Early risers can see Venus each morning before dawn low in the north-east. Those who are not early birds will need to wait until November when Venus will switch to the evening sky. Tomorrow morning a thin crescent Moon is near Venus; it is above and to the right or east of the planet.
Venus, Mercury and the Moon on the morning of 25 July 2014. Chart Nick Lomb
The entrance of the Adler Planetarium. Note the large poster advertising the planetarium’s premier sky show, Destination Solar System, on the left, while on the right a poster advertises the popular exhibition for young children, Planet Explorers. Photo Nick Lomb
At the beginning of July 2014 I visited one of my favourite places in the world, the Adler Planetarium in Chicago. Like the Griffith Observatory in Los Angeles that I had visited two days earlier, it is spectacularly located though not on hills but on a small peninsula jutting into Lake Michigan with a wonderful view of the Chicago skyline.
Again like Griffith Observatory, it has been extended relatively recently. Instead of digging underneath the original heritage building the Adler Planetarium was extended with a glass Sky Pavilion that opened in 1999 and provided extra space with great views for exhibitions and a cafeteria.
A panorama of the Adler Planetarium and the Chicago skyline visible from there. Click on the image for a larger view (same with the other images in this post). Photo Nick Lomb
There have been more recent developments as well. Soon after my last visit in 2011 the new Grainger Sky Theatre opened; this 300-seat sky theatre is believed to be the most sophisticated in the world. Its 20 projectors are controlled by two supercomputers, 46 servers and 42 Nvidia Quadro GPUs (graphic processor units) and provide a screen image of 8000 by 8000 pixels or 64 megapixels. This image, which is refreshed 30 times a second, is sharper than the resolution of the human eye.
To experience the Grainger Sky Theatre I booked our little group into seeing the Adler’s premier show, Destination Solar System. It was not cheap, as to see it is necessary to purchase Anytime All Access passes at $34.95 adults and $29.95 for children. Still it is worth the cost for the 30-minute show plus the pass allows viewing all other shows at the planetarium together with all the exhibits.
The Adler Planetarium can be seen (circled) in this view from the Chicago Skydeck, on the 103rd floor of the Willis (formerly Sears) Tower, which is the second tallest building in the United States. Photo Nick Lomb
To my pleasant surprise the show was very much designed with young children in mind and perfectly suited the three 8 to 11 year olds in our group. The fun began in the entrance foyer as we waited to be allowed into theatre. We were told that it is the year 2096 and we were about to undertake a tour of the highlights of our solar system. Inside, after the theatre filled the show began with the blast off into space. There was a live guide Jesse who wandered among the audience telling us about what we were seeing, all the while bantering with both members of the audience and the spaceship’s computer Max.
The images were truly impressive with sights ranging from the surface of the Moon to activity on the Sun’s visible surface together with visits to Titan, Mars and the asteroid belt. Certainly all the highlights in the solar system were visited. At one stage there was a serious problem with our spaceship and Jesse heroically had to make an emergency repair (I do not want to give too much away). No surprise that the three children in our group loved the show.
I wondered about Jesse as he seemed far too good an actor to be a usual planetarium presenter. A little subsequent research told me that there are six Jesses, or possibly three Jesses and three Jessies as three are male and three female. They are all actors with experience in improvisation and were given some astronomical training by the Adler staff.
We did see another of a number of shows on offer at the Adler Planetarium, but Destination Solar System is highly recommended, especially for those with children in tow. Presented in a state-of-the-art sky theatre, the show is fun and in a refreshingly new style.
The southern galaxy Centaurus A is relatively nearby at a distance of only 12 million light years from us. From a dark place away from city lights, it is easily visible through a small telescope. At its centre there is a massive black hole with a mass 55 million times that of our Sun.
Centaurus A. Courtesy ESO
Changes in sunspot group AR12109 plotted on four separate days. Sketch and copyright Harry Roberts ©, all rights reserved
The first week of 2014 July saw the Sun’s south-eastern hemisphere ‘peppered’ with large and complex sunspots – some reached (suitably protected) ‘naked-eye’ size! A wondrous sight in white light (WL): they were somewhat disappointing in H-alpha, with few dark filaments and modest plages. Let’s consider one of the biggest: NOAA AR12109.
AR12109 rounded the east limb on July 2nd (Fig1), looking like a typical large single spot (McI: Hsx) but for some faint patches of following (f) penumbra that may have held small attendant spots. A day earlier there had been strong signs of a large group approaching, with a spiky ‘crown’ of small but bright surges sited at –10,219. As surges occur only around sunspot penumbrae, a cluster of ‘spikes’ at the limb suggested a big spot just behind it. When first seen on the 2nd the (p) spot was already 16º from the limb, i.e. in good ‘seeing’ it might have been detectable on the 1st.
By the 3rd (Fig2) it was clear that 2109 was a complex spot group with the large (p) spot and its conspicuous light bridge attended by dozens of small spots, many in chains, suggesting complex magnetic mixes. The (p) spot was sited at –8,222 and the most remote follower (f) at –6,214: it was a new sunspot group. Mt. Wilson polarities showed red 2200G (R22) in the (p) spot and violet 1300G (V13) in the follower (f). Helio freeware © Peter Meadows gave the group an area of 650 units: a large group given this weak solar cycle.
The 5th saw the group larger than 700 units (Fig3) with the previously ‘roundish’ (p) spot now changing shape while the followers developed larger irregular penumbrae. There were now some conspicuous surges or filaments emanating from the (p) spot with one looping out of the (p) and returning to the middle of the group after an excursion some 7º northwards.
Flare. A flare erupted along what was likely the polarity boundary between red and violet spots, beginning as a sub-flare at 00:21 and reaching GOES C4 at 00:25: a minor but ‘pretty’ event.
The preceding spot now had an umbral field of R24 while the (f) spots remained at low values. Mt Wilson workers who detected mixed fields in it assigned Hale DELTA configuration to the group on the 8th. I had no detailed log of it on that day – but on the 10th (Fig4) it was also Beta-Gamma-Delta with R2600G in the (p) spot. The tiny V13 (arrowed) was deemed a DELTA mix by Mt. Wilson, while I saw that spot as separated from its red siblings by a small penumbral gap. Much earlier NOAA had deemed the group Delta class based, it seems, on disc magnetograms rather than the ‘original’ Hale definition of ‘mixed fields within the one penumbra’.
This was a most impressive sunspot group – Earth is shown dotted in Fig4; large in area with complex Delta class fields, yet its flare activity never exceed GOES C-class during its disc transit. What was missing?
One key ingredient of flaring is helicity: the degree of ‘twist’ in umbral fields. Perhaps the solar dynamo is generating fields with less helicity and that, combined with low power fields, results in lesser flares? It is noted that the vast coronal canopies formed above active regions by the sunspot fields (SDO daily logs), currently seem rather modest when compared to earlier records (e.g. year 2011). Is this effect real?
Perhaps time and more research will tell. Meanwhile, AR12109 was a great sunspot to follow as it rapidly evolved during its stately transit of the solar disc; will it reappear around August 1st? Keep a watch for clusters of small bright surges at the southeastern limb.
Harry Roberts is a Sun and Moon observer, a regular contributor to the Sydney Observatory blog and a member of the Sydney City Skywatchers.
Each of the gas giants in the outer solar system are circled by rings. The rings of the outermost planet Neptune were first discovered as arcs on this day in 1984. Five years later the Voyager 2 spacecraft imaged five rings as it passed the planet. One of these rings, the Adams ring, has five arcs some of which had been the ones discovered earlier.
Voyager 2 image of the rings of Neptune. Courtesy NASA/JPL
Australia’s research astronomers have gathered at Macquarie University for the annual scientific meeting of the Astronomical Society of Australia. They are discussing the latest studies of the origin of the Universe and the formation of galaxies as well the development of new instruments.
Part of conference logo. Courtesy ASA and Macquarie University
This weekend the Central West Astronomical Society holds its annual AstroFest in the NSW country town of Parkes, the home of “The Dish”. During the day on Saturday there are a series of fascinating talks while in the evening the winners of the prestigious David Malin Awards photography competition are to be announced.
David Malin with the 2012 overall winner Phil Hart. Photo Nick Lomb
The first American into space, John Glenn, was born on this day in 1921 in Cambridge, Ohio and so celebrates his 93rd birthday today. Glenn first circled the Earth in the one-person Mercury spacecraft Friendship 7 in 1962. 36 years later, at the age of 77 he embarked on another space flight aboard the space shuttle Discovery.
John Glenn. Courtesy NASA
A young crescent Moon. Photo Nick Lomb
The first visibility of the crescent Moon after the astronomical instant of new Moon is not only of interest to astronomers, but is of particular significance in the Islamic calendar. The crescent Moon is always first visible after sunset. For it to be visible the Moon has to have moved away from the glare of the Sun and it has to be suitably high above the horizon at sunset so that there is time for the sky to become sufficiently dark before moonset.
A number of criteria for predicting the visibility of the crescent Moon have been developed over the years.
The simplest useful criterion is the lagtime between sunset and moonset. If that time is greater than 47 minutes (at the latitude of Sydney) the crescent Moon should be visible to the unaided eye after sunset and before the setting of the Moon. This value for the time lag at Sydney’s latitude comes from the work of Mohammad Ilyas of the University of Science Malaysia (Quarterly Journal of the Royal Astronomical Society, volume 35, pages 425 to 461, 1994).
In July 2014 the Islamic month of Shawwal begins after the new Moon of 27 July. Although this occurs in the morning at 8:42 am AEST, there is no possibility of the Moon being seen that evening as in Sydney it sets only 24 minutes after the Sun.
A global map of the visibility of the Moon for 27 July is shown here. The map clearly indicates that the new Moon is not visible that day from Australia, but under perfect conditions can be seen from most of South America.
From Sydney the crescent Moon will be visible on Monday 28 July. The best time to view will be 5:47 pm when it be at azimuth 289° and altitude 7°. Its age at the time will be 33 hours 5 minutes.
Finding chart for the crescent Moon from Sydney at 5:47 pm AEST on 28 July 2014. Chart made with Stellarium
Anyone interested in trying to view the crescent Moon needs to find a place with a good view towards the western horizon as it will be very low in the sky. A pair of binoculars could help to locate it first in the still bright sky and only expect to see the crescent if the sky towards the west is absolutely free from clouds. Please let us know in the comments if you do manage to see the crescent Moon.
The above information is an extract from a previous post titled, The visibility of the crescent Moon from Sydney in June and July 2014. It is reposted for the convenience of readers.
On this date in 1994 the first fragment of Comet Shoemaker-Levy 9 crashed into the giant planet Jupiter followed by many more over the next five days. This was the first time that a collision between a comet and a planet has been observed. There were at least 21 fragments with sizes up to two kilometres in width.
Hubble Space Telescope image of impact sites on Jupiter. Courtesy Hubble Space Telescope Comet Team and NASA