Lunar eclipse february 17 2020 horoscope

But a lunar eclipse, specifically, is a bit different. For one, a lunar eclipse can be seen almost entirely in the half of the Earth that is experiencing night. And you'll be able to see the next eclipse which is Penumbral on January 10th, But before we dive into exactly how eclipses work—and how and where you can see it—let's delve into a little bit of science, plus everything else we know about when the next lunar eclipse will take place.

All eclipses happen because of the interactions between the sun, moon, and Earth.

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What makes a lunar and solar eclipse different is, surprisingly, the position of the moon. In August , a huge chunk of America saw a total solar eclipse, which is when the moon moves between the Earth and the sun to block out the sun from view. In a lunar eclipse, though, the moon is in a different position. A lunar eclipse happens because the Earth comes between the sun and the moon in such a way that the shadow of our planet is either partially or entirely covering our view of the moon—hence the lunar eclipse.

It's rare because the moon has to be in just the right part of its orbit for this to happen—and, yes, it can only happen when the moon is full. It might be a bit confusing to learn, but the three different types of lunar eclipses are: Penumbral, partial, and total. The most recognizable lunar eclipse type is the total eclipse, which happens when the entire moon passes through the Earth's umbral shadow.

In this case, the moon appears red or orange to us humans below—but more on that later. Meanwhile, a partial lunar eclipse is when a portion of the moon passes through the Earth's umbral shadow and it basically looks like a large part of the moon is covered by a shadow. Here's where things get even more complicated: A Penumbral eclipse happens when the moon passes through the Earth's Penumbral shadow.

In this type of eclipse, none of the moon is completely shaded by the Earth's umbra which is the fully shaded inner region of a shadow. This is the weakest type of eclipse—but still a pretty cool one to see if you can spot it. You already know that a total lunar eclipse is when the moon passes completely under the Earth's umbral shadow.

However, the moon doesn't completely disappear. Instead, it appears completely, just in shadows—and is hard to see if you are not looking for the eclipse, according to Space. Look for this impressive sight in the east just before sunrise. A total lunar eclipse occurs when the Moon passes completely through the Earth's dark shadow, or umbra. During this type of eclipse, the Moon will gradually get darker and then take on a rusty or blood red color.

February 4 - New Moon. February 19 - Full Moon, Supermoon. This full moon was known by early Native American tribes as the Full Snow Moon because the heaviest snows usually fell during this time of the year. Since hunting is difficult, this moon has also been known by some tribes as the Full Hunger Moon, since the harsh weather made hunting difficult.

This is also the second of three supermoons for February 27 - Mercury at Greatest Eastern Elongation. The planet Mercury reaches greatest eastern elongation of This is the best time to view Mercury since it will be at its highest point above the horizon in the evening sky. Look for the planet low in the western sky just after sunset. March 6 - New Moon. March 20 - March Equinox. The March equinox occurs at UTC. The Sun will shine directly on the equator and there will be nearly equal amounts of day and night throughout the world. This is also the first day of spring vernal equinox in the Northern Hemisphere and the first day of fall autumnal equinox in the Southern Hemisphere.

March 21 - Full Moon, Supermoon. This full moon was known by early Native American tribes as the Full Worm Moon because this was the time of year when the ground would begin to soften and the earthworms would reappear. This is also the last of three supermoons for April 5 - New Moon. April 11 - Mercury at Greatest Western Elongation. The planet Mercury reaches greatest western elongation of This is the best time to view Mercury since it will be at its highest point above the horizon in the morning sky.

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Look for the planet low in the eastern sky just before sunrise. April 19 - Full Moon. This full moon was known by early Native American tribes as the Full Pink Moon because it marked the appearance of the moss pink, or wild ground phlox, which is one of the first spring flowers. Many coastal tribes called it the Full Fish Moon because this was the time that the shad swam upstream to spawn. April 22, 23 - Lyrids Meteor Shower. The Lyrids is an average shower, usually producing about 20 meteors per hour at its peak.

The shower runs annually from April It peaks this year on the night of the night of the 22nd and morning of the 23rd. These meteors can sometimes produce bright dust trails that last for several seconds.

The waning gibbous moon will block out many of the fainter meteors this year, but if you are patient you should still be able to catch a few of the brightest ones. Meteors will radiate from the constellation Lyra, but can appear anywhere in the sky. May 4 - New Moon. May 6, 7 - Eta Aquarids Meteor Shower. The Eta Aquarids is an above average shower, capable of producing up to 60 meteors per hour at its peak.

Most of the activity is seen in the Southern Hemisphere. In the Northern Hemisphere, the rate can reach about 30 meteors per hour. It is produced by dust particles left behind by comet Halley, which has known and observed since ancient times. The shower runs annually from April 19 to May It peaks this year on the night of May 6 and the morning of the May 7. The thin crescent moon will set early in the evening leaving dark skies for what should be a good show. Meteors will radiate from the constellation Aquarius, but can appear anywhere in the sky.

May 18 - Full Moon, Blue Moon. This full moon was known by early Native American tribes as the Full Flower Moon because this was the time of year when spring flowers appeared in abundance. Since this is the third of four full moons in this season, it is known as a blue moon. But since full moons occur every The extra full moon of the season is known as a blue moon.

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Blue moons occur on average once every 2. June 3 - New Moon. June 10 - Jupiter at Opposition. The giant planet will be at its closest approach to Earth and its face will be fully illuminated by the Sun. It will be brighter than any other time of the year and will be visible all night long. This is the best time to view and photograph Jupiter and its moons. A medium-sized telescope should be able to show you some of the details in Jupiter's cloud bands. A good pair of binoculars should allow you to see Jupiter's four largest moons, appearing as bright dots on either side of the planet.

June 17 - Full Moon. This full moon was known by early Native American tribes as the Full Strawberry Moon because it signaled the time of year to gather ripening fruit. It also coincides with the peak of the strawberry harvesting season. June 21 - June Solstice. The June solstice occurs at UTC. The North Pole of the earth will be tilted toward the Sun, which will have reached its northernmost position in the sky and will be directly over the Tropic of Cancer at This is the first day of summer summer solstice in the Northern Hemisphere and the first day of winter winter solstice in the Southern Hemisphere.

June 23 - Mercury at Greatest Eastern Elongation.

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July 2 - New Moon. July 2 - Total Solar Eclipse. A total solar eclipse occurs when the moon completely blocks the Sun, revealing the Sun's beautiful outer atmosphere known as the corona. The path of totality will only be visible in parts of the southern pacific Ocean, central Chile, and central Argentina.

A partial eclipse will be visible in most parts of the southern Pacific Ocean and western South America. July 9 - Saturn at Opposition. The ringed planet will be at its closest approach to Earth and its face will be fully illuminated by the Sun. This is the best time to view and photograph Saturn and its moons.

A medium-sized or larger telescope will allow you to see Saturn's rings and a few of its brightest moons. July 16 - Full Moon. This full moon was known by early Native American tribes as the Full Buck Moon because the male buck deer would begin to grow their new antlers at this time of year. July 16 - Partial Lunar Eclipse. A partial lunar eclipse occurs when the Moon passes through the Earth's partial shadow, or penumbra, and only a portion of it passes through the darkest shadow, or umbra.

During this type of eclipse a part of the Moon will darken as it moves through the Earth's shadow. July 28, 29 - Delta Aquarids Meteor Shower. The Delta Aquarids is an average shower that can produce up to 20 meteors per hour at its peak. The total eclipse is visible from within a narrow corridor that traverses the Pacific Ocean and southern South America. A partial eclipse is seen within the much broader path of the Moon's penumbral shadow, which includes the Pacific Ocean and most of South America Figure 3. Oeno Island is a remote coral atoll and is part of the Pitcairn Islands.

Unfortunately, there is no other landfall along the entirety of the Pacific track of kilometers. The region enjoys especially dry and clear weather - so much so that a string of major international astronomical observatories have been built there, including Cerro Tololo, La Silla and Gemini South. After crossing the Andes, the lunar shadow descends into Argentina for the last segment of its track. The shadow covers the kilometer-stretch across Argentina in only 3 minutes. In Argentina, San Juan lies just inside the southern limit while Cordoba is 75 kilometers north of the track.

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Just before the path ends, it barely misses Buenos Aires, the northern edge only 30 kilometers south of the center of the capital. Nevertheless, all roads leading from Buenos Aires to the central line will probably be clogged with traffic on eclipse day. At UT1 the lunar shadow lifts off Earth and returns to space. Central line coordinates and circumstances are presented in Table 3.

Partial phases of the eclipse are visible across the southern Pacific Ocean and South America. Local circumstances for a number of cities in South America are found in Table 4. The Sun's altitude and azimuth, the eclipse magnitude and obscuration are all given at the instant of maximum eclipse at each location. The Jul 02 Solar Eclipse Circumstances Calculator is an interactive web page that can quickly calculate the local circumstances for the eclipse from any geographic location not included in Table 4.

This is the 58th eclipse of Saros Espenak and Meeus, All eclipses in the series occur at the Moon's ascending node and gamma decreases with each member in the family. The series is a mature one that began with a modest partial eclipse on Oct After 20 partial eclipses in the series and more than 3 centuries, the first umbral eclipse occurred on May The event was a 2-minute total eclipse through New England, eastern Canada and Greenland.

During the next 2 centuries, the umbral duration continued to increase as each path shifted progressively southward.


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The greatest umbral duration of Saros occurred during the total eclipse of Aug Unfortunately, the 5 minute 40 second total eclipse was only visible from equatorial Africa, which was virtually inaccessible to astronomers of the day. As the duration of each succeeding eclipse decreased, the paths reversed their southern migration and drifted northward during the 18th and 19th centuries. This effect occurred as a result of the Northern Hemisphere season shifting from winter to summer when the Northern Hemisphere tipped towards the Sun.

The southbound trend of the Saros series resumed with the eclipse of May At this point, the duration of totality at greatest eclipse had again increased to over 5 minutes. The most recent member occurred on Jun 21 and its path crossed southern Africa on the summer solstice. After , the next member occurs on Jul 13 and passes through Australia and New Zealand. On Jul 24, the series returns to the African continent producing a path through South Africa. The duration of totality drops as Saros continues to produce total eclipses during the 21st century.

The last total eclipse of the series occurs on Aug 15 and lasts a maximum of 1 minute 38 seconds. The final 20 eclipses of the series are all partial events in the polar regions of the Southern Hemisphere. The family terminates with the partial eclipse of Feb Click for detailed diagram Partial Lunar Eclipse of July It takes place 4.

At the instant of greatest eclipse UT1 the Moon lies near the zenith from a location in South Africa. The event is well placed for observers in Europe, Africa, and South Asia. None of the eclipse will be visible from North America.


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  • South America will see later stages of the eclipse, which begins before the Moon rises. Table 5 lists predicted umbral immersion and emersion times for 25 well-defined lunar craters. The July 16 eclipse is the 21st eclipse of Saros This series began on Dec 09 and is composed of 79 lunar eclipses in the following sequence: 16 penumbral, 7 partial, 27 total, 8 partial, and 21 penumbral eclipses Espenak and Meeus, a.

    The first total eclipse is on Aug 17 and the final eclipse of the series is on Apr Click for detailed diagram Annular Solar Eclipse of December