Tag Archives: Full Moon

Super Moon vs. Micro Moon 

supermicromoon_paduraru_900
Image Credit & Copyright: Catalin Paduraru

What is so super about tomorrow’s supermoon? Tomorrow, a full moon will occur that appears slightly larger and brighter than usual. The reason is that the Moon’s fully illuminated phase occurs within a short time from perigee – when the Moon is its closest to the Earth in its elliptical orbit. Although the precise conditions that define a supermoon vary, given one definition, tomorrow’s will be the third supermoon of the year — and the third consecutive month that a supermoon occurs. One reason supermoons are popular is because they are so easy to see — just go outside and sunset and watch an impressive full moon rise! Since perigee actually occurs today, tonight’s sunset moonrise should also be impressive. Pictured above, a supermoon from 2012 is compared to a micromoon — when a full Moon occurs near the furthest part of the Moon’s orbit — so that it appears smaller and dimmer than usual. Given many definitions, at least one supermoon occurs each year, with the next being 2015 August 30.

APOD NASA 08-Sep-14

Surreal Moon 

Super Moon
Image Credit & Copyright: Jerry Lodriguss (Catching the Light)

 Big, bright, and beautiful, a Full Moon near perigee, the closest point in its elliptical orbit around our fair planet, rose on August 10. This remarkable picture records the scene with a dreamlike quality from the east coast of the United States. The picture is actually a composite of 10 digital frames made with exposures from 1/500th second to 1 second long, preserving contrast and detail over a much wider than normal range of brightness. At a perigee distance of a mere 356,896 kilometers, August’s Full Moon was the closest, and so the largest and most super, of the three Full Moons nearest perigee in 2014 now popularly known as supermoons. But if you missed August’s super supermoon, the next not-quite-so supermoon will be September 8. Then, near the full lunar phase the Moon’s perigee will be a slightly more distant 358,387 kilometers. That’s only about 0.4 percent less super (farther and smaller) than the super supermoon.
APOD NASA 14-Aug-14

Alicante Beach Moonrise 

OLYMPUS DIGITAL CAMERA

Image Credit & Copyright: José Carlos González

In this beach and skyscape from Alicante, Spain, July’s Full Moon shines in the dark blue twilight, its reflection coloring the Mediterranean waters. Near the horizon, the moonlight is reddened by its long path through the atmosphere, but this Full Moon was also near perigee, the closest point to Earth along the Moon’s elliptical orbit. That made it a Supermoon, a mighty 14% larger and 30% brighter than a Full Moon at apogee, the Moon’s farthest orbital swing. Of course, most warm summer nights are a good time to enjoy a family meal oceanside, but what fish do you catch on the night of a Supermoon? They must be Moon breams…

APOD NASA 19-Jul-14

Lisbon Honey Moon 

LisbonHoneyMoonClaro
Image Credit & Copyright: Miguel Claro

 The Sun set on Friday the 13th as a full Honey Moon rose, captured in this well-planned time-lapse sequence. Lisbon, Portugal’s Christ the King monument is in the foreground, about 6 kilometers distant from camera and telephoto lens. During the days surrounding today’s solstice (June 21, 10:51 UT) the Sun follows its highest arc through northern hemisphere skies as it travels along the ecliptic plane. At night the ecliptic plane is low, and the Full Moon’s path close to the ecliptic was also low, the rising Moon separating more slowly from the distant horizon. Northern moon watchers were likely to experience the mysterious Moon Illusion, the lunar orb appearing impossibly large while near the horizon. But the photo sequence shows the Moon’s apparent size did not not change at all. Its light was initially scattered by the long line-of-sight through the atmosphere though, and a deeper reddened color gave way to a paler gold as the Full Moon rose into the night.

NASA APOD 21-Jun-14

A Strawberry Moon 

GS_20140514_FullMoon_5015_p1500


Image Credit & Copyright: Göran Strand

 June’s Full Moon (full phase on June 13, 0411 UT) is traditionally known as the Strawberry Moon or Rose Moon. Of course those names might also describe the appearance of this Full Moon, rising last month over the small Swedish village of Marieby. The Moon looks large in the image because the scene was captured with a long focal length lens from a place about 8 kilometers from the foreground houses. But just by eye a Full Moon rising, even on Friday the 13th, will appear to loom impossibly large near the horizon. That effect has long been recognized as the Moon Illusion. Unlike the magnification provided by a telescope or telephoto lens, the cause of the Moon illusion is still poorly understood and not explained by atmospheric optical effects, such as scattering and refraction, that produce the Moon’s blushing color and ragged edge also seen in the photograph.

NASA APOD 13-Jun-14

Red Moon, Green Beam

D140414_47_ApolloEclipse_AFCc_16f Image Credit & Copyright: Dan Long (Apache Point Observatory) – Courtesy: Tom Murphy (UC San Diego)
This is not a scene from a sci-fi special effects movie. The green beam of light and red lunar disk are real enough, captured in the early morning hours of April 15. Of course, the reddened lunar disk is easy to explain as the image was taken during this week’s total lunar eclipse. Immersed in shadow, the eclipsed Moon reflects the dimmed reddened light of all the sunsets and sunrises filtering around the edges of planet Earth, seen in silhouette from a lunar perspective. But the green beam of light really is a laser. Shot from the 3.5-meter telescope at Apache Point Observatory in southern New Mexico, the beam’s path is revealed as Earth’s atmosphere scatters some of the intense laser light. The laser’s target is the Apollo 15 retroreflector, left on the Moon by the astronauts in 1971. By determining the light travel time delay of the returning laser pulse, the experimental team from UC San Diego is able to measure the Earth-Moon distance to millimeter precision and provide a test of General Relativity, Einstein’s theory of gravity. Conducting the lunar laser ranging experiment during a total eclipse uses the Earth like a cosmic light switch. With direct sunlight blocked, the reflector’s performance is improved over performance when illuminated by sunlight during a normal Full Moon, an effect fondly known as The Full Moon Curse. NASA APOD 18-Apr-14

Waterton Lake Eclispe

C523-3144-8199
Image Credit & Copyright: Yuichi Takasaka / TWAN / www.blue-moon.ca

Recorded on April 15th, this total lunar eclipse sequence looks south down icy Waterton Lake from the Waterton Lakes National Park in Alberta, Canada, planet Earth. The most distant horizon includes peaks in Glacier National Park, USA. An exposure every 10 minutes captured the Moon’s position and eclipse phase, as it arced, left to right, above the rugged skyline and Waterton town lights. In fact, the sequence effectively measures the roughly 80 minute duration of the total phase of the eclipse. Around 270 BC, the Greek astronomer Aristarchus also measured the duration of lunar eclipses – though probably without the benefit ofdigital clocks and cameras. Still, using geometry, he devised a simple and impressively accurate way to calculate the Moon’s distance, in terms of the radius of planet Earth, from the eclipse duration. This modern eclipse sequence also tracks the successive positions of Mars, above and right of the Moon, bright star Spica next to the reddened lunar disk, and Saturn to the left and below.

NASA APOD 17-Apr-14

Spica, Mars, and Eclipsed Moon

eclipse_apr15th_dp
Image Credit & Copyright: Damian Peach

A beautiful, reddened Moon slid through dark skies on April 15, completely immersed in Earth’s shadow for well over an hour. It was the year’s first total lunar eclipse and was widely enjoyed over the planet’s Western Hemisphere. Seen from the Caribbean island of Barbados, the dimmed lunar disk is captured during totality in this colorful skyview. The dark Moon’s red color contrasts nicely with bright bluish star Spica, alpha star of the constellation Virgo, posing only about two degrees away. Brighter than Spica and about 10 degrees from the Moon on the right, Mars is near opposition and closest approach to Earth. The Red Planet’s own ruddy hue seems to echo the color of the eclipsed Moon.
NASA APOD 16-Apr-14

Micro Moon over Super Moon

microsupermoon_sciarpetti_960
Image Credit: Stefano Sciarpetti
Explanation: Did you see the big, bright, beautiful Full Moon last Wednesday night? That was actually a Micro Moon! On that night, the smallest Full Moon of 2014 reached its full phase only a few hours from lunarapogee, the time of its the most distant point from Earth in the Moon’s elliptical orbit. Of course, last year on the night of June 22, a Full Super Moon was near perigee, the closest point in its orbit. The relative apparent sizeof January 15’s Micro Moon is compared to the June 22 Super Moon in the above composite image digitally superimposing telescopic images from Perugia, Italy. The difference in apparent size represents a difference in distance of just under 50,000 kilometers between apogee and perigee, given the Moon’s average distance of about 385,000 kilometers. How long do you have to wait to see another Full Micro Moon? Until March 5, 2015, when the lunar full phase will again occur within a few hours of lunar apogee.

NASA APOD 21-Jan-2014