This eclipse is visible in Tokyo - go to local timings and animation
What This Lunar Eclipse Looks Like
The curvature of the shadow's path and the apparent rotation of the Moon's disk is due to the Earth's rotation.
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Regions seeing, at least, some parts of the eclipse: Europe, Much of Asia, Much of Australia, Much of Africa, North America, South America, Pacific, Atlantic, Arctic, Antarctica.
Expand for a list of selected cities where at least part of the total eclipse is visible Stockholm, Sweden Copenhagen, Denmark Brussels, Brussels, Belgium Honolulu, Hawaii, USA Santiago, Chile Los Angeles, California, USA São Paulo, São Paulo, Brazil Buenos Aires, Argentina Amsterdam, Netherlands Mexico City, Ciudad de México, Mexico Caracas, Venezuela Lisbon, Lisbon, Portugal Lima, Lima, Peru Detroit, Michigan, USA Montréal, Quebec, Canada Havana, Cuba Casablanca, Morocco London, England, United Kingdom Dublin, Ireland Paris, Paris, France San Salvador, El Salvador Washington DC, District of Columbia, USA Santo Domingo, Dominican Republic Guatemala City, Guatemala New York, New York, USA San Francisco, California, USA Toronto, Ontario, Canada Chicago, Illinois, USA Rio de Janeiro, Rio de Janeiro, Brazil Madrid, Madrid, Spain Expand for a list of selected cities where the partial eclipse is visible Khartoum, Sudan Cairo, Egypt Ankara, Turkey Moscow, Moscow, Russia Athens, Greece Bucharest, Romania Sofia, Bulgaria Lagos, Lagos, Nigeria Budapest, Hungary Warsaw, Poland Zagreb, Croatia Vienna, Vienna, Austria Rome, Italy Algiers, Algeria Berlin, Berlin, Germany Tokyo, Japan Brisbane, Queensland, Australia Sydney, New South Wales, Australia Seoul, South Korea Shanghai, Shanghai Municipality, China Melbourne, Victoria, Australia Beijing, Beijing Municipality, China Taipei, Taiwan Manila, Philippines This eclipse is visible in Tokyo - go to local timings and animation
Eclipse Map and Animation The animation shows where this total lunar eclipse is visible during the night (dark “wave” slowly moving across the Earth's surface).
Shades of darkness Night, moon high up in sky.
Moon between 12 and 18 degrees above horizon.
Moon between 6 and 12 degrees above horizon. Make sure you have free line of sight.
Moon between 0 and 6 degrees above horizon. May be hard to see due to brightness and line of sight.
Day, moon and eclipse both not visible.
Note: Twilight will affect the visibility of the eclipse, as well as weather.
The entire eclipse is visible from start to end.
The entire partial and total phases are visible. Misses part of penumbral phase.
The entire total phase is visible. Misses part of partial & penumbral phases.
Some of the total phase is visible. Misses part of total, partial & penumbral phases.
Some of the partial phase is visible. Misses total phase and part of partial & penumbral phases.
Some of the penumbral phase is visible. Misses total & partial phases.
The eclipse is not visible at all.
Note: Areas with lighter shadings left (West) of the center will experience the eclipse after moonrise/sunset. Areas with lighter shadings right (East) of the center will experience the eclipse until moonset/sunrise. Actual eclipse visibility depends on weather conditions and line of sight to the Moon.
When the Eclipse Happens Worldwide — Timeline Lunar eclipses can be visible from everywhere on the night side of the Earth, if the sky is clear. From some places the entire eclipse will be visible, while in other areas the Moon will rise or set during the eclipse.
Eclipse Stages Worldwide UTC Time Local Time in Tokyo* Visible in Tokyo Penumbral Eclipse begins 2月3日 (金)4時15分05秒 2月3日 (金)13時15分05秒 No, below the horizon Partial Eclipse begins 2月3日 (金)5時28分03秒 2月3日 (金)14時28分03秒 No, below the horizon Full Eclipse begins 2月3日 (金)6時45分00秒 2月3日 (金)15時45分00秒 No, below the horizon Maximum Eclipse 2月3日 (金)7時16分46秒 2月3日 (金)16時16分46秒 No, below the horizon Full Eclipse ends 2月3日 (金)7時48分34秒 2月3日 (金)16時48分34秒 No, below the horizon Partial Eclipse ends 2月3日 (金)9時05分31秒 2月3日 (金)18時05分31秒 Yes Penumbral Eclipse ends 2月3日 (金)10時18分24秒 2月3日 (金)19時18分24秒 Yes
* The Moon is below the horizon in Tokyo some of the time, so that part of the eclipse is not visible.
Quick Facts About This Eclipse Data Value Comments Magnitude 1.168 Fraction of the Moon’s diameter covered by Earth’s umbra Obscuration 100.0% Percentage of the Moon's area covered by Earth's umbra Penumbral magnitude 2.259 Fraction of the Moon's diameter covered by Earth's penumbra Overall duration 6 hours, 3 minutes Period between the beginning and end of all eclipse phases Duration of totality 1 hour, 4 minutes Period between the beginning and end of the total phase Duration of partial phases 2 hours, 34 minutes Combined period of both partial phases Duration of penumbral phases 2 hours, 26 minutes Combined period of both penumbral phases
Eclipse calculations usually accurate to a few seconds
An Eclipse Never Comes Alone! A solar eclipse always occurs about two weeks before or after a lunar eclipse.
Usually, there are two eclipses in a row, but other times, there are three during the same eclipse season.
All eclipses 1900 — 2199
This is the second eclipse this season.
First eclipse this season: 2102年1月19日木曜日 — Partial Solar Eclipse
How accurate is the eclipse calculation