A Lord of Rings: Saturn at Opposition 2016

Saturn 2016
Saturn in early May 2016. Image credit: Efrain Morales.

They’re back. After a wintertime largely devoid of evening worlds, the planets are once again in the evening sky. First Jupiter, then Mars have crossed opposition over the past few months, and now Saturn is set to take center stage later next week, reaching opposition at 7:00 Universal Time (UT) on the night of June 2/3rd. This places the ringed world in a position of favorable evening viewing, rising in the east as the Sun sets in the west, and riding highest near local midnight across the meridian.

Opposition 2016 sees the planet Saturn looping through the southern realm of the constellation Ophiuchus, making a retrograde run this summer at the Scorpius border before looping back and resuming eastward motion. That’s right: Saturn currently occupies the dreaded ‘13th house,’ of Ophiuchus, for all you Snake-Bearers out there. Saturn is currently at bright as it can be, at magnitude +0.04.

Saturn rising on the night of June 2nd. Image credit: Starry Night Education Software.
Saturn rising on the night of June 2nd. Image credit: Starry Night Education Software.

Saturn reaches opposition once every 378 days, as it orbits the Sun at a leisurely pace every 29.5 years. 2016 and the next few oppositions sees Saturn ‘bottoming out,’ sitting around -20 degrees south. Saturn won’t peek northward across the celestial equator again until March 2026. This places the 2016 appearance of Saturn high in the sky south of the equator, transiting about 30 degrees above the southern horizon around midnight for folks observing around 40 degrees north latitude. Saturn also begins looping towards the star-rich region of the galactic equator for a crossing it late next year in December 2017. Saturn sits 9 Astronomical Units (AU) or 1.4 billion kilometers distant on June 3rd, a slightly larger distance than usual, owing to the fact that the planet is headed towards aphelion on April 17th, 2018.

The waxing gibbous Moon passes 3.2 degrees north from Saturn on Sunday, June 19th, just a day before reaching Full.

Watch for a sudden brightening of the planet in early June, known as an ‘opposition surge’ due to what is known as the Seeliger effect. This is a coherent back-scattering of light, focusing it similar to highway retro-reflectors shining your headlights back at you at night. In this case, the Sun is the ‘headlight,’ and the millions of snowball moonlets hiding their shadows from view reaching 100% illumination are the highway retro-reflectors. The effect is subtle, to be sure, but serves to raise the brightness of the planet by about half a magnitude. This should be apparent in an animation sequence shot before, during and after over the span of a about a week. Any takers?

Almost there... the widening tilt of Saturn's rings. image credit and copyright: Andrew Symes (@failedprotostar).
Almost there… the widening tilt of Saturn’s rings. image credit and copyright: Andrew Symes (@failedprotostar).

And speaking of the rings, here’s another reason to check out Saturn this opposition 2016 season. The tilt of rings is about 26 degrees wide as seen from our Earthly perspective… about as wide as they can be. Saturn’s rings were last edge on in 2009, and reach a maximum width of 27 degrees on October 16th, 2017 before slowly heading towards edge on again in 2025.

The path of Saturn through the last half of 2016. Image credit: Starry Night Education software.
The path of Saturn through the last half of 2016. Image credit: Starry Night Education software.

At the eyepiece, Saturn shows a yellowish disk 18” extended to 43” across if you count the rings. Crank up the magnification to over 100x under good seeing, and the black thread of the Cassini division jumps into view. Saturn has 62 moons in all, with +9th magnitude Titan being the brightest. You’re looking at the most distant surface outpost of humanity, the site of the 2005 landing of the European Space Agency’s Huygens lander. Six moons are readily visible in a small telescope, while the fainter moons Hyperion and Phoebe present a challenge to owners of extreme light buckets. Also, as Saturn heads past opposition and towards eastern quadrature 90 degrees from the Sun on September 2nd, 2016, watch for the shadow of the bulk of the planet, cast back across the rings.

A sampling of the Moons of Saturn. Image credit: Stellarium.
A sampling of the Moons of Saturn. Image credit: Stellarium.

We never miss a chance to observe Saturn if it’s above the horizon. Saturn is a sure-fire crowd-pleaser for any sidewalk astronomy session, and no one forgets their first glimpse of the glorious ringed world. You can just imagine how much consternation this bizarre-looking planet must have caused Galileo. You can tell just how primitive his first telescope was, as his sketches show off Saturn as more of a two-handled ‘coffee cup’ in appearance. Christaan Huygens first deduced something of the true nature of Saturn’s rings in 1655, correctly claiming that they are physically separated from the disk.

Don’t miss Saturn at opposition next week!

A May Full ‘Blue Moon’ on Tap For This Weekend?

Blue Moon
A filtered 'Blue Moon' from July 31st, 2015. Image credit and copyright: John Chumack

Brace yourselves. You are about to hear talk this week of an astronomical non-occurrence of the utmost in obscurity. We’re talking about this weekend’s Blue Moon.

Now, I know what you’re thinking. Isn’t a ‘Blue Moon’ the second Full Moon of the month? How can a Blue Moon fall on the 21st? Trust me, we’re both correct… in a sense. The term ‘Blue Moon’ has taken on several meanings over the last few decades, with the ‘the second Full Moon in a calendar month containing two Full Moons’ now in vogue across ye old Internet. It seems the masses just can’t get enough of Super, Blood, Honey and Moons Black and Blue. We point to last month’s rumored ‘Green Moon‘ as evidence. (Spoiler alert: it wasn’t).

No, we’re talking instead of a Blue Moon in an old-timey sense. You’ll be hard pressed to explain source of this week’s Blue Moon for sure, though it has a fascinating origin story.

A Full Moon rising with Saturn and Mars on the night of May 21st, 2016. Image credit: Starry Night Education software.
A Full Moon rising with Saturn and Mars on the night of May 21st, 2016. Image credit: Starry Night Education software.

The term seems to come down to us from the Maine Farmer’s Almanac, which denoted the ‘third Full Moon in an astronomical season with four as blue.’ The lunar synodic period of 29.5 days — the length of time it takes the Moon to return to a like phase, such as New to New, or Full to Full — means that on most years, there are 12 Full Moons. 29.5 times 12 comes out about 11 days short of a 365.25 day solar year at 354 days, meaning that about every three years, we have a year with 13 Full Moons.

Not a big deal, you say? Well, it assures that lunar based forms of reckoning time, such as the Muslim calendar loses 11 days relative to the Gregorian calendar every year.

Here’s how the 2016 Blue Moon breaks down:

March Equinox- March 20th 4:30 Universal Time (UT)

March Full Moon- March 23rd 12:02 UT

April Full Moon- April 22nd 5:22 UT

May Full Moon- May 21st 21:17 UT (3rd in an astronomical season, ‘blue’)

June Full Moon- June 20th 11:05 UT

June Solstice- June 20th 22:34 UT

The last time we had a season with four Full Moons was August 21st, 2013, and the next Blue Moon under this rule is May 18th, 2019.

Adding a pinch of blue to the Full Moon with a military flashlight filter. Image credit: Dave Dickinson
Adding a pinch of blue to the Full Moon with a military flashlight filter. Image credit: Dave Dickinson

Of course, a deeper riddle is just why the Maine Farmer’s Almanac termed this occurrence as Blue, and why they picked the 3rd of a season with 4 specifically… one legend goes that the extra anomalous Full Moon was depicted on the calendar in blue ink to stand out. We’d love to get our hands on a copy of the Old Maine Farmer’s Almanac circa late 19th early 20th century era to see if this was indeed the case. This is on our list of research projects, next time we find ourselves back in our home state of Maine.

Types of Blue Moons

We’ve chronicled the tales of Moons, both Black and Blue. Sky and Telescope also explored the role they had in introducing the modern day Blue Moon into common vernacular. We’ll admit, the ‘2nd in a month with two Full Moons’ is a much easier rule to explain!

Of course, the Moon isn’t scheduled to actually appear blue this week… that’s actually a much rarer occurrence, and the Moon doesn’t need to even be Full for this to happen. In September 23rd, 1950, the residents of the northeastern United States saw the 94% illuminated waxing gibbous Moon rise with a distinctly bluish cast, owing to the high concentration of oily soot particles suspended high in the atmosphere, scattering out red and yellow light but filtering through blue. Reports of similar Blue Moons dot observational lore, though to our knowledge, no one has actually captured an image of such a cerulean apparition of the Moon.

The rising Full Moon of September 23rd, 1950. Image credit: Stellarium
The rising Full Moon of September 23rd, 1950. Image credit: Stellarium

Is the Moon ever really Full? You can make a pretty good argument that the Moon as seen from the Earth is never truly fully illuminated, though it gets really close. Full 100% illumination would occur when the Moon is exactly opposite to the Sun, but when this occurs, the Moon also passes into the dark shadow of the Earth, during a total lunar eclipse.

Fun fact: the next ‘Blue Blood Moon’ lunar eclipse occurs on January 31st, 2018, following the ‘2nd Full Moon in a month with 2′ rule.

I see some blue in there... the Full Moon, enhanced to bring out subtle color. Image credit and copyright: Rolf Wahl Olsen
I see some blue in there… the Full Moon, enhanced to bring out subtle color. Image credit and copyright: Rolf Wahl Olsen

The May Full Moon also has the romantic name of the Full Flower, Corn Planting or Milk Moon in Algonquin Indian lore.

In 2016, the Moon continues to follow a shallow path relative to the ecliptic plane, which in turn traces out the Earth’s path around the Sun. 2015 was the bottoming out of the ‘shallow year’ known as a minor lunar standstill, and we’re now headed towards a hilly or steep year of a major lunar standstill in 2025, a time once every 19 years when the Moon rides high in the sky, adding its 5 degree inclination relative to the ecliptic plane.

Too bad Mars doesn't have a large moon... because it would indeed appear blue, as do Martian sunsets. Image credit: JPL/NASA
Too bad Mars doesn’t have a large moon… because it would indeed appear blue, as do Martian sunsets. Image credit: JPL/NASA

Will this weekend’s olden times Blue Moon gain traction in today’s fast-paced social media news cycle? Stay tuned!

Watch Mercury Race Across the Sun, Courtesy of the Big Bear Solar Observatory

Mercury transit
The Big Bear Solar Observatory Captures a high-res image of this week's transit of Mercury across the face of the Sun. Image credit: NJIT/BBSO

Just. Wow.

Just when we thought we’d seen every amazing image and video sequence from Monday’s transit of Mercury, a new one surfaces that makes our jaw hit the floor.

The folks at the Big Bear Solar Observatory may have just won the internet this week with this amazing high-definition view of Mercury racing across the surface of the Sun:

Remember, Mercury is tiny a world, just 1.4 times the diameter of our Moon, at 4,880 kilometers across. At about 9″ arc seconds across during the transit, it took Mercury seven and a half hours to race across the 30′ (over 180 times the apparent size of Mercury as seen from the Earth) disk of the Sun.

The video has an ethereal three dimensional quality to it, as we seem to race along with the fleeting world. You can see the granulation in the dazzling solar photosphere whiz by in the background.

Big Bear Solar Observatory Telescope Engineer and Chief Observer Claude Plymate explains some of the technical aspects of the captured sequence:

“John Varsik assembled (the video) from our speckle reconstructed broadband filter images. The images were taken with a high speed PCO2000 CCD camera. Bursts of 100 frames were taken at a cadence of 15 seconds. After flat fielding and dark subtraction, speckle reconstruction is used on each burst to generate the final single frame. Exposure time was 1.0 ms through a broadband TiO (7057A, 10A FWHM) filter. 
Our actual primary science data was data taken with a fast scanning spectrometer that very quickly produces 2D Na D-line maps. The objective was to measure the Na distribution in Mercury’s exosphere in absorption.”
So there’s some science there as well, as measurements taken from Big Bear will make a fine comparison and contrast with NASA’s measurements of the tenuous exosphere of Mercury measured by the MESSENGER spacecraft.
Based on the shores of Big Bear Lake in the San Bernardino Mountains 120 kilometers east of downtown Los Angeles, the Big Bear Solar Observatory employed the 1.6-meter New Solar Telescope (NST) to follow the transit. The NST is the largest clear aperture solar telescope in the world currently in use. Capable of resolving features on the Sun just 50 kilometers across, the mirror blank for the NST was figured at the Mirror Lab at the University of Arizona in Tucson and served as a proof of concept for the seven mirror Giant Magellan Telescope currently under construction.
The Big Bear Solar Observatory. Image Credit: The NJIT/BBSO
The Big Bear Solar Observatory. Image Credit: The NJIT/BBSO
The Big Bear Solar Observatory is managed under the New Jersey Institute of Technology and is funded by NASA, the United States Air Force and the National Science Foundation.
The Big Bear Solar Observatory is also part of the GONG (Global Oscillation Network Group), a series of observatories worldwide dedicated to observing the Sun around the clock. It’s strange to think, but in a sense, we live inside the outer atmosphere of our host star, and knowing just what it’s doing is of paramount importance to our modern technology-dependent civilization.
An awesome capture, with some amazing science to boot. Big Bear will also get a sunrise view of the November 11th, 2019 transit of Mercury as well:
Because it's never too early to start planning... here's the visibility prospects for the 2019 transit of Mercury. Image credit: Xavier Juber.
Because it’s never too early to start planning… here’s the visibility prospects for the 2019 transit of Mercury. Image credit: Xavier Juber.
Stay tuned!
Also check out Universe Today’s Flickr forum for more amazing images of the transit of Mercury, and Nancy Atkinson’s roundup of the view from the Solar Dynamics Observatory.

Video used with permission of the BBSO.

The BBSO operation is supported by NJIT, US NSF AGS-1250818, and NASA
NNX13AG14G grants, and the NST operation is partly supported by the Korea
Astronomy and Space Science Institute and Seoul National University and by
the strategic priority research program of CAS with Grant No.
XDB09000000″.

Images of Today’s Transit of Mercury From Around the World

Mercury Transit
Mercury meets the Sun in Hydrogen Alpha. Image credit and copyright: Brendan Martin @HASungazer

Lead image credit: Brendan Martin.

(Note: Awesome images are being added as they come in!)

Update: Here’s two more amazing videos of yesterday’s transit of Mercury that have come our way. First: double solar transits featuring Mercury, the International Space Station and a low flying plane right here in the skies of good old planet Earth courtesy of (who else?) Thierry Legault:

And here’s one of the very few sequences we’ve seen of the transit with foreground, captured at sunset by Gadi Eidelheit based in Israel:

And finally, check out this amazing (and mesmerizing) animation of Mercury racing across the Sun, courtesy of the Big Bear Solar Observatory!

It’s not every day you get to see a planet pass in front of the Sun.

But today, skywatchers worldwide got to see just that, as diminutive Mercury passed in front of the disk of the Sun as seen from the Earth. This was the first transit of Mercury across the face of the Sun since November 8th, 2006, and the last one until November 11th, 2019. Continue reading “Images of Today’s Transit of Mercury From Around the World”

A Summer Comet: Our Guide to Observing X1 PanSTARRS

Comet X1 PanSTARRS
Comet C/2013 X1 PanSTARRS from early January 2016, shortly after a reported outburst. Image credit and copyright: Hisayoshi Kato.

Ready for one of the better binocular comets of 2016? Emerging from behind the Sun and a surprise outburst in January, Comet C/2013 X1 PanSTARRS is about to put on its summer show. The waning crescent Moon just crossed paths with the comet in the dawn sky on its way to New on May 6th, and the time to start tracking it is now as it plunges southward across the ecliptic this weekend. Continue reading “A Summer Comet: Our Guide to Observing X1 PanSTARRS”

An Old Glass Plate Hints at a Potential New Exoplanet Discovery

Polluted white dwarf
An artist's conception of a 'polluted white dwarf' star, plus debris disk. Image credit: NASA.

What’s the value to exoplanet science of sifting through old astronomical observations? Quite a lot, as a recent discovery out of the Carnegie Institution for Science demonstrates. A glass plate spectrum of a nearby solitary white dwarf known as Van Maanen’s Star shows evidence of rocky debris ringing the system, giving rise to a state only recently recognized as a ‘polluted white dwarf.’ Continue reading “An Old Glass Plate Hints at a Potential New Exoplanet Discovery”

Into the Red: Our Complete Guide to Mars Opposition 2016

Mars 2014
Mars from opposition 2014. Image credit and copyright: Paul Stewart.

Ready to explore the Red Planet? Starting in May, Mars invades the evening skies of the Earth, as it heads towards opposition on May 22nd. Not only does this place Mars front and center for prime time viewing, but we’re headed towards a cycle of favorable oppositions, with Mars near perihelion, while Earth is near aphelion. Continue reading “Into the Red: Our Complete Guide to Mars Opposition 2016”

April Lunacy: Getting Ready for the Full ‘Mini-Moon’

2015 Mini-Moon
The March 5th 2015 Mini-Moon. Image credit and copyright: Alan Dyer

Do you welcome the extra evening light of the Full Moon, or curse the additional light pollution? Either way, this week’s Full Moon on Friday April 22nd is special. It’s the smallest Full Moon of 2016, something we here at Universe Today have christened the Mini-Moon.

Mini-Moon 2016: This year’s Mini-Moon falls on April 22nd at 5:25 Universal Time (UT), just 13 hours and 19 minutes after lunar apogee the evening prior at 16:06 UT on April 21st. Though apogee on the 21st is 406,350 km distant – a bit on the far end, but the third most distant for the year by 300 km — this week’s Full Moon is the closest to apogee for 2016 time-wise. The 2015 Mini-Moon was even closer, in the 10 hour range, but you’ll have to wait until December 10th, 2030 to find a closer occurance.

Image credit and copyright:
The Mini-Moon versus the 2011 Supermoon. Image credit and copyright: Ken Lord.

What is the Mini-Moon, you might ask? As with the often poorly defined Supermoon, we like to eschew the ambiguous ‘90% of its orbit’ definition, and simply refer to it as a Full Moon occurring within 24 hours of lunar apogee, or its farthest point from the Earth in its orbit.

Fun fact: the 29.55 day period from perigee to perigee (or lunar apogee-to-apogee) is known as an anomalistic month.

Image credit: Dave Dickinson
Mini-Moons by year for the remainder of the decade. Note that the 2020 Full Moon is also the 2nd of the month… A ‘Mini-Blue Halloween Moon?’ Image credit: Dave Dickinson

Thank our Moon’s wacky orbit for all this lunacy. Inclined 5.14 degrees relative to the ecliptic plane, the Moon returns to the same phase (say, Full back to Full) every 29.53 days, known as a synodic month. The Moon can appear 33.5′ across during perigee, and shrink to 29.4′ across near apogee.

The appearance of the Moon through one synodic period. Note that in addition to rocking back and forth (libration) and side-to-side (nutation), the Moon appears to swell and shrink in size. Wikimedia Commons graphic in the public Domain.
The appearance of the Moon through one synodic period. Note that in addition to rocking back and forth (libration) and side-to-side (nutation), the Moon appears to swell and shrink in size. Wikimedia Commons graphic in the Public Domain.

And don’t fear the ‘Green Moon,’ and rumors going ’round ye’ ole internet that promise a jaded Moon will occur in April or May; this is 100% non-reality based, seeking to join the legends of Super, Blood, and Full Moons, Black and Blue.

Image faked by: David Dickinson.
No. Just. No. Image faked by: David Dickinson.

The April Full Moon is also known as the Full Pink Moon to the Algonquin Indians. The April Full Moon, can, on occasion be the Full Moon ushering in Easter (known as the Paschal Moon) as per the rule established by the 325 AD council of Nicaea, stating Easter falls on the first Sunday after the first Full Moon after the fixed date of the Vernal Equinox of March 21st. Easter can therefore fall as late as April 25th, as next occurs on 2038. The future calculation of Easter by the Church gets the Latin supervillain-sounding name of Computus.

April 21st. Image credit: Stellarium
Looking east on the evening of April 21st. Image credit: Stellarium

Of course, the astronomical vernal equinox doesn’t always fall on March 21st, and to complicate matters even further, the Eastern Orthodox Church uses the older Julian Calendar and therefore, Easter doesn’t always align with the modern western Gregorian calendar used by the Roman Catholic Church.

The Moon can create further complications in modern timekeeping as well.

Here’s one wonderful example we recently learned of in our current travels. The Islamic calendar is exclusively based on the synodic cycle of the Moon, and loses 11 days a year in relation to the Gregorian solar calendar. Now, Morocco officially adopted Daylight Saving (or Summer) Time in 2007, opting to make the spring forward during the last weekend of March, as does the European Union to the north. However, the country reverts back to standard time during the month of Ramadan… otherwise, the break in the daily fast during summer months would fall towards local midnight.

You can see a curious future situation developing. In 2016, Ramadan runs from sundown June 5th, to July 4th. Each cycle begins with the sighting of the thin waxing crescent Moon. However, as Ramadan falls earlier, you’ll get a bizarre scenario such as 2022, when Morocco springs forward on March 27th, only to fall back to standard time six days later on April 2nd on the start of Ramadan, only to jump forward again one lunation later on April 30th!

Morocco is the only country we’ve come across in our travels that follows such a convoluted convention of timekeeping.

Fun fact #2: the next ‘Mini-Moon’ featuring a lunar eclipse occurs on July 27th 2018.

And the Spring Mini-Moon sets us up for Supermoon season six months later this coming October-November-December. Though lunar perigees less than 24 hours from Full usually occur as a trio, an apogee less than 24 hours from Full is nearly always a solitary affair, owing to the slightly slower motion of the Moon at a farther distance.

Don’t miss the shrunken Mini-Moon rising on the evenings of Thursday April 21st and Friday 22nd, coming to a sky near you.

Prelude to Transit: Catching Mercury Under Dusk Skies

Mercury and the Moon
The waxing gibbous Moon passes Mercury (low to the right). Image credit and copyright: Tavi Greiner

Have you ever seen Mercury? The diminutive innermost world takes the center stage next month, as it transits the Sun as seen from our early perspective on May 9th. This week, we’d like to turn your attention to bashful Mercury’s dusk apparition, which sets up the clockwork celestial gears for this event. Continue reading “Prelude to Transit: Catching Mercury Under Dusk Skies”