritz Zwicky,[10][11] and was first used in print in 1926.[12]
Supernova
good question,
meka benz thiyana hamuduru kenekgen ahanna one prasnayak.
samaharawita NISHANTHA danna dewal e hamuduruwaru danne nethuwa ethi.
බුදු හාමුදුරුවො කියල තියෙන්නෙ තණ්හාව අත අරින්න කියල තමයි. උන්වහන්සේ දේශනා කරල තියෙනව සංඝයාට, මාලිගාවක හිටියත් ගහක් යට ඉන්නව කියල හිතාගෙන ඉන්න කියල. ඉතින් හාමුදුරු නමකට මාලිගාවක ඉන්න එකෙයි, ගහක් යට ඉන්න එකෙයි වෙනසක් නෑ.
ඒවගේම බෙන්ස් එකක යන එකත් ගැලක යන එකත් සමානයි. ඇලෙන්නෙ නැතිව ඉන්න එක විතරයි වැදගත්.
ඔයා ඇලිල ගැලිල ඉන්න කෙනෙක් නිසයි ඔයාට ෂා බෙන්ස් එක කොච්චර හොඳද, ගැල වගේද, කොච්චර සැපක්ද කියල හිතෙන්නෙ. ඒත් ඒකෙ අනිත්ය බව වටහා ගත්තම දෙකම ඇති වෙනසක් නෑ කියල තේරේවි
ඒවගේම බෙන්ස් එකක යන එකත් ගැලක යන එකත් සමානයි. ඇලෙන්නෙ නැතිව ඉන්න එක විතරයි වැදගත්.
ඔයා ඇලිල ගැලිල ඉන්න කෙනෙක් නිසයි ඔයාට ෂා බෙන්ස් එක කොච්චර හොඳද, ගැල වගේද, කොච්චර සැපක්ද කියල හිතෙන්නෙ. ඒත් ඒකෙ අනිත්ය බව වටහා ගත්තම දෙකම ඇති වෙනසක් නෑ කියල තේරේවි
Bola kaalakanniyo, thota oya prashna thiyenawa nam atha arapu eka honda. aye reddatada ewa ahanne apen? p***yek wage
Harima sarala answer eka umba buddhagama gena melo deyak danne neha, ohe prashna ahanawa. Aasawan atha arinawa kiyana ekai, kaleta gelapena widihata jeewath wenawa kiyana ekai dekak, Buduhamuduruwange kaleth maha sanga rathnaya raja maaliga wala danata wadina kota riya peraharen aapu awastha thiyenawa. Anika Lankawe inna 1million withara hamuduruwarungen Benz pavichchi karana hamuduru waru keedenek innawada, Buddha kaleth budu maga nogiya sangaya wahansela hitiya. Api ape hema haamuduru kenekma hari kiyanne neha, onama thanaka umba wage weneth agenda walata awith mahana wechcha hamuduru waruth innawa.
ඇයි හාමුදුරු වරු පුෂ් බයිසිකලයෙනුත් යන්නේ? ඇයි හාමුදුරුවරු පයිනුත් යන්නේ (වඩින්නේ)?
වැදගත් ගමන යන එක විතරයි. යන්නෙ මොකෙන්ද කියන එක ප්රශ්නයක් නෑ.
ඊලඟට අහයි ඇයි හාමුදුරුවෝ එයා බස් එකෙන් යන්නෙ පියාඹන්නේ නැතුව කියල.ඒ විතරක්ද රටකින් රටකට යන්නේ අහස යන්තරෙන් නොවැ
මෝඩ හම්බයෝ
නිශාන්ත කිවුවට මූ බුද්ධාගම නොදන්න බව මාට්ටු වෙච්ච එකෙක්.
