NASA’s Solar Dynamics Observatory captured this image of Earth and the Moon transiting the Sun together on 13 September 2015. The edge of Earth, visible near the top of the frame, appears fuzzy because Earth’s atmosphere blocks different amounts of light at different altitudes. On the left, the Moon’s edge is perfectly crisp, because it has no atmosphere. This image was taken in extreme ultraviolet wavelengths of 171 angstroms. Though this light is invisible to our eyes, it is typically colourised in gold. Image credits: NASA/SDO.On 13 September 2015, as NASA’s Solar Dynamics Observatory, or SDO, kept up its constant watch on the Sun, its view was photobombed not once, but twice. Just as the Moon came into SDO’s field of view on a path to cross the Sun, Earth entered the picture, blocking SDO’s view completely. When SDO’s view of the Sun emerged from Earth’s shadow, the Moon was just completing its journey across the Sun’s face.This animation shows the relative movement of Earth and the Moon as they both crossed SDO’s field of view on 13 September 2015. Just as the Moon came into SDO’s field of view on a path to cross the Sun, Earth entered the picture, blocking SDO’s view completely. When SDO’s orbit finally emerged from behind Earth, the Moon was just completing its journey across the Sun’s face. Image credits: NASA/SDO.Though SDO sees dozens of Earth eclipses and several lunar transits each year, this is the first time ever that the two have coincided. This alignment of the Sun, Moon and Earth also resulted in a partial solar eclipse on 13 September, visible only from parts of Africa and Antarctica.
SDO’s orbit usually gives us unobstructed views of the Sun, but Earth’s revolution around the Sun means that SDO’s orbit passes behind Earth twice each year, for two to three weeks at a time. During these phases, Earth blocks SDO’s view of the Sun for anywhere from a few minutes to over an hour once each day.
You may notice that Earth’s outline looks fuzzy, while the Moon’s is crystal-clear. This is because — while the planet itself completely blocks the Sun’s light — Earth’s atmosphere is an incomplete barrier, blocking different amounts of light at different altitudes. On the other hand, the Moon has no atmosphere, so during the transit we can clearly see the crisp edges of the Moon’s horizon.
If clear skies persist, observers in the UK can view four naked-eye planets between now and the end of the month. Brightest planet Venus is visible low in the west some 45 minutes after sunset, while the waxing Moon is your celestial pointer to Jupiter, Saturn and Mars between 21 and 28 July at midnight.
The penultimate 2016 occultation of Neptune by the Moon occurs on 9 November for observers in Western Asia, Eastern Europe and northernmost Africa. In Western Europe, the nine-day-old waxing gibbous Moon merely brushes by the outermost planet, but the pair will be close enough to be seen within the same field of view of a typical binocular from the UK.
Jupiter is now less than a month from opposition (7 April), so it’s very much open season for the Solar System’s largest planet. If you’re unsure where to find it, the rising 17-day-old waning gibbous Moon passes just two degrees from Jupiter on the UK evening of 14 March. Virgo’s brightest star, first-magnitude Spica, makes it a great binocular triumvirate.
