Sunday 6 November 2011

The latest Stellarium available


2011/11/04

Stellarium 0.11.1 has been released!

The Stellarium team is proud to announce the release of version 0.11.1. This is an important bug fix release closing more than 20 bugs in the main application and in the plug-ins. It also brings small GUI usability improvements. A huge thanks to all community bug reporters who helped us a lot finding bugs! You can find the full list of changes the change log.

We have updated the configuration file and the Solar System file, so if you have an existing Stellarium installation, you need to reset the settings after you install the new version.
  • Bring a memory stick to the next meeting (ASSA Bloemfontein).  It will be available!



Sunday 23 October 2011

Hot News: Supernova 2011gv in Galaxy IC4901

 
 
This image shows supernova SN2011gv, discovered last week by IceInSpace member Greg Bock as part of the amateur BOSS supernova searching team. The supernova is in the galaxy IC4901, in the constellation Pavo and is marked by the 2 lines near the centre of the galaxy. Greg Bock has taken tens of thousands of images hunting for supernova over the years, and to finally get one must be very satisfying for him. Image by Greg Bradley with an FLI Microline 8300 and Planewave CDK17, 70 mins exposure.

Saturday 8 October 2011

Sterrekundewoordeboek / Dictionary of astronomy


Sterrekundewoordeboek 

Die Suid-Afrikaanse Akademie vir Wetenskap en Kuns gee vir ons `n aanlyn  Sterrekundewoordeboek / Dictionary of astronomy.

(
Afrikaans – Engels)

Voorbeeld

aangroeistroom (akkresiestroom) : accretion stream
aangroeitempo (akkresietempo) : accretion rate, rate of accretion
aangroeiteorie (akkresieteorie) : accretion theory aanjaagvuurpyl : booster rocket aanraking (kontak) : contact aantrek : attract aantrekking : attraction aantrekkingsfeer (sentrosfeer) : attraction sphere, centrosphere aantrekkingskrag : attractive force
    - Die Engels/Afrikaans-weergawe is later beskikbaar

Ruimtewoordeboek in Afrikaans

`n  Engels/Afrikaans  en Afrikaans/Engels Woordeboek van Ruimteterminologie is in Kaapstad  deur die Internasionale Akademie van Ruimtevaart  (IAA) bekend gestel.
  • Dit is ook aanlyn beskikbaar   (Meer inligting sodra die skakel werk)

Pharos Speller Speltoetser
Nog `n stukkie inligting vir ouens wat met Afrikaanse spelling van woorde sukkel.

Die gewilde Pharos Speller Speltoetser & woordafbreker is pas opgedateer en bygewerk en is nou versoenbaar met Windows 7.
     


A Photographic Atlas of Selected Regions of the Milky Way





A Photographic Atlas of Selected Regions of the Milky Way
Edward Emerson Barnard, Yerkes Observatory, Wisconsin


Edward Emerson Barnard's Photographic Atlas of Selected Regions of the Milky Way was originally published in two volumes in 1927. Together these volumes contained a wealth of information, including photographic plates of the most interesting portions of the Milky Way, descriptive text, charts, and data. Only 700 copies were printed, making the original edition a collector's item. Reproduced in print for the first time, this edition combines both volumes of Barnard's Atlas. It directly replicates Barnard's text, and contains high resolution images of the original photographic plates and charts, reordered so that they can be seen together. It also includes a biography of Barnard and his work, a Foreword and Addendum by Gerald Orin Dobek describing the importance of the Atlas and additions to this volume, and a pull-out section with a mosaic of all 50 plates combined in a single panorama.

Sunday 2 October 2011

Speed-of-light results under scrutiny at Cern

Enormous underground detectors are needed to catch neutrinos, that are so elusive as to be dubbed "ghost particles"

Source: BBC





A meeting at Cern, the world's largest physics lab, has addressed results that suggest subatomic particles have gone faster than the speed of light.
The team has published its work so other scientists can determine if the approach contains any mistakes.
If it does not, one of the pillars of modern science may come tumbling down.
Antonio Ereditato added "words of caution" to his Cern presentation because of the "potentially great impact on physics" of the result.
The speed of light is widely held to be the Universe's ultimate speed limit, and much of modern physics - as laid out in part by Albert Einstein in his theory of special relativity - depends on the idea that nothing can exceed it.

Thousands of experiments have been undertaken to measure it ever more precisely, and no result has ever spotted a particle breaking the limit.
"We tried to find all possible explanations for this," the report's author Antonio Ereditato of the Opera collaboration told BBC News on Thursday evening.
"We wanted to find a mistake - trivial mistakes, more complicated mistakes, or nasty effects - and we didn't.
"When you don't find anything, then you say 'well, now I'm forced to go out and ask the community to scrutinise this'."
Friday's meeting was designed to begin this process, with hopes that other scientists will find inconsistencies in the measurements and, hopefully, repeat the experiment elsewhere.
"Despite the large [statistical] significance of this measurement that you have seen and the stability of the analysis, since it has a potentially great impact on physics, this motivates the continuation of our studies in order to find still-unknown systematic effects," Dr Ereditato told the meeting.
"We look forward to independent measurement from other experiments."

The Ten Commandments for Amateur Astronomers


 Sourced from October Canopus, Newsletter - ASSA Johannesburg Centre

  • Articles about the Bloemfontein visit in Canopus.

Submitted by Annelie Hoberg; Source: www.physlink.com, Anonymous

1. Thou shalt have no white light before thee, behind thee, or to the side of thee whilst sharing the night sky with thy fellow stargazers.
2. Thou shalt not love thy telescope more than thy spouse or thy children; as much as, maybe, but not more.
3. Thou shalt not covet thy neighbour's telescope, unless it exceeds in aperture or electronics twice that of thy wildest dreams.
4. Thou shalt not read "Astronomy" or "Sky & Telescope" on company time, for thine employer makes it possible to continue thine astronomical hobby.
5. Thou shalt have at least two telescopes so as to keep thy spouse interested when the same accompanies thee under the night sky or on eclipse expeditions to strange lands where exotic wild animals doth roam freely.
6. Thou shalt not allow either thy sons or thy daughters to get married during the Holy Days of Starfest.
7. Thou shalt not reveal to thy spouse the true cost of thy telescope collection; only the individual components and that shall be done with great infrequency.
8. Thou shalt not buy thy spouse any lenses, filters, dew shields, maps, charts, or any other necessities for Christmas, anniversaries, or birthdays unless thy spouse needs them for their own telescope.
9. Thou shalt not deceive thy spouse into thinking that ye are taking them for a romantic Saturday night drive when indeed thou art heading for a dark sky site.
10. Thou shalt not store thy telescope in thy living room, dining room, or bedroom, lest thou be sleeping with it full time.

Neville Young's book "Astronomy - Yes You Can"




New book - by Neville Young This composite photograph shows Fred Oosthuizen with the Stevick-Paul telescope that he built and mounted inside his observatory on the roof of his house. The photograph is being included in Neville Young's book "Astronomy - Yes You Can" which will reach the bookshops in March next year. Neville is a former chairman of the Pretoria Centre and is still a member of it. 

The book is also being translated into Afrikaans by Bosman Olivier, a committee member of the Pretoria Centre. The book is intended to interest the layman in astronomy particularly and in science generally, but has been received with great interest by the experienced amateur Michael Poll and the professional Barbara Cunow, who are helping Neville to ensure that the content of the book will be accurate. 

Friday 9 September 2011

NASA’s Cassini orbiter snaps unbelievable picture of Saturn

Click to enlarge

Science fiction movies have spoiled us on high definition views of our planetary neighbors, but real-life photographs with equal jaw-dropping potential are exceedingly rare. That's what makes NASA's awe-inspiring snapshot of Saturn (hi-res version here) such a stunning piece of eye candy.

Taken by NASA's Cassini robotic orbiter, the shot was captured from the dark side of Saturn as the Sun's bright rays illuminated every piece of dust and debris circling the planet. Cassini has offered astronomers a never-before-seen look at Saturn and revealed more information about the planet than any craft before it. The craft has taken so many pictures of the ringed wonder that they were recently made into a short flyby film that looks like it was created by George Lucas rather than a robotic space explorer.

The Cassini probe was launched in 1997 and took a further 7 years to reach Saturn's orbit. The total cost of its overarching objective of studying the ringed planet stands at a staggering $3.26 billion. However, the wealth of information it has wrought — including amazing pictures like the one above, and recordings of massive lightning storms on the planet — have already made it one of the best investments in space exploration. Hopefully Juno — which began a 5-year trek to Jupiter just last month — will bring us some equally stunning shots of Saturn's neighbor.
[Image credit: NASA]

Thursday 8 September 2011

Transit of Venus, 2012


The next transit of Venus will occur on June 5–June 6 in 2012, succeeding the previous transit on June 8, 2004. After 2012, the next transits of Venus will be in December 2117 and December 2125.

Monday 29 August 2011

Astronomers discover planet made of diamond


LONDON (Reuters) - Astronomers have spotted an exotic planet that seems to be made of diamond racing around a tiny star in our galactic backyard.
The new planet is far denser than any other known so far and consists largely of carbon. Because it is so dense, scientists calculate the carbon must be crystalline, so a large part of this strange world will effectively be diamond.
"The evolutionary history and amazing density of the planet all suggest it is comprised of carbon -- i.e. a massive diamond orbiting a neutron star every two hours in an orbit so tight it would fit inside our own Sun," said Matthew Bailes of Swinburne University of Technology in Melbourne.

Sunday 28 August 2011

Kollimasie werkswinkel


Met al die sirkeltjies en swart kolletjies in plek gaan jy net baie beter sien met jou teleskoop. By `n werkswinkel wat Thinus van der Merwe en Brett du Preez by die Boyden-sterrewag vir amateur sterrekundiges aangebied het, het lede geleer hoe om onder meer `n Cheshire kollimeerder te gebruik. 

Tipiese somer vlieswolke het die dieplugwaarneming in die wiele gery, maar daar was genoeg oop kolle om vinnig na Tuc 47 (NGC 104) en ook  `n paar ander voorwerpe te kyk.

Komeet C/2009 P1 (Garradd) in Sagitta was ook op die spyskaart en is en Wessel du Preez van Senekal het dit vinnig met sy nuwe 10" Skywatcher opgespoor. Net so links onder M71 (sterbondel).

  • Vroeër die middag het James Ross gehelp om al die spieël wat geslyp word se randjies te "bevel". Hy en Thinus het ook geloer of almal nog op die regte spoor is met die harde werk.

Saturday 30 July 2011

2012 Karoo-sterrefees

Die Sterrefees by Kambro Padstal by Britstown is in Weg, die reistydskrif aangekondig.
  • Kambro padstal was een van die naaswenners in Weg se kompetisie vir padstalle in Suid-Afrika.
  • 21 - 25 Maart 2012

Gerrit Penning en Pieter Pieterse maak reg vir die nag se waarnemings by Britstown tydens die 2011 sterrefees.
KAROO STARPARTY 2012

The ASSA Pretoria Centre is continuing the annual National Karoo Starparty which was started in
2009 at the Kambro Padstal, about 20 km north of Britstown in the Karoo, next to the N12 National Road. This event is intended to be a get-together for friends that want to enjoy the beautiful Karoo sky and there are no scheduled events, talks or workshops – we go there simply to enjoy the company of fellow stargazers and the legendary Karoo sky. 

The date for the 2012 Starparty is scheduled for the week-end of 21 March 2012. That is Wednesday 21 to Sunday 25 March 2012.

- Wednesday 12 March is a National Holiday. Please book early to avoid dissappointment! 

There is also accommodation available in Britstown at the Karoo Country Inn.

See http://www.kambroaccom.co.za or phone Wilma Strauss at 0833056668 for details of the site and to make a booking.

- Kambro Padstal by Britstown   GPS S30°-25-00.3 E23°-33-56.1

Thursday 28 July 2011

A Southern Comet on its way to us

 Copyright © 1995 by Tim Puckett


This image was taken by Tim Puckett (Villa Rica, Georgia, USA) on 1995 December 28.99, using a 0.30-m f/7 Meade LX-200 and an SBIG ST-6 CCD camera. It is a 300-second exposure.

16 August 2011: Closest approach of the brightest comet of the year
Comet: 45P/Honda-Mrkos-Pajdušáková
Visible: August until September, fading in October
Magnitude: 6
Finder charts: Sky Guide (pg 31)

 45P/Honda-Mrkos-Pajdušáková

 The comet Honda-Mrkos-Pajdusakova is expected to brighten rapidly in August as it passes to the south of the Earth. It will be observable from the southern hemisphere for about 2 weeks before getting too close to the Sun.

At its closest the comet will be 0.060 AU from the Earth, that is about 9 million kilometers away. While this is close for a comet, it is still about 24 times the distance of the moon. When it is first at magnitude 10, on the evening of August 9/10 it will be visible from New Zealand throughout the night, setting only briefly during daylight hours. For the next few nights until August 16 it will be circumpolar although low in the sky in the evening. On the 17th it will set briefly in the evening to rise again about midnight.

Over the next few days, as the comet moves north it will rise after midnight so becoming a morning object. Its elongation from the Sun will decrease as the comet moves away from the Earth towards the Sun and it will rise later in the morning to become lost in the morning twilight by about August 23.

By mid September Honda-Mrkos-Pajdusakova will be an 8th magnitude object rising about 90 minutes before the Sun into the dawn sky. The comet will then be slow moving in Leo, a few degrees from Regulus. By mid October it will have faded to magnitude 10.

45P/Honda-Mrkos-Pajdušáková is a periodic comet discovered by Minoru Honda December 3, 1948. The comet is named after Minoru Honda, Antonín Mrkos and Ludmila Pajdušáková. The orbit is elliptical with a period of 5.252 years. The comet nucleus is estimated to be 1.6 kilometers in diameter. (Information from Wikipedia.) 

45P/Honda-Mrkos-Pajdusakova
Perihelion: 2011 September 28
Maximum magnitude about 7 

 

Thursday 21 July 2011

Vaarwel aan NASA se ruimtependeltuig, Atlantis

Willie Koorts:

Wat ‘n fantastiese manier om die Pendeltuig program vaarwel te roep!  Na Oleg se voorspelling dat die twee ‘n paar minute uitmekaar sou wees en Rudie se opmerking op Facebook dat hulle verby die Suiderkruis gaan vlieg, het ek my foto beplan deur op een plek te konsentreer en agterna die fotos te kombineer.  Ek was so besig om te konsentreer op Atlantis, dat ek eers later besef het dat ISS so kort na dit volg, om die waarheid te sê, hulle was naby genoeg om in een veld te pas, maar ek moes deurdruk met my beplande foto.
Dit was wonderlik dat ons so goed geplaas was vir die swanesang, en boonop ook nog perfekte weer in die middel van die winter!

Monday 11 July 2011

Happy first birthday, Neptune!

On 12 July, Neptune will celebrate its very first birthday because exactly one Neptunian year -- or 164.79 Earth years -- will have passed since its discovery.
Neptune was mathematically predicted before it was first telescopically observed on 24 September 1846. Astronomer Johann Gottfried Galle and his assistant Heinrich Louis d'Arrest used Urbain Le Verrier's calculations to locate the planet. It was found to be within a single degree of where Le Verrier had predicted it would be and it was the first planet to have been discovered deliberately.

More...

Thursday 23 June 2011

How to tick the Horesehead nebula of your astro bucket list

Seeing the Horsehead with a filter is a real accomplishment; finding it without one is something to very be proud of!


Dark Nebula w/nebulosity
aka B33, LDN 1630

Minimum requirements to detect: 8-inch scope under dark skies


Monday 20 June 2011

Nog `n maanverduisteringfoto

Frans Human van ASSA Bloemfontein het hierdie samestelling van die totale maanverduistering afgeneem.


Friday 17 June 2011

Total Lunar Eclipse , 15 June 2011 - Animation




Click on Picture to view eclipse animation

Photos: Hannes Pieterse

Tuesday 14 June 2011

Onthou: Algehele Maanverduistering, 15 Junie 2011


 Tye volgens The Sky 6:

19:24: Beweeg in Penumbra in
20:23: Beweeg in Umbra in (Verduistering is meer sigbaar)
21:23: Algehele verduistering begin. Maan in in rooi gloed gehul.
23:03 Algehele verduistering eindig. Beweeg in penumbra in. (Maan word meer strokie-vir-strokiesigbaar)
00:04 Maan uit Umbra en in Penumbra.
01:04  Maan uit Penumbra en algehele verduistering is verby.

Reminder: Total Lunar Eclipse, 15 June

Friday 10 June 2011

NGC 3324, Gabriela Mistral nebula vanaf Boyden-sterrewag, Bloemfontein

Klik om te vergroot

NGC 3324, Gabriela Mistral nebula
Constellation: Carina (Car)
Foto: Brett du Preez, ASSA Bloemfontein
Atik 383L+
280mins Ha data
20mins subs
127mm Apo triplet refractor
Cgem off axis autoguided with Meade dsi pro
Captured with Maxim DL 5, Sigma stacked, processed with startools and Photoshop cs5

Monday 6 June 2011

ATM: Amaterur teleskoopmakers in Bloemfontein bymekaar

Thinus van der Merwe van ASSA Bloemfontein wys hier hoe `n spieël geslyp moet word by `n inligtingsessie om jou eie teleskoop te bou.

Saturday 4 June 2011

Die "Jet Stream" beïnvloed jou waarnemingsomstandighede!

 Kliek om te vergroot
 Die Suidelike "Jet stream" soos op 4 Junie 2011 besig om oor Suidelike Afrika te beweeg. Tog as jy na die Wolkekaart van Kobus Botha (hieronder) kyk is dit oopgetrek oor Suid-Afrika.  
Kliek om te vergroot

Hoe gaan die "seeing" vanaand by Boyden wees? Waarskynlik onstabiel. Is dit nie `n nfaktor wat ons amateurs nie in gedagte hou as ons observasieaande beplan nie. Agterna kla ons oor die voorwerpe wat rondspring.

Lees gerus die artikel hieronder wat ek op `n webtuiste raak ge-google het.  Onderaan is 'n paar skakels.

Source: Astronomy Club of Asheville
"Seeing" refers to the the amount of "blurring" caused by the earth's atmosphere -- most apparent in a telescope using higher magnifications.  Astronomers refer to this atmospheric turmoil as "bad seeing".  Seeing well at high magnifications is only possible when the air is steady.

Excellent seeing means, at high magnification, you will see fine detail on planets.  In bad seeing, planets might look like they are under a layer of rippling water and show little detail at any magnification, but the view of galaxies is probably undiminished.

Bad seeing is caused by turbulence combined with temperature differences in the atmosphere.  The turbulence may be caused by ground level winds as well as higher level air movements created by the jet stream. When the jet stream is overhead, seeing is generally poor.

Bad seeing can occur during perfectly clear weather.  Often good seeing occurs during poor transparency.  It's because seeing is not very related to the water vapor content (transparency) of the air. 

Skakels







Wednesday 1 June 2011

Deep Space Atlas - Father's day Special

FATHER'S DAY SPECIAL!
Father's Day special of R299 for the Deep Space Atlas for the
month of June. (Usual price R399)
Postage: R45
To order, please use the following email address: wayne.mitchell@penbogroupe.com

For more info about the book visit blog article: Deep Space Atlas

Tuesday 31 May 2011

Kom bou jou eie teleskoop!

 Inligtingsessie:  Kom bou jou eie teleskoop! 

Datum: 4 Junie 2011 (Saterdag)
Tyd:  18:00
Plek: Boyden-sterrewag
Aangebied deur die Bloemfontein Sterrekundevereniging

Thinus van der Merwe,
`n gesoute teleskoopbouer van die vereniging, met `n hele paar teleskope op sy kerfstok, gaan ons meer oor die projek vertel.
  • Hy gaan ook vir ons `n praktiese demonstrasie gee van die stappe om `n spieël te slyp.
Vir wie:  Almal wat belangstel om sy eie teleskoop te bou.  `n Lekker gesinsprojek.
Nee, dit is nie net `n projek vir die manne nie. Mia Zeelie, van die vereniging het vroeër haar eie teleskoop gebou.
Waaroor gaan ons praat?
- Koste van so `n projek.
- Hoe gaan ons die projek aanpak?
- Is dit goedkoper as om `n teleskoop te koop?
-
Hoe maklik is dit om dit self te doen?
- Wat het jy alles nodig om so `n projek aan te pak?
- Waar kry jy al die benodigdhede vir so `n projek?
- Hoe slyp mens self die spieël?
- Het jy duur toerusting nodig om die voetstuk/basis te maak?
- Wie gaan help as jy vashaak?
- Hoe lank gaan die projek neem?
- Is `n selfgemaakte teleskoop beter as `n gekoopte teleskoop?
  • As daar nog vrae is kan jy dit gerus vir ons stuur. e-pos aan: assabfn@gmail.com  Die kundige ouens sal dit Saterdagaand beantwoord.
Besoek ons 2007 webblad toe ons `n soortgelyke projek aangepak het en loer na die teleskope wat gebou is.
Daar is ook `n paar kort videos oor die slyp en bouproses van `n teleskoop.
Ons sal ook van die selfgeboude teleskope by Boyden hê, sodat jy kan sien hoe dit lyk. 
As die weer saamspeel sal ons ook deur `n selfgeboude teleskoop kan kyk.
Die kanse is goed dat jy al so `n teleskoop by Boyden op die platform gesien het.

Laat weet asseblief of jy die geleentheid gaan bywoon.
e-pos aan: assabfn@gmail.com

Monday 30 May 2011

A Reminder: Total eclipse of the Moon (Wednesday June 15, 2011)

 
Date: 27 – 28 October 2004
Time: 02:00 – 04:25Place: Back Yard Observatory, Westdene, Bloemfontein
Equipment:  Canon 10; ISO 400 - 1600; Exposure: 1/250 – ¼  sec; Camera attached to Celestron 11GPS telescope; Focal length: 2800mm. Only first half of eclipse was visible. Neighbours roof and sun interfered with last part.
Technique: Shutter release used to prevent movement. Telescope was in Lunar tracking mode.
Image Processing: Photoshop
 Photographer: Hannes Pieterse

On Wednesday evening, June 15, 2011, the Moon will be in line with the Earth and the Sun, and the shadow from our planet will obscure the Moon, turning it a dramatic orangey-red colour.
This beautiful and rare event is inspiring to watch

Observing 101: Averted Vision

Averted Vision: Getting The Most From What Nature Gave You

Using averted vision means looking slightly off to one side rather than straight on. It exposes the most sensitive part of your eye and lets you see much fainter objects. If you’ve never tried this before, you’ll be amazed at how much more you can see, with or without a telescope.
The Basics
• The retina of your eye has two types of light-detecting cells: rods and cones.
• Cones detect color under well-lit conditions and are densely packed in the fovea, near the center of your retina. Cones help you see color and fine detail, which is why you look directly at objects you want to see well, like books, movies, and faces.
• Rods are mostly away from the center of your retina. You see less detail and no color with the rods, but they are much more sensitive to light.
• The way your eye is structured means you see the faintest objects if you look 8 to 16 degrees off center. The exact angle is a little different for each person.
• This only works if the object you’re looking at is on the nose-ward side of your eye. So look slightly rightward with your right eye and leftward with your left eye. Do the reverse and you’ll expose the blind spot of your eye and you won’t see a thing.

A cross section of the human retina, showing rod and cone cells.
A Deeper Look
• If you’re using both eyes, as with binoculars, looking only sideways makes one eye more sensitive at the expense of the other. The solution? Look up. That uses another rod-rich part of your retina above the fovea.
• With a little practice, averted vision reveals objects 20-40x fainter than direct vision. That’s a huge difference.
• Rods are most sensitive to blue-green light, but your optics nerve and brain are not wired to detect color when only your rod cells are exposed to light. That’s why faint objects appear grayish-white.

The sensitivity of rods and cones to light across the spectrum
Good To Know
The blinking nebula, NGC 6826, is an object that most dramatically demonstrates averted vision. Stare directly at this blue-green planetary nebula and you see only the dim central star. Look slightly to the side and the faint nebula around the star appears suddenly. When you switch from straight on to averted vision, the nebula appears to blink on and off. It’s darned impressive.
Personal View
I usually begin with a short lesson on averted vision when showing faint objects to beginners. When they try it, they usually gasp at the subtle detail that suddenly appears.

Observing 101: Dark Adaptation


Dark Adaptation: “Looking” Your Best

March 14, 2008
To best see faint deep-sky objects like galaxies and nebulae, you have to make sure your eyes are “dark adapted”. Here’s what you need to know.
The Basics
• The human eye evolved to operate in two modes, photopic for seeing in well-lit conditions and scotopic for seeing faint objects in the dark.
• As you learned earlier, your retina has two types of cells, rods and cones. In photopic mode, the cones detect bright light and colors. But in scotopic mode, the rods detect faint light. Both types of cells contain dyes that undergo a chemical change called “bleaching” when hit by light.
• In light-adapted or photopic mode, the dyes in your rods are fully bleached, so they can’t detect faint light… they’re out of action. Turn the lights off and the rods to return to dark-adapted mode, but it takes a long time, about 20-60 minutes. That’s why astronomers get so angry when someone carelessly shines a white light in their eyes… they have to wait a long time to recover their dark-adapted vision.
• Going from a dark to light adapted state happens much faster, in only a few seconds.
A Deeper Look
• Each eye reacts separately to light, so you can keep one eye dark adapted while using your other eye to read star charts and slew your telescope. An eye patch is ideal.
• You can keep unwanted streetlights out of your eyes by throwing a towel over your head when looking through the eyepiece of your scope with your dark adapted eye.
• You often see astronomers using bright red LED flashlights when looking at star maps and gear around the telescope. That’s because red light cannot bleach the dye in the rods if the wavelength is > 620 nanometers. So the chemical structure of the dye in the rods is completely unaffected, while the dye in the cones still enables scotopic vision.
Good To Know
Your body cannot by itself make the dyes for the rods and cones in your retina. It needs an external chemical-beta carotene-to synthesize the dyes. A good source of beta-cartone? Carrots. So carrots really can be good for your eyesight.
Personal View
You can imagine the reaction I get from the police officers who occasionally find me in the local park wearing an eye patch with a towel over my head to block out the nearby street lights. “Really officer, I’m just trying to see the faint structure in M97. Want a carrot?”

Thursday 19 May 2011

The Atmosphere and Observing - A guide to Astronomical seeing.



Introduction
An observer, be they at a mountain top observatory, or in their own back yard must, at all times contend with the Earth’s atmosphere. It is a notoriously unpredictable and limiting factor in obtaining fine views of the Planets, and close binary stars. Many often comment, especially here in the UK that seeing is all too often mediocre on most nights, but what are the factors that contribute to this?. Are there ways and signs, which indicate whether the atmosphere, will be stable or turbulent on a given night?.

What is “seeing”?
So what exactly is atmospheric seeing? - it is high frequency temperature fluctuations of the atmosphere, and the mixing of air “parcels” of different temperatures/densities. This behaviour of the atmosphere is seen at the eyepiece as a blurred, moving, or scintillating image. There are roughly 3 main areas where Atmospheric turbulence occurs. Near ground seeing (0 – 100metres or so.) central troposphere (100m – 2km), and High troposphere (6-12km.) Each area exhibits different characteristics, which are explained in more detail below.