BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//SpaceCatalog.org//Sky calendar//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Sky calendar
X-WR-CALDESC:The next twelve months of things that happen on a date — met
 eor showers\, eclipses\, flybys. Every instant is the same fact everywhere
  on Earth. Computed from the ephemeris by spacecatalog.org.
REFRESH-INTERVAL;VALUE=DURATION:P1D
X-PUBLISHED-TTL:P1D
BEGIN:VEVENT
UID:flyby-2026-oh3-2026-09-11@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20260911T042600Z
DTEND:20260911T052600Z
SUMMARY:2026 OH3 passes at 12.3 lunar distances
DESCRIPTION:2026 OH3\, somewhere between 142 m and 318 m across depending o
 n how dark its surface is\, makes its closest approach to Earth at 12.3 lu
 nar distances (4.7 million km)\, moving past at 20.17 km/s. At magnitude 2
 2.0 it is far below anything an amateur telescope reaches — this one is 
 a fact rather than a sight. A pass at this range is ordinary rather than a
 larming — it is the reason the object is tracked\, not a reason to worry
  about it.\n\nhttps://spacecatalog.org/calendar#2026-09
URL:https://spacecatalog.org/calendar#2026-09
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-2026-nt2-2026-09-17@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20260917T050600Z
DTEND:20260917T060600Z
SUMMARY:2026 NT2 passes at 16.1 lunar distances
DESCRIPTION:2026 NT2\, somewhere between 235 m and 525 m across depending o
 n how dark its surface is\, makes its closest approach to Earth at 16.1 lu
 nar distances (6.2 million km)\, moving past at 12.54 km/s. At magnitude 1
 8.0 it is far below anything an amateur telescope reaches — this one is 
 a fact rather than a sight. A pass at this range is ordinary rather than a
 larming — it is the reason the object is tracked\, not a reason to worry
  about it.\n\nhttps://spacecatalog.org/calendar#2026-09
URL:https://spacecatalog.org/calendar#2026-09
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-draconids-2026-10-09@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261009T012156Z
DTEND:20261009T022156Z
SUMMARY:Draconids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 21P/
 Giacobini-Zinner\, and the debris burns up at 20 km/s. Under a genuinely d
 ark sky with the radiant overhead this is worth about 5 meteors an hour 
 — a real sky and a real radiant altitude will give fewer\, and a bright 
 moon fewer still. Meteors appear all over the sky\; they only trace back t
 o Draco\, which is where to point a camera and not where to stare. It is u
 sually almost nothing\, and about once a generation a storm of thousands a
 n hour\; the slowest meteors of any shower\, and the only major one best w
 atched in the evening rather than after midnight.\n\nhttps://spacecatalog.
 org/calendar#2026-10
URL:https://spacecatalog.org/calendar#2026-10
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-southern-taurids-2026-10-10@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261010T161328Z
DTEND:20261010T171328Z
SUMMARY:Southern Taurids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 2P/E
 ncke\, and the debris burns up at 27 km/s. Under a genuinely dark sky with
  the radiant overhead this is worth about 5 meteors an hour — a real sky
  and a real radiant altitude will give fewer\, and a bright moon fewer sti
 ll. Meteors appear all over the sky\; they only trace back to Cetus\, whic
 h is where to point a camera and not where to stare. It is ten weeks of ac
 tivity at a handful an hour\, made worth watching by the fireballs — slo
 w\, orange and bright enough to cast a shadow. The radiant drifts right ac
 ross the sky over those weeks\, from Cetus in September into Taurus in Nov
 ember\, so the shower is named for where it ends up rather than where it i
 s on any one night.\n\nhttps://spacecatalog.org/calendar#2026-10
URL:https://spacecatalog.org/calendar#2026-10
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-orionids-2026-10-21@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261021T182821Z
DTEND:20261021T192821Z
SUMMARY:Orionids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 1P/H
 alley\, and the debris burns up at 66 km/s. Under a genuinely dark sky wit
 h the radiant overhead this is worth about 20 meteors an hour — a real s
 ky and a real radiant altitude will give fewer\, and a bright moon fewer s
 till. Meteors appear all over the sky\; they only trace back to Orion\, wh
 ich is where to point a camera and not where to stare. It is the other hal
 f of Halley's dust — the same comet as the η Aquariids\, met at the oth
 er place its orbit crosses ours\, and equally fast.\n\nhttps://spacecatalo
 g.org/calendar#2026-10
URL:https://spacecatalog.org/calendar#2026-10
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-2025-uk9-2026-10-31@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261031T023400Z
DTEND:20261031T033400Z
SUMMARY:2025 UK9 passes at 0.8 lunar distances
DESCRIPTION:2025 UK9\, somewhere between 3 m and 6 m across depending on ho
 w dark its surface is\, makes its closest approach to Earth at 0.8 lunar d
 istances (315 000 km)\, moving past at 7.83 km/s. At magnitude 20.1 it is 
 far below anything an amateur telescope reaches — this one is a fact rat
 her than a sight. A pass at this range is ordinary rather than alarming 
 — it is the reason the object is tracked\, not a reason to worry about i
 t.\n\nhttps://spacecatalog.org/calendar#2026-10
URL:https://spacecatalog.org/calendar#2026-10
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-524522-2026-11-02@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261102T190800Z
DTEND:20261102T200800Z
SUMMARY:524522 Zoozve (2002 VE68) passes at 15.7 lunar distances
DESCRIPTION:524522 Zoozve (2002 VE68)\, somewhere between 207 m and 464 m a
 cross depending on how dark its surface is\, makes its closest approach to
  Earth at 15.7 lunar distances (6.0 million km)\, moving past at 8.72 km/s
 . At magnitude 15.6 it is far below anything an amateur telescope reaches 
 — this one is a fact rather than a sight. A pass at this range is ordina
 ry rather than alarming — it is the reason the object is tracked\, not a
  reason to worry about it.\n\nhttps://spacecatalog.org/calendar#2026-11
URL:https://spacecatalog.org/calendar#2026-11
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-2001-kf54-2026-11-06@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261106T033700Z
DTEND:20261106T043700Z
SUMMARY:2001 KF54 passes at 18.8 lunar distances
DESCRIPTION:2001 KF54\, somewhere between 293 m and 655 m across depending 
 on how dark its surface is\, makes its closest approach to Earth at 18.8 l
 unar distances (7.2 million km)\, moving past at 16.42 km/s. At magnitude 
 15.9 it is far below anything an amateur telescope reaches — this one is
  a fact rather than a sight. A pass at this range is ordinary rather than 
 alarming — it is the reason the object is tracked\, not a reason to worr
 y about it.\n\nhttps://spacecatalog.org/calendar#2026-11
URL:https://spacecatalog.org/calendar#2026-11
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-northern-taurids-2026-11-12@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261112T181729Z
DTEND:20261112T191729Z
SUMMARY:Northern Taurids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 2P/E
 ncke\, and the debris burns up at 29 km/s. Under a genuinely dark sky with
  the radiant overhead this is worth about 5 meteors an hour — a real sky
  and a real radiant altitude will give fewer\, and a bright moon fewer sti
 ll. Meteors appear all over the sky\; they only trace back to Taurus\, whi
 ch is where to point a camera and not where to stare. It is the second bra
 nch of the same broad stream\, overlapping the first for most of November 
 and throwing the same slow fireballs.\n\nhttps://spacecatalog.org/calendar
 #2026-11
URL:https://spacecatalog.org/calendar#2026-11
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-leonids-2026-11-17@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261117T235200Z
DTEND:20261118T005200Z
SUMMARY:Leonids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 55P/
 Tempel-Tuttle\, and the debris burns up at 71 km/s. Under a genuinely dark
  sky with the radiant overhead this is worth about 15 meteors an hour — 
 a real sky and a real radiant altitude will give fewer\, and a bright moon
  fewer still. Meteors appear all over the sky\; they only trace back to Le
 o\, which is where to point a camera and not where to stare. It is the fas
 test meteors that reach us\, and the shower with the most spectacular hist
 ory — every 33 years or so\, when the parent comet has just been past\, 
 it has produced storms of tens of thousands an hour.\n\nhttps://spacecatal
 og.org/calendar#2026-11
URL:https://spacecatalog.org/calendar#2026-11
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-2016-nv-2026-12-08@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261208T184200Z
DTEND:20261208T194200Z
SUMMARY:2016 NV passes at 14.3 lunar distances
DESCRIPTION:2016 NV\, somewhere between 284 m and 634 m across depending on
  how dark its surface is\, makes its closest approach to Earth at 14.3 lun
 ar distances (5.5 million km)\, moving past at 10.42 km/s. At magnitude 15
 .0 it needs a decent telescope\, and it crosses the field fast enough to s
 ee it drift against the stars. A pass at this range is ordinary rather tha
 n alarming — it is the reason the object is tracked\, not a reason to wo
 rry about it.\n\nhttps://spacecatalog.org/calendar#2026-12
URL:https://spacecatalog.org/calendar#2026-12
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-geminids-2026-12-14@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261214T134921Z
DTEND:20261214T144921Z
SUMMARY:Geminids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 3200
  Phaethon\, and the debris burns up at 35 km/s. Under a genuinely dark sky
  with the radiant overhead this is worth about 150 meteors an hour — a r
 eal sky and a real radiant altitude will give fewer\, and a bright moon fe
 wer still. Meteors appear all over the sky\; they only trace back to Gemin
 i\, which is where to point a camera and not where to stare. It is the ric
 hest shower of the year\, and one of the two major showers whose parent is
  an asteroid rather than a comet\, the Quadrantids being the other\; mediu
 m-speed\, often yellow\, and active from mid-evening because the radiant r
 ises early.\n\nhttps://spacecatalog.org/calendar#2026-12
URL:https://spacecatalog.org/calendar#2026-12
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-ursids-2026-12-22@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20261222T221716Z
DTEND:20261222T231716Z
SUMMARY:Ursids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 8P/T
 uttle\, and the debris burns up at 33 km/s. Under a genuinely dark sky wit
 h the radiant overhead this is worth about 10 meteors an hour — a real s
 ky and a real radiant altitude will give fewer\, and a bright moon fewer s
 till. Meteors appear all over the sky\; they only trace back to Ursa Minor
 \, which is where to point a camera and not where to stare. It is a small 
 northern shower nobody watches because it falls the week of the December s
 olstice\; the radiant never sets from most of the northern hemisphere\, so
  it can be watched all night.\n\nhttps://spacecatalog.org/calendar#2026-12
URL:https://spacecatalog.org/calendar#2026-12
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-quadrantids-2027-01-04@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270104T033412Z
DTEND:20270104T043412Z
SUMMARY:Quadrantids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 1962
 56 (2003 EH₁)\, and the debris burns up at 41 km/s. Under a genuinely da
 rk sky with the radiant overhead this is worth about 110 meteors an hour 
 — a real sky and a real radiant altitude will give fewer\, and a bright 
 moon fewer still. Meteors appear all over the sky\; they only trace back t
 o Boötes\, which is where to point a camera and not where to stare. It is
  the sharpest maximum of any shower — the good hours are about six wide\
 , so the peak either falls on your night or it does not.\n\nhttps://spacec
 atalog.org/calendar#2027-01
URL:https://spacecatalog.org/calendar#2027-01
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-2020-op3-2027-01-28@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270128T233200Z
DTEND:20270129T003200Z
SUMMARY:2020 OP3 passes at 7.6 lunar distances
DESCRIPTION:2020 OP3\, somewhere between 172 m and 384 m across depending o
 n how dark its surface is\, makes its closest approach to Earth at 7.6 lun
 ar distances (2.9 million km)\, moving past at 16.86 km/s. At magnitude 18
 .0 it is far below anything an amateur telescope reaches — this one is a
  fact rather than a sight. A pass at this range is ordinary rather than al
 arming — it is the reason the object is tracked\, not a reason to worry 
 about it.\n\nhttps://spacecatalog.org/calendar#2027-01
URL:https://spacecatalog.org/calendar#2027-01
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:eclipse-solar-2027-02-06@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270206T155932Z
DTEND:20270206T165932Z
SUMMARY:Annular solar eclipse
DESCRIPTION:The Moon passes centrally across the Sun but is too far from Ea
 rth to cover it\, so at greatest eclipse — over 31.3°S\, 48.5°W — a 
 ring of Sun stays visible all the way round it\, with 86% of the disc cove
 red. It never gets dark and it is never safe to look at without a certifie
 d solar filter.\n\nhttps://spacecatalog.org/calendar#2027-02
URL:https://spacecatalog.org/calendar#2027-02
CATEGORIES:ECLIPSE
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:eclipse-lunar-2027-02-20@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270220T231244Z
DTEND:20270221T001244Z
SUMMARY:Penumbral lunar eclipse
DESCRIPTION:The Moon passes through the soft outer edge of Earth's shadow\,
  not the dark core of it. The whole disc dims slightly and unevenly — en
 ough to notice in a photograph taken before and after\, and easy to miss b
 y eye.\n\nhttps://spacecatalog.org/calendar#2027-02
URL:https://spacecatalog.org/calendar#2027-02
CATEGORIES:ECLIPSE
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-474158-2027-03-04@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270304T050000Z
DTEND:20270304T060000Z
SUMMARY:474158 (1999 FA) passes at 16.5 lunar distances
DESCRIPTION:474158 (1999 FA)\, somewhere between 192 m and 429 m across dep
 ending on how dark its surface is\, makes its closest approach to Earth at
  16.5 lunar distances (6.4 million km)\, moving past at 6.63 km/s. At magn
 itude 16.6 it is far below anything an amateur telescope reaches — this 
 one is a fact rather than a sight. A pass at this range is ordinary rather
  than alarming — it is the reason the object is tracked\, not a reason t
 o worry about it.\n\nhttps://spacecatalog.org/calendar#2027-03
URL:https://spacecatalog.org/calendar#2027-03
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-535844-2027-03-04@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270304T205800Z
DTEND:20270304T215800Z
SUMMARY:535844 (2015 BY310) passes at 9.2 lunar distances
DESCRIPTION:535844 (2015 BY310)\, somewhere between 111 m and 249 m across 
 depending on how dark its surface is\, makes its closest approach to Earth
  at 9.2 lunar distances (3.5 million km)\, moving past at 8.02 km/s. At ma
 gnitude 16.2 it is far below anything an amateur telescope reaches — thi
 s one is a fact rather than a sight. A pass at this range is ordinary rath
 er than alarming — it is the reason the object is tracked\, not a reason
  to worry about it.\n\nhttps://spacecatalog.org/calendar#2027-03
URL:https://spacecatalog.org/calendar#2027-03
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-506074-2027-03-18@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270318T192800Z
DTEND:20270318T202800Z
SUMMARY:506074 Svarog (2015 UM67) passes at 19.0 lunar distances
DESCRIPTION:506074 Svarog (2015 UM67)\, 665 m across\, makes its closest ap
 proach to Earth at 19.0 lunar distances (7.3 million km)\, moving past at 
 22.41 km/s. At magnitude 15.2 it is far below anything an amateur telescop
 e reaches — this one is a fact rather than a sight. A pass at this range
  is ordinary rather than alarming — it is the reason the object is track
 ed\, not a reason to worry about it.\n\nhttps://spacecatalog.org/calendar#
 2027-03
URL:https://spacecatalog.org/calendar#2027-03
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-lyrids-2027-04-23@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270423T014916Z
DTEND:20270423T024916Z
SUMMARY:Lyrids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by C/18
 61 G1 (Thatcher)\, and the debris burns up at 49 km/s. Under a genuinely d
 ark sky with the radiant overhead this is worth about 18 meteors an hour 
 — a real sky and a real radiant altitude will give fewer\, and a bright 
 moon fewer still. Meteors appear all over the sky\; they only trace back t
 o Hercules\, close to Vega\, which is where to point a camera and not wher
 e to stare. It is the oldest shower on record\, watched from China in 687 
 BC\, and still capable of a brief outburst nobody predicted.\n\nhttps://sp
 acecatalog.org/calendar#2027-04
URL:https://spacecatalog.org/calendar#2027-04
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-eta-aquariids-2027-05-06@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270506T151935Z
DTEND:20270506T161935Z
SUMMARY:η Aquariids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 1P/H
 alley\, and the debris burns up at 66 km/s. Under a genuinely dark sky wit
 h the radiant overhead this is worth about 50 meteors an hour — a real s
 ky and a real radiant altitude will give fewer\, and a bright moon fewer s
 till. Meteors appear all over the sky\; they only trace back to Aquarius\,
  which is where to point a camera and not where to stare. It is dust from 
 Halley's Comet\, hitting the atmosphere almost head-on and leaving glowing
  trains that hang for seconds\; much better from the southern hemisphere\,
  where the radiant climbs before dawn instead of skimming the horizon.\n\n
 https://spacecatalog.org/calendar#2027-05
URL:https://spacecatalog.org/calendar#2027-05
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-4953-2027-06-06@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270606T224200Z
DTEND:20270606T234200Z
SUMMARY:4953 (1990 MU) passes at 12.0 lunar distances
DESCRIPTION:4953 (1990 MU)\, somewhere between 2.8 km and 6.3 km across dep
 ending on how dark its surface is\, makes its closest approach to Earth at
  12.0 lunar distances (4.6 million km)\, moving past at 23.82 km/s. At mag
 nitude 9.9 it is a binocular object\, moving fast enough across the stars 
 to watch it move. A pass at this range is ordinary rather than alarming 
 — it is the reason the object is tracked\, not a reason to worry about i
 t.\n\nhttps://spacecatalog.org/calendar#2027-06
URL:https://spacecatalog.org/calendar#2027-06
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-456938-2027-06-28@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270628T181500Z
DTEND:20270628T191500Z
SUMMARY:456938 (2007 YV56) passes at 19.6 lunar distances
DESCRIPTION:456938 (2007 YV56)\, somewhere between 169 m and 379 m across d
 epending on how dark its surface is\, makes its closest approach to Earth 
 at 19.6 lunar distances (7.5 million km)\, moving past at 17.79 km/s. At m
 agnitude 17.8 it is far below anything an amateur telescope reaches — th
 is one is a fact rather than a sight. A pass at this range is ordinary rat
 her than alarming — it is the reason the object is tracked\, not a reaso
 n to worry about it.\n\nhttps://spacecatalog.org/calendar#2027-06
URL:https://spacecatalog.org/calendar#2027-06
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:eclipse-lunar-2027-07-18@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270718T160254Z
DTEND:20270718T170254Z
SUMMARY:Penumbral lunar eclipse
DESCRIPTION:The Moon passes through the soft outer edge of Earth's shadow\,
  not the dark core of it. The whole disc dims slightly and unevenly — en
 ough to notice in a photograph taken before and after\, and easy to miss b
 y eye.\n\nhttps://spacecatalog.org/calendar#2027-07
URL:https://spacecatalog.org/calendar#2027-07
CATEGORIES:ECLIPSE
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-alpha-capricornids-2027-07-30@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270730T184021Z
DTEND:20270730T194021Z
SUMMARY:α Capricornids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 169P
 /NEAT\, and the debris burns up at 23 km/s. Under a genuinely dark sky wit
 h the radiant overhead this is worth about 5 meteors an hour — a real sk
 y and a real radiant altitude will give fewer\, and a bright moon fewer st
 ill. Meteors appear all over the sky\; they only trace back to Capricornus
 \, which is where to point a camera and not where to stare. It is slow and
  bright rather than numerous — the rate is low but a good fraction of wh
 at it does produce are fireballs\, and both hemispheres see it equally.\n\
 nhttps://spacecatalog.org/calendar#2027-07
URL:https://spacecatalog.org/calendar#2027-07
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-southern-delta-aquariids-2027-07-30@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270730T184021Z
DTEND:20270730T194021Z
SUMMARY:Southern δ Aquariids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 96P/
 Machholz\, and the debris burns up at 41 km/s. Under a genuinely dark sky 
 with the radiant overhead this is worth about 25 meteors an hour — a rea
 l sky and a real radiant altitude will give fewer\, and a bright moon fewe
 r still. Meteors appear all over the sky\; they only trace back to Aquariu
 s\, which is where to point a camera and not where to stare. It is a broad
 \, faint stream with no sharp peak\, best from the southern hemisphere and
  from southern latitudes in the north.\n\nhttps://spacecatalog.org/calenda
 r#2027-07
URL:https://spacecatalog.org/calendar#2027-07
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:eclipse-solar-2027-08-02@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270802T100634Z
DTEND:20270802T110634Z
SUMMARY:Total solar eclipse
DESCRIPTION:The Moon covers the Sun completely along a narrow track across 
 the Earth\, and takes a bite out of it for a wide margin either side. Grea
 test eclipse falls over 25.5°N\, 33.2°E — being on that track is the w
 hole difference between a total eclipse and a partial one\, and this page 
 does not know where you are standing. Never look at any phase of it withou
 t a certified solar filter.\n\nhttps://spacecatalog.org/calendar#2027-08
URL:https://spacecatalog.org/calendar#2027-08
CATEGORIES:ECLIPSE
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-137108-2027-08-07@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270807T070900Z
DTEND:20270807T080900Z
SUMMARY:137108 (1999 AN10) passes at 1.0 lunar distances
DESCRIPTION:137108 (1999 AN10)\, somewhere between 653 m and 1.5 km across 
 depending on how dark its surface is\, makes its closest approach to Earth
  at 1.0 lunar distances (390 000 km)\, moving past at 26.28 km/s. At magni
 tude 7.8 it is a binocular object\, moving fast enough across the stars to
  watch it move. A pass at this range is ordinary rather than alarming — 
 it is the reason the object is tracked\, not a reason to worry about it.\n
 \nhttps://spacecatalog.org/calendar#2027-08
URL:https://spacecatalog.org/calendar#2027-08
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:shower-perseids-2027-08-13@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270813T081914Z
DTEND:20270813T091914Z
SUMMARY:Perseids at maximum
DESCRIPTION:The Earth crosses the densest part of a dust trail left by 109P
 /Swift-Tuttle\, and the debris burns up at 59 km/s. Under a genuinely dark
  sky with the radiant overhead this is worth about 100 meteors an hour —
  a real sky and a real radiant altitude will give fewer\, and a bright moo
 n fewer still. Meteors appear all over the sky\; they only trace back to P
 erseus\, which is where to point a camera and not where to stare. It is th
 e reliable one\, and the one that falls in the northern hemisphere's warme
 st nights — bright\, fast\, and often leaving persistent trains.\n\nhttp
 s://spacecatalog.org/calendar#2027-08
URL:https://spacecatalog.org/calendar#2027-08
CATEGORIES:METEORS
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:eclipse-lunar-2027-08-17@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270817T071344Z
DTEND:20270817T081344Z
SUMMARY:Penumbral lunar eclipse
DESCRIPTION:The Moon passes through the soft outer edge of Earth's shadow\,
  not the dark core of it. The whole disc dims slightly and unevenly — en
 ough to notice in a photograph taken before and after\, and easy to miss b
 y eye.\n\nhttps://spacecatalog.org/calendar#2027-08
URL:https://spacecatalog.org/calendar#2027-08
CATEGORIES:ECLIPSE
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-2017-qw17-2027-08-19@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270819T043600Z
DTEND:20270819T053600Z
SUMMARY:2017 QW17 passes at 17.8 lunar distances
DESCRIPTION:2017 QW17\, somewhere between 126 m and 281 m across depending 
 on how dark its surface is\, makes its closest approach to Earth at 17.8 l
 unar distances (6.8 million km)\, moving past at 19.86 km/s. At magnitude 
 17.4 it is far below anything an amateur telescope reaches — this one is
  a fact rather than a sight. A pass at this range is ordinary rather than 
 alarming — it is the reason the object is tracked\, not a reason to worr
 y about it.\n\nhttps://spacecatalog.org/calendar#2027-08
URL:https://spacecatalog.org/calendar#2027-08
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
BEGIN:VEVENT
UID:flyby-826799-2027-08-29@spacecatalog.org
DTSTAMP:20260908T000000Z
DTSTART:20270829T054900Z
DTEND:20270829T064900Z
SUMMARY:826799 (2023 OE6) passes at 16.7 lunar distances
DESCRIPTION:826799 (2023 OE6)\, somewhere between 285 m and 637 m across de
 pending on how dark its surface is\, makes its closest approach to Earth a
 t 16.7 lunar distances (6.4 million km)\, moving past at 25.21 km/s. At ma
 gnitude 16.5 it is far below anything an amateur telescope reaches — thi
 s one is a fact rather than a sight. A pass at this range is ordinary rath
 er than alarming — it is the reason the object is tracked\, not a reason
  to worry about it.\n\nhttps://spacecatalog.org/calendar#2027-08
URL:https://spacecatalog.org/calendar#2027-08
CATEGORIES:FLYBY
TRANSP:TRANSPARENT
STATUS:CONFIRMED
END:VEVENT
END:VCALENDAR