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Book review: Haynes manual – Saturn V

W. David Woods (2016). NASA Saturn V – 1967-1973 (Apollo 4 to Apollo 17 & Skylab) – Owner’s workshop manual – An insight into the history, development and technology of the rocket that launched man to the Moon. Haynes Publishing, Yeovil, Somerset. ISBN 978 0 85733 828 0. Hardcover, 27.2×20.8×1.4 cm. 172 pages, several photos or illustrations per page. £22.99 rrp.

ASE members will recall the author’s fascinating talk on how Apollo flew to the Moon. He has written other books on spaceflight, including co-authorship of the Haynes manuals on Gemini and the Lunar Rover. About 50 years after NASA settled on the Saturn IB and V designs as carrier for the Apollo programme, Woods places this iconic machine centre-stage and makes the engineering the story itself.

The first chapter deals with the history leading up to the Saturn rocket, not least Wernher von Braun and the German A-4, which under its belligerous assignation “V2” inflicted tens of thousands of casualties among the British population and the slave labourers that were forced to build it. Originally interested in spaceflight for its own sake, von Braun was again lead figure when NASA made spaceflight a civilian project again.

The main chapters deal with the rocket from the bottom up. The F1 engine is described in good and consistent detail. This is followed by the chapter about the S-IC stage – the first stage of the Saturn V and powered by five F1 motors. Description of the J2 engine is a bit shorter due to similarities with the F1. Both the second S-II stage and the third S-IVB stage are powered by five and one J2 motors resp. The bulk of the volume and mass of the rocket is necessarily in the tanks for liquid oxygen and fuel (kerosene in the S-IC and liquid hydrogen in the S-II and S-IVB). The IU instrument unit atop the third stage is given its own chapter as the brains of the rocket.

The penultimate chapter draws it all together and takes us through an average flight from launch to lunar transit injection and final disposal of the third stage. The average flight was not without complications, and so a variety of real flights serve to illustrate the problems that did occur on occasion.

The final chapter is about Skylab, which seems strange at first. The book otherwise refrains from speaking about the Apollo missions after the S-IVB had done its job and was usually orbiting the Sun or had crashed into the Moon. Launching the space station (without crew) was the last flight of a Saturn V. But also, Skylab itself was a modified S-IVB and in that sense part of the last Saturn V to fly.

It is fascinating to learn in some detail how these rocket motors work. There is elegance in the design, for example how the propellants are used to lubricate, and to drive the turbo pumps that then pump those same propellants to the combustion chamber. I was surprised that the iconic bell shape of the rocket motor nozzles is not solid metal cast or shaped from sheets, but is merely a collection of hundreds of parallel tiny metal pipes bonded together to make the shape required for best performance as an exhaust nozzle. One of the propellants is fed through these pipes down the nozzle wall and back up, both to cool the nozzle and to warm up the propellant, or even evaporate the liquid hydrogen prior to combustion.

The book has a lavish collection of high quality photographs and purpose-made drawings and diagrams, which make good use of colour. It does not so much work as a picture book, the text and pictures go together and match closely. Still, some diagrams illustrate more than the point in hand, such as the plot of g-force versus time into the rocket flight, which also illustrates how short the first-stage flight is compared to the second stage. In the text the level of detail is good and consistent.

There are a variety of technical terms used in the Saturn V programme. Some sound serious like “max-Q”, others may confuse like the two-page lecture on specific impulse in relation to weight and mass, resp. Others are refreshingly intuitive like the “pogo phenomenon” that could make astronauts very uncomfortable at times.

Should you wonder at the end, why some Apollo flights are hardly mentioned – Apollo 7, the three Skylab crew flights and the Apollo-Soyuz rendezvous – this is because they flew on the lesser, two-stage Saturn IB, which was sufficient to reach Earth orbit. Saturn V was all about the Moon, even if not much of the rocket itself reached the Moon. Some of its third stages flew by the Moon to enter solar orbit, others were crashed into the Moon to be monitored by seismometers already in place.

Horst Meyerdierks

Horst is currently Secretary of the Astronomical Society of Edinburgh and was the Journal’s previous editor, prior to it’s online incarnation.

Scotland’s Sky in July, 2016

Juno to begin hazardous mission at Jupiter

The maps show the sky at 01:00 BST on the 1st, midnight on the 16th and 23:00 on the 31st. (Click on map to enlarge)

The maps show the sky at 01:00 BST on the 1st, midnight on the 16th and 23:00 on the 31st. (Click on map to enlarge)

The Sun is edging southwards again but our night-long summer twilight subsides only slowly and, given that we also have bright moonlight through mid-July, we must wait until the month’s final week to enjoy a truly dark midnight sky.

From a good vantage point, we may then see the Milky Way as it arches high across our eastern sky, culminating close to the star Deneb in Cygnus. Deneb occupies the top-left corner of the Summer Triangle which remains a feature of our high southern night sky until the autumn. The Triangle was so named by our much-missed Sir Patrick Moore and has its other corners marked by Vega in Lyra and Altair in Aquila.

Sunrise/sunset times for Edinburgh change from 04:32/22:01 BST on the 1st to 05:16/21:21 on the 31st, by which date nautical twilight persists for two hours before dawn and after dusk. The Moon is new on the 4th, at first quarter on the 12th, full on the 19th and at last quarter on the 26th.

As the twilight fades at present, the giant planet Jupiter shines brightly low in the west and Mars, only a little fainter but distinctly reddish in hue, hovers at much the same altitude in the south-south-west. Our third naked-eye planet, Saturn, stands 18° to the east (left) of Mars and is creeping westwards in the southern reaches of the constellation Ophiuchus as Mars begins to accelerate eastwards in Libra.

Jupiter is nearing the end of its apparition as it sinks lower in our evening sky on its way to conjunction on the Sun’s far side in September. Its altitude above Edinburgh’s western horizon one hour after sunset falls from 11° on the 1st to less than 2° on the 31st. By then it will be difficult to spot in the bright twilight, and we will not see it again in our evening sky for another six months.

Moving eastwards in southern Leo, Jupiter remains brighter than any star, though it does fade slightly from magnitude -1.9 to -1.7 as its distance grows between 862 million and 919 million km. Viewed telescopically, its disk appears 34 arcseconds across when it stands 6° to the right of the crescent Moon on the 9th.

Although Jupiter is well past its best for telescopic study, we can expect some of our sharpest views after NASA’s Juno probe enters a highly-eccentric orbit over the planet’s poles early on July 5th UK time – the engine firing to do so is due to last for 35 minutes and end at 04:53 BST on that day. Launched in 2011, and with the benefit of a gravity assist flyby of the Earth in 2013, Juno will have travelled for 2,800 million km to reach Jupiter, not far shy of the distance between the Sun and Uranus.

Juno’s initial orbit is to carry it around Jupiter in 53.5 days, but this is to be reduced by mid-October to one of 14 days that takes within 4,200 to 4,900 km of the equatorial cloud-tops. That path plunges through Jupiter’s hazardous radiation belts and, while it avoids their most deadly regions, Juno’s sensitive electronics need to be located in a first-of-its-kind radiation-shielded vault.

Jupiter owns some of the most interesting moons we know of, but Juno is focused firmly on learning as much as possible about Jupiter’s origins and structure, from its intense magnetosphere all the way down to its core. The probe’s trio of 9-metres long solar panels provide 500 watts of power, making it the first craft to rely on solar power so far from the Sun. If it survives, the plan calls for Juno to dive to a fiery destruction in Jupiter’s atmosphere in February, 2018.

Venus, brilliant at magnitude -3.9, stands closer to the Sun in our evening twilight than Jupiter and is unlikely to be seen from our latitudes. Mercury, much fainter, enters the same area of sky following its superior conjunction on the Sun’s far side on the 7th and is even less likely to be seen.

Mars dims from magnitude -1.4 to -0.8 this month as its distance grows from 86 million to 106 million km and its diameter shrinks from 16 to 13 arcseconds. Telescopes still show some detail on its rusty surface, but it, too, stands lower each evening and by the month’s end it sets before midnight BST. Look for Mars 7° below the gibbous Moon on the evening of the 14th.

The opposing motions of Mars and Saturn mean that their separation in the sky decreases to 11°, with Saturn fainter at magnitude 0.2 to 0.4 and noticeably above-left of Mars by the month’s end. The red supergiant star Antares in Scorpius lies 6° below Saturn while the Moon stands 5° above-right of Saturn on the 15th and 9° to the planet’s left on the 16th.

Viewed telescopically, Saturn appears 18 arcseconds wide at mid-month with the north face of the rings inclined 26° towards us and 40 arcseconds from side to side. Saturn’s main moon, Titan, shines at magnitude 8.5 and is best seen through a telescope as it orbits every16 days. Catch it 3 arcminutes west of Saturn on the 4th and 20th, and a similar distance east on the 11th and 27th.

It happens that my previous note was timely in its warning about noctilucent clouds. The first good displays were sighted within a couple of days, appearing as electric-blue cirrus-like banks low above the north-western horizon after dusk and shifting round into the north-east before dawn. Composed of ice-crystals some 82 km above the ground, we should expect further shows until mid-August.

Alan Pickup

This is a slightly-revised version of Alan’s article published in The Scotsman on July 1st 2016, with thanks to the newspaper for permission to republish here.

Scotland’s Sky in April, 2014

Mars shines brightly at opposition in Virgo

2014_Apr_ase

The maps show the sky at midnight BST on the 1st, 23:00 on the 16th and 22:00 on 30th. An arrow depicts the motion of Mars. (Click on map to enlarge)

Six years have passed since Mars was as close and bright as it is this month, but two other planets outshine it and a fourth, Saturn, will soon be at its best for the year. There are also two of 2014’s four eclipses but, as with the second pair in October, neither is of much interest for observers in Scotland.

For the moment, our evening sky retains a flavour of stellar feast we enjoyed over the winter. Orion is still on show in the south-west at nightfall below the conspicuous planet Jupiter. Orion’s Belt now lies almost parallel to the horizon, a line along it pointing to the left towards Sirius, our brightest nighttime star, and to the right towards Aldebaran and the Pleiades in Taurus. By our star map times, though, Orion has all but sunk below our western horizon.

Jupiter, however, continues as our brightest evening object bar the Moon. As it slips 3.5° or seven Moon-widths eastwards in the middle of Gemini during April, it fades a little between magnitude -2.2 and -2.0 and its telescopic diameter shrinks from 38 to 35 arcseconds. The earlier in the night that we catch it, the higher it stands and the sharper the view of its cloud-banded disk. By our map times Jupiter is some 30° high in the west and on its way to setting in the north-west four hours later.

The month begins with impressive views of the young earthlit Moon in the west at nightfall. It is only 5% illuminated on the 1st as it stands 14° high forty minutes after sunset. Look for it below the Pleiades on the 2nd, below the Aldebaran-Pleiades line on the 3rd and 6° below Jupiter on the 6th as it nears first quarter.

Mars reaches opposition on the 8th when it lies 93 million km away and shines at magnitude -1.5 so that its orange-red beacon rivals Sirius in brightness if not in colour. By definition, it stands opposite the Sun in the sky so that we find it climbing from the eastern horizon as the evening twilight fades to pass 28° high on Edinburgh’s meridian two hours after our map times. As the arrow on our south map shows, Mars tracks 10° westwards in Virgo during April, from 5° above the magnitude 1.0 Spica today to lie 1.6° below-left of the famous binary star Porrima as the month ends.

Often the day of opposition is when a planet is closest to us but Mars is approaching the Sun in its orbit and is 450,000 km closer to us on the 14th than on the 8th. Through a telescope, its ochre disk is 15 arcseconds wide and shows dusky markings and the dwindling white smudge of its north polar ice cap, tipped about 22° towards us.

The full Moon lies below Mars on the evening of the 14th and is approaching Spica as it sets for Edinburgh at 06:08 BST on the 15th. Only 14 minutes before this, and while it is less than 2° above the west-south-western horizon in the twilight, it begins to enter the outer shadow of the Earth, the penumbra. Sadly, we have no hope of seeing any dimming of the lunar disk before it sets. Observers in the Americas are much better placed to view the resulting total eclipse of the Moon which is total from 08:07 until 09:26 BST (03:07 to 04:25 EDT).

Sunrise/sunset times for Edinburgh change from 06:44/19:51 BST on the 1st to 05:32/20:50 on the 30th while the duration of nautical twilight at dawn and dusk stretches from 84 to 105 minutes. After first quarter on the 7th, the Moon is full during the eclipse on the 15th, at last quarter on the 22nd and new on the 29th when a small area of Antarctica and perhaps a few penguins experience an annular eclipse of the Sun. A partial solar eclipse is visible from Australia and the southern Indian Ocean.

On course to reach opposition in May, Saturn rises at Edinburgh’s east-south-eastern horizon at 23:31 on the 1st and only 36 minutes after sunset by the 30th, climbing to pass 18° high on the meridian four hours after our map times. Improving from magnitude 0.3 to 0.1, it edges westwards in Libra and draws ever closer to the Moon overnight on the 16th-17th when Saturn’s disk is 18 arcseconds wide while its stunning rings span 42 arcseconds.

Mercury is hidden in the dawn twilight until it passes around the Sun’s far side on the 26th. Venus, brilliant as a morning star, rises in the east-south-east seventy minutes before sunrise on the 1st and in the east only 51 minutes before the Sun on the 30th. Dimming from magnitude -4.3 to -4.1, its gibbous disk shrinks from 22 to 17 arcseconds in diameter.

It is less than a month since results from NASA’s WISE spacecraft appeared to rule out any Jupiter or Saturn-sized planet lurking unseen in the outermost solar system. Now we learn that a new dwarf planet, dubbed 2012 VP113, has been found to have an orbit that comes no closer to the Sun than 80 times the Earth’s distance, further than any other known object in the solar system. Thought to be a ball of rock and ice perhaps 450 km wide, it may be six times further away at its farthest, and take perhaps 5,000 years to complete each orbit.

Surprisingly, 2012 VP113’s orbit is similarly orientated to those of some other remote bodies, including the only other comparable object, Sedna. There is speculation that this is because they are influenced by a larger undiscovered world, perhaps a super-Earth, even further out.

Alan Pickup

This is a slightly-revised version of Alan’s article published in The Scotsman on April 2nd 2014, with thanks to the newspaper for permission to republish here.