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VERSION:2.0
PRODID:-//Mazalogy//Moon phase references//PT
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Um mês ao meio-dia local
BEGIN:VEVENT
UID:last-quarter-20261003T132533Z@mazalogy.com
DTSTAMP:20261014T120000Z
DTSTART:20261003T132533Z
DURATION:PT1M
SUMMARY:Quarto minguante
DESCRIPTION:Leia o instante\, a amostra e a fonte\n{"engine":"Astronomy Eng
 ine 2.1.19"\,"engineVersion":"2.1.19"\,"engineLicense":"MIT"\,"center":"ge
 ocentric"\,"frame":"apparent ecliptic longitude of date relative to the Su
 n"\,"clock":"UTC instants\; IANA-zone civil display uses the runtime time-
 zone database"\,"eventDefinition":"Primary phases are Moon minus Sun geoce
 ntric ecliptic longitude 0°\, 90°\, 180° and 270°."\,"illumination":"I
 llumination(Moon).phase_fraction is the fraction of the disk illuminated a
 s seen from Earth\; it is not inferred from a rounded phase angle."\,"samp
 leConvention":"One sample at 12:00 local civil time on each date in the se
 lected zone. A missing noon has no sample. A repeated noon uses the earlie
 r occurrence and retains every candidate instant."\,"phaseLabels":"Interme
 diate sample labels use waxing/waning and calculated illumination. A prima
 ry label is used only within 0.0001° of its defining longitude\; exact ev
 ent enumeration is separate."\,"primaryLabelToleranceDegrees":0.0001\,"sup
 portedInputRange":"Gregorian month inputs 1800–2100. Public UTC instant 
 inputs include 1799-12-30 through 2101-01-02 so every boundary local-noon 
 sample remains reproducible."\,"monthRange":{"minYear":1800\,"maxYear":210
 0\,"minDate":"1800-01-01"\,"maxDate":"2100-12-31"}\,"instantRange":{"minDa
 te":"1799-12-30"\,"maxDate":"2101-01-02"\,"min":"1799-12-30T00:00:00.000Z"
 \,"max":"2101-01-02T23:59:59.999Z"}\,"timePrecision":"Computed ISO timesta
 mps retain seconds and milliseconds for reproducibility\, not a claim of e
 quivalent physical accuracy. The engine approximates UT1 and UTC\; indepen
 dent USNO primary-event checks use published UT1 minute values with a 120-
 second tolerance."\,"historicalTimeZones":"Before 1970\, historical clock 
 offsets may vary across runtime time-zone databases. Future civil-time rul
 es can also change."}\nA Lua nova astronômica é uma conjunção. Rosh Ch
 odesh segue o calendário hebraico fixo\; o molad tradicional é um cálcu
 lo de movimento médio. As duas datas hebraicas são possibilidades antes 
 e depois do limite do anoitecer. Aqui não se calcula um lugar nem o pôr 
 do sol.\nOne-minute reference marker for a calculated instant\; not a phas
 e duration.\nhttps://mazalogy.com/pt/moon-phases/
URL:https://mazalogy.com/pt/moon-phases/
TRANSP:TRANSPARENT
END:VEVENT
BEGIN:VEVENT
UID:new-20261010T155036Z@mazalogy.com
DTSTAMP:20261014T120000Z
DTSTART:20261010T155036Z
DURATION:PT1M
SUMMARY:Lua nova
DESCRIPTION:Leia o instante\, a amostra e a fonte\n{"engine":"Astronomy Eng
 ine 2.1.19"\,"engineVersion":"2.1.19"\,"engineLicense":"MIT"\,"center":"ge
 ocentric"\,"frame":"apparent ecliptic longitude of date relative to the Su
 n"\,"clock":"UTC instants\; IANA-zone civil display uses the runtime time-
 zone database"\,"eventDefinition":"Primary phases are Moon minus Sun geoce
 ntric ecliptic longitude 0°\, 90°\, 180° and 270°."\,"illumination":"I
 llumination(Moon).phase_fraction is the fraction of the disk illuminated a
 s seen from Earth\; it is not inferred from a rounded phase angle."\,"samp
 leConvention":"One sample at 12:00 local civil time on each date in the se
 lected zone. A missing noon has no sample. A repeated noon uses the earlie
 r occurrence and retains every candidate instant."\,"phaseLabels":"Interme
 diate sample labels use waxing/waning and calculated illumination. A prima
 ry label is used only within 0.0001° of its defining longitude\; exact ev
 ent enumeration is separate."\,"primaryLabelToleranceDegrees":0.0001\,"sup
 portedInputRange":"Gregorian month inputs 1800–2100. Public UTC instant 
 inputs include 1799-12-30 through 2101-01-02 so every boundary local-noon 
 sample remains reproducible."\,"monthRange":{"minYear":1800\,"maxYear":210
 0\,"minDate":"1800-01-01"\,"maxDate":"2100-12-31"}\,"instantRange":{"minDa
 te":"1799-12-30"\,"maxDate":"2101-01-02"\,"min":"1799-12-30T00:00:00.000Z"
 \,"max":"2101-01-02T23:59:59.999Z"}\,"timePrecision":"Computed ISO timesta
 mps retain seconds and milliseconds for reproducibility\, not a claim of e
 quivalent physical accuracy. The engine approximates UT1 and UTC\; indepen
 dent USNO primary-event checks use published UT1 minute values with a 120-
 second tolerance."\,"historicalTimeZones":"Before 1970\, historical clock 
 offsets may vary across runtime time-zone databases. Future civil-time rul
 es can also change."}\nA Lua nova astronômica é uma conjunção. Rosh Ch
 odesh segue o calendário hebraico fixo\; o molad tradicional é um cálcu
 lo de movimento médio. As duas datas hebraicas são possibilidades antes 
 e depois do limite do anoitecer. Aqui não se calcula um lugar nem o pôr 
 do sol.\nOne-minute reference marker for a calculated instant\; not a phas
 e duration.\nhttps://mazalogy.com/pt/moon-phases/
URL:https://mazalogy.com/pt/moon-phases/
TRANSP:TRANSPARENT
END:VEVENT
BEGIN:VEVENT
UID:first-quarter-20261018T161319Z@mazalogy.com
DTSTAMP:20261014T120000Z
DTSTART:20261018T161319Z
DURATION:PT1M
SUMMARY:Quarto crescente
DESCRIPTION:Leia o instante\, a amostra e a fonte\n{"engine":"Astronomy Eng
 ine 2.1.19"\,"engineVersion":"2.1.19"\,"engineLicense":"MIT"\,"center":"ge
 ocentric"\,"frame":"apparent ecliptic longitude of date relative to the Su
 n"\,"clock":"UTC instants\; IANA-zone civil display uses the runtime time-
 zone database"\,"eventDefinition":"Primary phases are Moon minus Sun geoce
 ntric ecliptic longitude 0°\, 90°\, 180° and 270°."\,"illumination":"I
 llumination(Moon).phase_fraction is the fraction of the disk illuminated a
 s seen from Earth\; it is not inferred from a rounded phase angle."\,"samp
 leConvention":"One sample at 12:00 local civil time on each date in the se
 lected zone. A missing noon has no sample. A repeated noon uses the earlie
 r occurrence and retains every candidate instant."\,"phaseLabels":"Interme
 diate sample labels use waxing/waning and calculated illumination. A prima
 ry label is used only within 0.0001° of its defining longitude\; exact ev
 ent enumeration is separate."\,"primaryLabelToleranceDegrees":0.0001\,"sup
 portedInputRange":"Gregorian month inputs 1800–2100. Public UTC instant 
 inputs include 1799-12-30 through 2101-01-02 so every boundary local-noon 
 sample remains reproducible."\,"monthRange":{"minYear":1800\,"maxYear":210
 0\,"minDate":"1800-01-01"\,"maxDate":"2100-12-31"}\,"instantRange":{"minDa
 te":"1799-12-30"\,"maxDate":"2101-01-02"\,"min":"1799-12-30T00:00:00.000Z"
 \,"max":"2101-01-02T23:59:59.999Z"}\,"timePrecision":"Computed ISO timesta
 mps retain seconds and milliseconds for reproducibility\, not a claim of e
 quivalent physical accuracy. The engine approximates UT1 and UTC\; indepen
 dent USNO primary-event checks use published UT1 minute values with a 120-
 second tolerance."\,"historicalTimeZones":"Before 1970\, historical clock 
 offsets may vary across runtime time-zone databases. Future civil-time rul
 es can also change."}\nA Lua nova astronômica é uma conjunção. Rosh Ch
 odesh segue o calendário hebraico fixo\; o molad tradicional é um cálcu
 lo de movimento médio. As duas datas hebraicas são possibilidades antes 
 e depois do limite do anoitecer. Aqui não se calcula um lugar nem o pôr 
 do sol.\nOne-minute reference marker for a calculated instant\; not a phas
 e duration.\nhttps://mazalogy.com/pt/moon-phases/
URL:https://mazalogy.com/pt/moon-phases/
TRANSP:TRANSPARENT
END:VEVENT
BEGIN:VEVENT
UID:full-20261026T041215Z@mazalogy.com
DTSTAMP:20261014T120000Z
DTSTART:20261026T041215Z
DURATION:PT1M
SUMMARY:Lua cheia
DESCRIPTION:Leia o instante\, a amostra e a fonte\n{"engine":"Astronomy Eng
 ine 2.1.19"\,"engineVersion":"2.1.19"\,"engineLicense":"MIT"\,"center":"ge
 ocentric"\,"frame":"apparent ecliptic longitude of date relative to the Su
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 zone database"\,"eventDefinition":"Primary phases are Moon minus Sun geoce
 ntric ecliptic longitude 0°\, 90°\, 180° and 270°."\,"illumination":"I
 llumination(Moon).phase_fraction is the fraction of the disk illuminated a
 s seen from Earth\; it is not inferred from a rounded phase angle."\,"samp
 leConvention":"One sample at 12:00 local civil time on each date in the se
 lected zone. A missing noon has no sample. A repeated noon uses the earlie
 r occurrence and retains every candidate instant."\,"phaseLabels":"Interme
 diate sample labels use waxing/waning and calculated illumination. A prima
 ry label is used only within 0.0001° of its defining longitude\; exact ev
 ent enumeration is separate."\,"primaryLabelToleranceDegrees":0.0001\,"sup
 portedInputRange":"Gregorian month inputs 1800–2100. Public UTC instant 
 inputs include 1799-12-30 through 2101-01-02 so every boundary local-noon 
 sample remains reproducible."\,"monthRange":{"minYear":1800\,"maxYear":210
 0\,"minDate":"1800-01-01"\,"maxDate":"2100-12-31"}\,"instantRange":{"minDa
 te":"1799-12-30"\,"maxDate":"2101-01-02"\,"min":"1799-12-30T00:00:00.000Z"
 \,"max":"2101-01-02T23:59:59.999Z"}\,"timePrecision":"Computed ISO timesta
 mps retain seconds and milliseconds for reproducibility\, not a claim of e
 quivalent physical accuracy. The engine approximates UT1 and UTC\; indepen
 dent USNO primary-event checks use published UT1 minute values with a 120-
 second tolerance."\,"historicalTimeZones":"Before 1970\, historical clock 
 offsets may vary across runtime time-zone databases. Future civil-time rul
 es can also change."}\nA Lua nova astronômica é uma conjunção. Rosh Ch
 odesh segue o calendário hebraico fixo\; o molad tradicional é um cálcu
 lo de movimento médio. As duas datas hebraicas são possibilidades antes 
 e depois do limite do anoitecer. Aqui não se calcula um lugar nem o pôr 
 do sol.\nOne-minute reference marker for a calculated instant\; not a phas
 e duration.\nhttps://mazalogy.com/pt/moon-phases/
URL:https://mazalogy.com/pt/moon-phases/
TRANSP:TRANSPARENT
END:VEVENT
END:VCALENDAR