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Current Positions of the Planets in the Night Sky:









Star map of Eclipse at Totality

Simulated View of Sky at Eclipse Totality

Direction & Altitude of Sun & Planets at Totality from 30 USA locations

 The American Eclipse,

August 21st 2017:

Positions of the Planets at Totality


by Martin J Powell

On August 21st 2017 millions of observers will look skywards to witness the first total solar eclipse over the USA mainland since 1979. The 'Great American Eclipse', visible from twelve states across the country from North-west to South-east, is likely to become the most photographed, filmed and talked-about solar eclipse in history. This article does not examine the eclipse itself, however, but the naked-eye planets which one can expect to glimpse in the vicinity of the eclipsed Sun (and a little further afield) within the 2 minutes or so of totality. A total solar eclipse is the only circumstance in which planets positioned on either side of the Sun (morning and evening planets) can be observed from Earth at the same time.

A fully eclipsed Sun with Venus and Mercury above it, observed from the Java Sea, Indonesia on March 9th 2016 (Photograph  Joseph A Carr)

A fully eclipsed Sun with Venus and Mercury above it, observed from the Java Sea, Indonesia on March 9th 2016 (Photograph Joseph A Carr)

What Planets are Visible During the Eclipse?

There are potentially four naked-eye planets which are viewable during totality, two with ease and two with some difficulty. The two brightest will be visible long before totality arrives:

Venus, at an apparent magnitude of -4.0 is easily seen against the twilit sky caused by the eclipse totality. In fact, it should become visible some 15 minutes or more before totality, when the eclipse is still partial and the sky is slowly darkening. Venus is positioned 34 West of the Sun at the time of the eclipse. It is now about half-way through its 2017 morning apparition, having been visible as a 'Morning Star' before dawn for several months. The planet is positioned in the Western half of the constellation of Gemini, the Twins. Its two brightest stars Castor (Greek lower-case letter 'alpha' Gem or Alpha Geminorum, mag. +1.6) and Pollux (Greek lower-case letter 'beta' Gem or Beta Geminorum, mag. +1.1) are positioned a short distance above (North of) the planet, both of which should be visible in the twilight of eclipse totality.

Jupiter (magnitude -1.6) is positioned 52 to the East of the Sun at eclipse totality. It should also become visible during the partial phase of the eclipse. For observers along the track of totality who are located West of central Idaho, Jupiter cannot be seen because the eclipse takes place before the planet has risen (see table below). Jupiter is positioned in central Virgo, the Virgin, near its brightest star Spica (Greek lower-case letter 'alpha' Vir or Alpha Virginis, mag. +1.0) which should also be glimpsed in the twilight of totality. Jupiter is now an evening planet, visible after sunset, around 90% through its 2016-17 apparition.

Mars (mag. +1.8) is positioned just 8 to the West of the Sun. Mars is very distant from the Earth at this time and consequently it is more difficult than normal to spot in the twilight. Being considerably fainter than both Venus and Jupiter, it is only likely to become visible in the final seconds leading up to totality. The Red Planet, which appears pale orange to the naked-eye whenever it is bright, is positioned in Eastern Leo and will soon emerge out of the dawn twilight into the start of its 2017-19 apparition (in July 2018 Mars will reach its closest point to the Earth in almost fifteen years).

Mercury (mag. +3.4) is positioned 11 to the South-east of the Sun at the time of the eclipse. It is the faintest of the four planets visible during the eclipse and will be the most difficult to detect. Mercury is now at the end of its second evening apparition of 2017 and is the closest of the planets to Earth at this time.

At the time of the eclipse, the Sun is positioned in the Western half of the constellation of Leo, the Lion, not far from its brightest star, Regulus (Greek lower-case letter 'alpha' Leo or Alpha Leonis, mag. +1.4). Regulus itself may be easy or difficult to discern, depending upon the brightness of the eclipsed sky and any glare effect caused by the Sun's corona. The brightness of an eclipsed sky is dependant on several factors and is difficult to determine in advance, so the magnitude of the faintest stars to be seen at totality is uncertain. Historically, eclipse observers have often seen stars with the naked-eye down to about magnitude +3.5, although photographic equipment will often detect stars of much fainter magnitude.

Star map showing the positions of Venus, Mercury, Mars and Jupiter at eclipse totality on August 21st 2017 (Copyright Martin J Powell 2017)

Star map showing the positions of Venus, Mercury, Mars and Jupiter at eclipse totality on August 21st 2017. A simulation of this region of the sky at totality is shown below. The ecliptic  (pale yellow line) is the apparent path of the Sun through the zodiac constellations as seen from the orbiting Earth during the year - the Moon and planets follow it very closely. The numbers along the sides of the map (Right Ascension and Declination) are co-ordinates of celestial longitude and latitude which are used to locate the positions of celestial bodies in the night sky. A printer-friendly (greyscale) version of the star map is available here.

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A simulation of the sky at the moment of eclipse totality on August 21st 2017, showing the planets and brighter stars which are likely to be seen (Copyright Martin J Powell 2017)

A simulation of the sky at the moment of eclipse totality on August 21st 2017, showing the planets and brighter stars which are likely to be seen in the twilight. Stars are shown down to magnitude +3.5, although their actual visibility is difficult to determine in advance of the event. Roll your pointer over the image (or click on the image) to identify the various points of light (only stars brighter than magnitude +2 are labelled). The scale and orientation of the picture matches that of the star map above. Because of the wide area of sky shown, the stars and planets necessarily appear small, their brightness refecting the likely difficulty in viewing them. Jupiter, at the lower left of the image, will not be seen from locations within the track of totality in Oregon and Western Idaho (see table below).

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Direction & Altitude of the Sun and Planets during the Eclipse

The positions of stars and planets in relation to the Sun at total eclipse depends upon where along the track of totality the observer is located. The table below shows the direction and altitude (angle above the horizon) of the eclipsed Sun and the four naked-eye planets for thirty locations across the USA. Direction is given using conventional compass points; altitude is measured as 0 at the level horizon and 90 directly above the observer's head (a point known in astronomy as the zenith). Hence an altitude of 45 is positioned 'halfway up the sky' (see diagram below right).

Diagram showing how a celestial body is located in the night sky using direction and altitude (Copyright Martin J Powell, 2008)

Using direction and altitude to find a star or planet in the night sky. In this case, the star/planet is in the South-east (SE) at an altitude of 20.


The eclipsed Sun is seen at higher altitudes above the horizon in the Eastern half of the USA than the Western half, the highest altitude being in South-western Kentucky at a little over 64. East of Tennessee the Sun's altitude at totality reduces, but only by a few degrees. In Oregon the eclipse takes place at mid-morning, positioning the Sun in the ESE at around 40 above the horizon. At Columbia, Missouri - approximately halfway along the track of totality - the Sun is on the meridian (due South) at eclipse totality, at 63 high. In South Carolina the eclipse takes place around mid-afternoon, placing the Sun in the South-west at a little over 60 above the horizon.


In Eastern Nebraska, the Sun and Venus appear at almost the same altitude at totality, Venus being 34 directly to the right of the Sun. West of Eastern Nebraska, Venus appears higher than the Sun in the sky (i.e. to the upper right of it); East of Eastern Nebraska, it appears lower than the Sun (to the lower right of it).

From all locations which are able to see it, Jupiter appears lower in the sky than the Sun, i.e. to the lower left in all cases. It is positioned in the opposite direction from the Sun to that of Venus. At a solar elongation of 52, Jupiter appears about 1 times further away from the Sun than Venus.

From Western Kentucky through to central Tennessee, Mars appears at the same altitude as the Sun at totality. West of Western Kentucky, Mars appears to the upper right of the Sun; East of central Tennessee the Red Planet appears to the right of the Sun, but only slightly lower down.

Difficult-to-see Mercury is to the lower left of the Sun from all states except Oregon, where the planet is positioned almost directly below it. From South Carolina Mercury appears to the left of the Sun but only slightly lower than it.

The table below shows that, in a few states, pairs of planets have the same altitude in the sky at totality (i.e. they appear level with each other, in relation to the horizon). In central Nebraska, Venus and Mars appear almost level with each other, differing in altitude by 1 and being 26 apart horizontally. In central Missouri, Venus and Mercury appear level, having the same altitude and being 43 apart. In central South Carolina, Venus and Jupiter appear level, being 85 apart (almost one-quarter of the angular distance around the horizon). Finally, in central and Eastern South Carolina Mars and Mercury appear almost level (within 1 in altitude of each other), being separated horizontally by an angular distance of 18.

Table showing direction & altitude of the eclipsed Sun and four planets at totality for 30 US locations on August 21st 2017 (Copyright Martin J Powell 2017)

Table showing the direction & altitude of the eclipsed Sun and four naked-eye planets at thirty locations within the USA sited along the eclipse path on August 21st 2017. A hyphen (-) indicates that the planet is below the horizon at the time of the eclipse.

The location of the longest period of eclipse (2 mins, 41.6 secs) is in Southern Illinois at geographical coordinates North 37 34' 4", West 89 6' 10".

Although the excitement and the short duration of a total solar eclipse mean that most observers will spend little or no time searching for planets, the spectacle of witnessing the Sun and its family of planets in Earth's daytime sky is a rare and special experience. The next opportunity to witness a total solar eclipse over the USA mainland will be on April 8th 2024, when all five naked-eye planets will be visible at totality! The path of totality on this occasion will cross through central Mexico, Texas, Oklahoma, Arkansas, Missouri, Illinois, Indiana, Ohio and Eastern Canada.

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Copyright  Martin J Powell  March 2017

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