by APOD Robot » Sun Nov 10, 2019 5:09 am
A Mercury Transit Sequence
Explanation: Tomorrow -- Monday --
Mercury will cross the
face of the
Sun, as
seen from Earth. Called a
transit, the last time this happened was in
2016. Because the
plane of Mercury's orbit is not exactly coincident with the
plane of Earth's orbit, Mercury usually
appears to pass over or under the Sun. The featured time-lapse sequence, superimposed on a single frame, was taken from a balcony in
Belgium shows the entire
transit of 2003 May 7. That
solar crossing lasted over five hours, so that the above 23 images were taken roughly 15 minutes apart. The
north pole of the
Sun, the
Earth's orbit, and
Mercury's orbit, although all different, all occur in directions slightly above the left of the image. Near the center and on the far right,
sunspots are visible. After
Monday, the next
transit of Mercury will occur in 2032.
[url=https://apod.nasa.gov/apod/ap191110.html] [img]https://apod.nasa.gov/apod/calendar/S_191110.jpg[/img] [size=150]A Mercury Transit Sequence[/size][/url]
[b] Explanation: [/b] Tomorrow -- Monday -- [url=https://solarsystem.nasa.gov/planets/mercury/overview/]Mercury[/url] will cross the [url=https://apod.nasa.gov/apod/ap060925.html]face[/url] of the [url=http://apod.nasa.gov/apod/sun.html]Sun[/url], as [url=https://nightsky.jpl.nasa.gov/download-view.cfm?Doc_ID=653]seen[/url] from Earth. Called a [url=https://en.wikipedia.org/wiki/Transit_(astronomy)]transit[/url], the last time this happened was in [url=https://apod.nasa.gov/apod/ap160511.html]2016[/url]. Because the [url=https://mathinsight.org/applet/plane_three_points]plane[/url] of Mercury's orbit is not exactly coincident with the [url=https://apod.nasa.gov/apod/ap001014.html]plane of Earth's orbit[/url], Mercury usually [url=http://eclipse.gsfc.nasa.gov/transit/catalog/MercuryCatalog.html]appears[/url] to pass over or under the Sun. The featured time-lapse sequence, superimposed on a single frame, was taken from a balcony in [url=https://en.wikipedia.org/wiki/Belgium]Belgium[/url] shows the entire [url=https://apod.nasa.gov/apod/ap030508.html]transit[/url] of 2003 May 7. That [url=https://apod.nasa.gov/apod/ap030513.html]solar crossing[/url] lasted over five hours, so that the above 23 images were taken roughly 15 minutes apart. The [url=https://apod.nasa.gov/apod/ap040919.html]north pole[/url] of the [url=https://solarsystem.nasa.gov/solar-system/sun/overview/]Sun[/url], the [url=https://apod.nasa.gov/apod/ap001020.html]Earth[/url]'s orbit, and [url=https://solarsystem.nasa.gov/planets/mercury/in-depth/]Mercury[/url]'s orbit, although all different, all occur in directions slightly above the left of the image. Near the center and on the far right, [url=https://apod.nasa.gov/apod/ap000223.html]sunspot[/url]s are visible. After [url=https://www.youtube.com/watch?v=lu9ASSZQEbg]Monday[/url], the next [url=https://en.wikipedia.org/wiki/Transit_of_Mercury]transit of Mercury[/url] will occur in 2032.
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