Scopes, scopes, scopes: if you are looking for a telescope, well, we have several looking for good homes. Ring Mark for details.
Welcome to the WDAS monthly newsletter for July 2018: a digest of the month's latest contributions to our website. Below you'll find Society News, Sky Notes, the latest in Mark's monthly Crossing the Line series, as well as coming events.
Society News
The society has again been invited to the NYM Park Fest day on Sunday 22nd July, to be held at the Danby Moors centre.
We attended the event in 2016, and although Mark and Keith put on a good display the weather didn’t, and only fleeting glimpses of the Sun were possible for solar viewing. We have been tasked again with solar viewing and if conditions are fine a scaled solar system demo. The event runs from 10:00-17:00h. Two free car spaces have been allocated to us and the attending charge has been waved.
Mark and Keith will be in one car – so any member wishing to help out and has a car can have a free day!
As this edition of the WDAS Newsletter goes to press (digitally speaking) Mark's on holiday, enjoying the sunshine on some windy mountain, I expect. And he's sent me a photo of a star party from last Saturday (23-Jun-2018) with no little by way of accompanying article. "Views of the moon, Jupiter, Venus and finally Saturn", it said. "Kept all busy, but Mercury could not be picked out of some streaky haze low in the west". So lucky you... you get to read a short and geeky padded article from me.
Mark took a break from writing this month's Planetary Skylights last Saturday evening to run a Star Party on West Cliff. He was excited to try out Keith's new scope: a treat he'd been anticipating for much of the month. (Various missives reached me in Tenerife carrying news of fog, fog and more fog in Whitby in the early month... in the end even with idle speculation about whether Keith's telescope may be cursed!).
But here you have it.. a small image of Keith's new, black, 12" Skywatcher Dobsonian 'Truss' telescope with Go-to facilities, which they've helpfully photographed against a black background!
And, shining bright through the gloom you see it here in action in the star party, although - wouldn't you know it - everyone was globularly clustered around a far smaller scope at that moment.
Sky Notes
In this month's Sky Notes:
Planetary Skylights
July is going to be a busy month, with all the naked eye planets visible and a total lunar eclipse to enjoy as well, weather providing!
Let us start with the planets visible low in the west. Mercury will still be on show for the first couple of weeks, retreating back toward the WNW horizon by mid month. Admittedly it will be a little tricky to spot, but look for it approximately 40 minutes after sunset (around 22:10h) lower right of Venus. A flat, unobstructed view is a must as it will be low down. Use binoculars to help pick out this elusive world, before trying with just the naked eye. On July 14th a crescent Moon resides lower left of Mercury, but this will be a challenge with skies still bright.
Brilliant Venus cannot be missed, dominating the western sky. The ‘evening star’ will start to arc down toward the horizon over the course of the month. Telescopically (or through any optical aid) Venus is rather dazzling, but if you observe it as early as possible in bright twilight, you should be able to detect its phase, which is currently around half. On the 9th Venus passes just above Regulus in Leo. A crescent moon lies nearby on the 15th.
The beacon of Jupiter reigns supreme to the SSW and is a rewarding target for any sized scope. Of course the larger the aperture, the more atmospheric detail becomes apparent, including the great red spot which is facing us on the following dates; 1st, 3rd, 5th, 8 th, 13 th,15 th, 17 th, 20 th, 22 th, 25 th, 27th and 29th; timings are for around 22:30h. The Galilean moons also provide great spectacle, throwing up a different configuration each evening. Usually 2, 3 or 4 are visible strung out in line with Jupiter. Notable satellite events to look out for during the late evening (22:30h) are a shadow transit of Io on the 10th and probably more noticeable a Ganymede shadow transit on the 31st. Our moon resides to the upper right of Jupiter on the 20th.
20-Jul-2018 at 23:00h (S):
The Moon, Venus and Jupiter
(Click for full-sized image)
24-Jun-2018 at 23:00h (S):
The Moon, Venus and Jupiter
(Click for full-sized image)
27-Jul-2018 at 23:00h (S):
Saturn, The Moon and Mars
(Click for full-sized image)
Next up we have Saturn, which starts to make inroads into the evening sky. Look for a conspicuous pearly ‘star’ low to the southeast as twilight deepens. Having not long reached opposition Saturn will lie due south around midnight. Ring orientation is currently very favourable and any modest telescope should reveal them, but do be patient, waiting for those steady ‘seeing’ interludes in the often turbulent air in which Saturn resides. The tiny speck close by Saturn will be its chief moon Titan, which orbits round in 16 days. The moon lies nearby on the 24th
Mars at Opposition
The Red planet is back in the spotlight, reaching opposition on July 27th (the same evening as the lunar eclipse). This will be the biggest and brightest appearance of Mars in 15 years with this opposition being perihelic, ie; one where Mars is closest to the Sun in its orbit. Unless you specifically wait up, Mars may seem a little shy to show its ‘ruddy’ face at first, not becoming a feature in the sky until late in the month. August will actually be more favourable.
As with all close oppositions of Mars, media attention will be good bad and indifferent, so pay no attention to the latter two, which usually involve erroneous claims of how Mars will appear as big as a full moon, dominating the sky. The same happened for the 2003 and 2005 oppositions. Mars will not be huge but it certainly will be conspicuous, rivalling Jupiter, if not exceeding it in brilliance around opposition. On July 27th there will be a large orange red presence low in the sky that evening... the rising full moon in eclipse, the orange hue of Mars will be located below the moon down in the south east and appear ‘substantially smaller’.
In fact when viewed through a telescope Mars will still appear rather small, even at the relatively close distance of almost 35.78million miles it will only be 24.3 arc seconds across. At 4,200 miles (6,800km) across, Mars is a little over half the diameter of our planet, appearing roughly half the size of Jupiter’s disk in the eyepiece and Jupiter lies 3 times further away! Our fascination stems from the knowledge that when we observe Mars, we are scrutinising the actual surface, viewing features on a world which once had seas, perhaps primitive life forms and the largest volcanoes in the solar system ; currently dormant.
Because this opposition (opposite the Sun in the sky) occurs in July, the declination of Mars will be quite low from our latitude, only 12 degrees or so above the south horizon at local midnight. Turbulent air will therefore interfere with observations, so patience at the eyepiece will be required. On Mars itself it will be early spring in the Southern Hemisphere and the beginning of the season in which large dust storms can develop. If one does, surface detail will become difficult to discern or be completely obscured, sometimes for several weeks, another reason why post opposition viewing is often more rewarding. Mars closest approach is actually on the last day of July, 4 days after opposition, when it will be slightly brighter at mag -2.8.
Apart from any meteorological phenomena on display, the most obvious features will be the polar caps, in particular the changing size of the southern one will be of interest, but there should be good views of the N. polar hood as well. The famous fin shape of Syrtis Major will be turned toward us on the 6-8th. On opposition night Mare Acidalium will be visible on Mars northern hemisphere, whilst to the south Mare Erythraeum and Solis Lacus will be evident. The two hour window centred on culmination will be the optimum time to observe. This means midnight to 02:00h from the UK I’m afraid.
Mars will be a dominant object well into late summer, allowing plenty of time to observe it – just don’t expect it to be as big a pizza.
Total Lunar Eclipse
The second total lunar eclipse of the year occurs on July 27th. The first lunar eclipse of 2018 occurred in January but was not visible from our shores. This eclipse is visible over most of Europe and Asia, Australia and South America. However, from the UK the start of the lunar eclipse will be hidden as the Moon will still be below the horizon, rising in the Earth’s umbra (the darkest part of the Earth’s shadow) and will already look red or blood orange.
A Rising Lunar Eclipse. (Image Credit: Gain Lee, Huddersfield Astronomical Society)
From Whitby this will be around 21:05h, clearing the horizon by 21:20h, just a few minutes before greatest eclipse occurs at 21:22h. At this point the Moon is closest to the centre of the Earth’s shadow. The umbral part of the eclipse ends at 22:13h, when the Moon leaves the deepest shadow and enters into partial phase, the orange/red colour will start to disappear, leaving a plain, dark shadow effect. This lasts until 23:19h, when the moon enters into Earth’s penumbral shadow, a much more subtle shade, lasting until 00:28h when the eclipse ends.
During totality the Moon does not disappear completely, but usually turns a deep, dark red or blood orange hue. This is because it is illuminated by light passing through the Earth's atmosphere and bending back towards the Moon by refraction. The colour of the moon at a total lunar eclipse is often influenced by earth’s atmospheric conditions, usually when there are higher than normal levels of dust or pollutants. Dust in the atmosphere blocks out the higher frequency blue light waves, but the longer wavelength of red light comes through. With several quite large volcanic eruptions occurring recently, it will be interesting to what effect this may have on the colour.
Meteors
A number of lesser meteor showers occur during July. The Capri-Cornids have 3 maxima, July 8, 15, and 26, but all have Zenith hourly rates (ZHR) of only half a dozen, the same as sporadic rates. Moon light will interfere with the last maxima.
The Alpha-Cygnids peak on July 21st, but again rates are barely more than sporadic levels. Cygnus is well placed high in the SSE by midnight. Moon light will interfere until after midnight.
The Delta-Aquarids are a little more prolific, peaking on July 30th with a ZHR of 15-18. Post midnight viewing is advised and there is little moonlight to bother about.
Noctilucent Cloud
Keep watch still for sightings of Noctilucent cloud as there has been some quite decent displays visible during the latter half of June. Mark observed this type of cloud (see last month for full feature) on several nights around midnight low to the north. Shining with a characteristic sliver blue hue, Noctilucent cloud is often on show from our latitude during June, July and sometimes early August.
Noctilucent Cloud taken in Whitby by Mark, on 25th June 2018 at 23:52h.
 |
 |
|
Looking North
Mid-July - 23:00h |
Looking South |
 |
 |
|
Looking East
Mid-July - 23:00h |
Looking West
Mid-July - 23:00h |
 |
 |
|
Northern Aspect
Mid-July - 02:00h |
Southern Aspect
Mid-July - 02:00h |
Additional Image Credits:
- Planets and Comets where not otherwise mentioned: NASA
- Sky Charts: Stellarium Software
In our tour of stellar objects crossing the meridian line this month: three objects from the constellation of Hercules. the 'Turtle' Planetary nebula, a open globular cluster M92, and star Alpha Herculis or Rasalgethi (‘the kneeler’s head’).
Planetary Nebula: Turtle (or NGC 6502)
Location of Hercules and
all of this month's objects
10-Jul-2018 at 23:00h
(Click for full-sized image)
Telescope, Medium
Located about 6500 light-years away in the constellation of Hercules, NGC 6210 was discovered in 1825 by the German astronomer Friedrich Georg Wilhelm Struve. Recording it as a small but bright nebula, we now know that NGC 6210 is a planetary nebula; the last gasp of a star slightly less massive than our Sun at the final stage of its life cycle. The striking high resolution image taken by the HST shows multiple shells of material ejected by the dying star forming structures with different degrees of symmetry, giving NGC 6210 its odd shape. The image shows the inner region of the planetary nebula in unprecedented detail, where the central star is surrounded by a thin, bluish bubble that reveals a delicate filamentary structure. This bubble is superposed onto an asymmetric, reddish gas formation where holes, filaments and pillars are clearly visible.
The still-heating 13th magnitude central star has a temperature of 58,000 Kelvin, probably rising to 100,000 Kelvin before cooling and eventually dimming. The nebula is expanding in its inner region by 21 kilometers per second, the outer part at 36 km/s. It is believed the original star had a relatively low mass, perhaps similar to our own Sun.
NGC 6210 has a very high surface brightness, making it a good target for small scopes and high magnification. Look for it between two nearly identical stars. In telescopes less than 8 inches NGC 6210 appears as a small, round, blue-green disk. Larger instruments and/or a UHC or OIII filter may reveal a faint outer shell. On nights of good seeing the 12.7 magnitude star should be visible at the centre. – Telescopic object –medium difficulty. Crosses south meridian at 11pm on July 3rd.
Two Hubble images of the 'Turtle' Planetary Nebula: NGC 6502 in Hercules.
(Right-hand image is a composite showing single- (red) and double- (green) ionised oxygen.)
Globular Cluster: M92
Telescope, Easy.
Discovered by Johann Elert Bode in 1777, the cluster was independently rediscovered by Charles Messier in March 1781 and added as the 92nd entry in his catalogue. M92 is at a distance of approximately 26,700 light-years away from Earth, similar to M13 in Hercules. With a total mass of 400,000 solar masses and a diameter of 110 light years it is though rather smaller than its more famous neighbour.
M92 is actually one of the brighter globular clusters in the northern hemisphere with an apparent magnitude of 6.3 but it is often overlooked by amateur astronomers because of its proximity to M13. In terms of absolute magnitude M92 is also among the brighter clusters, and one of the oldest, being 14 billion years old having a very low abundance of elements other than hydrogen and helium, what astronomers term its metallicity, characteristic of other globular’s. M 92 is located around 16,000 light years above the galactic plane and 33,000 light years from the Galactic Centre.
M92 is positioned north of the Keystone asterism in Hercules, between the Keystone star Eta Herculis and Iota Herculis. The cluster lies about 60 percent of the way from Eta to Iota. It forms a triangle with the two northernmost stars of the Keystone, Eta and Pi Herculis, which form the widest part of the asterism. In 10×50 binoculars, M92 appears like a blurry star with a brighter core. Small and medium-sized telescopes will resolve some of the stars in the outer regions of the cluster. 6-inch and 8-inch telescopes show an oval-shaped cluster with a bright centre, surrounded by a halo of stars. 12-inch telescopes resolve dozens of individual stars in the halo and throughout the cluster. The best time of year to observe M92 is July and early August, when Hercules is high overhead in the evening for northern observers. Telescopic – easy target. Crosses south meridian at 23:00h on July 10th.
Globular Cluster: M92 in Hercules (Image Credit: NASA/Hubble)
Star: Alpha Herculis (or 'Rasalgethi')
The stars of Hercules (above)
and the telescopic double star
Alpha Herculis (Image:
Dietmar Hager (Vienna, Austria))
Can see star with naked eye, but use Telescope to split, Medium
Alpha Herculis or Rasalgethi, from the Arabic meaning ‘the kneeler’s head’, is a red giant star some 40 million miles in diameter that varies from third to fourth magnitude (2.78 – 3.12). It is actually a triple star system some 359 light-years distant, the main components of which can be separated in amateur telescopes. The primary (alpha 1 Herculis) is a variable red giant, the secondary, a spectroscopic binary some 500 astronomical units away, (1 au = 93 million miles) orbits the primary every 3600 years, and is a blue-green hued star of magnitude 5.6. Rasalgethi is actually approaching us and will be closet in 2 million years time some 218 light years distant.
This star system shows nicely in a small telescope having quite a striking contrast. The brighter of the two is the red star, and the secondary the dimmer yellow giant. But visually, in a telescope, the fainter yellow star appears almost green against the red giant. They are 5 arc-seconds apart, so use at least moderate magnification to split them, say 80x or more.
Crosses meridian line at 11pm on July 10th.
Events
Observe the night sky with us at the Bruce Observatory, Caedmaon College - Normanby campus (formally Whitby College).
Observing Nights are held weather permitting: check for a relatively clear sky before leaving home. If in doubt, Mark can be reached on tel 01947 605516.
Please note the college drive gate is now operated via a electronic key code - so anyone wishing to attend must be at the car park at the top of the drive by 19:00hrs, unless an arrival time has been arranged with Mark/Keith after 19:30hrs. Otherwise shout or bip car horn - we'll hear.
Observe the night sky with us at the Bruce Observatory, Whitby School - formally Caedmon College - Normanby campus ).
Observing Nights are held weather permitting: check for a relatively clear sky before leaving home. If in doubt, Mark can be reached on tel 01947 605516.
Please note the college drive gate is now operated via a electronic key code - so anyone wishing to attend must be at the car park at the top of the drive by 19:00hrs - unless an arrival time has been arranged with Mark/Keith after 19:00hrs.
Observe the night sky with us at the Bruce Observatory, Whitby School - formally Caedmon College - Normanby campus ).
Observing Nights are held weather permitting: check for a relatively clear sky before leaving home. If in doubt, Mark can be reached on tel 01947 605516.
Please note the college drive gate is now operated via a electronic key code - so anyone wishing to attend must be at the car park at the top of the drive by 19:00hrs - unless an arrival time has been arranged with Mark/Keith after 19:00hrs.
