Beauty Cubed

Moon, Mars and Venus

Conjunction of the Moon, Venus and Mars on May 22nd, 2009
Sketch and Details by Carlos E. Hernandez

I was able to view a Waning Crescent Moon (~23 degrees above the eastern horizon), a brilliant Venus (-4.32m,~31* above the eastern horizon) and Mars (1.35m, ~27* above the eastern horizon) over a lavender to bluish-gray clouded horizon. The trio was impressive over the hazy sky.

A digital image produced in Gimp.

Carlos

My Favorite Mars

Mars Map

A Mars Map, representing a complilation of Mars sketches Opposition 2007,2008
Sketches and Details by Kris Smet

In January I posted the sketches I managed to make up to then, later I added 7 more sketches and tried to make a marsmap based on my them. Just when I felt I was getting familiar with the various martian features on the disk, the opposition was rapidly coming to an end. I can’t choose any one sketch as my ‘favourite’ but it would have to be the last one then. It was my first, and ironically also last, view of the sinus sabaeus region of that opposition. Luckily the seeing was good and I was able to make a decent observation. The later sketches are also less crude but have a more soft finish, which i’ve been struggling to do from the beginning.

Mars sketches 2007 2008

Mars sketches Opposition 2007,2008
by Kris Smet

My earlier report from January:

I started observing Mars early in July to make the most of the opposition in December when the planet’s disk reached almost 16“. However the first few sketches may not look like much, I believe making the sketches helped me gain more experience
over the months. Putting the colour of mars on paper was much harder than I thought it would be, I’ve tried a few different colours but kept changing them because I wasn’t completely happy with it. The last sketch in my opinion looks most as how
Mars appears to my eye in the scope. (All sketches were done with my 8” f/5 reflector on equatorial mount btw, I didn’t took the tube from the dobson base until October though.)

All sketches are made outside sitting at the scope, with plain A4 printer-paper on a clipboard on my lap. After the scope is brought back inside I work the sketch out with colours and scan them in on my computer. The only ‘processing’ I (sometimes) do
is adjusting the brightness and sharpness levels a bit to look a bit more eyepiece-like.

If you look very closely you can see the small disappearing south polar cap on the first 5 sketches, after that I couldn’t detect it anymore. During September and the first part of October the north polar hood appeared bluish to me, but it seemed to disappeared and on the 14 October sketch the hood doesn’t show any blue. While Mars was showing me it’s so called ‘boring side’ during September and October (accept 5/10 & 31/10) I had the impression that the area south of mare Sirenum, Cimmerium and Mare Tyrrherium was brighter and more yellow than the desert plains laying south of them. In December I had some very good views of the Syrtis Major region in which I could see some detail. I had to wait until early 2008 to get my first view of the Solis
Lacus region, because whenever this side was facing earth I was clouded out :p

I hope to get more viewing time during January, February and perhaps March to make another ‘collage’ of Mars sketches.)

To Sketch a Sketch for the Sake of Science

Mars

Modified Test Drawing of Mars: 1890
Drawing by Professor Schiaparelli, modified by test administrators

The above sketch was used as part of an experiment in determining the origin of the observation of Martian canals. Excerpts from the article are shown below. The entirety of this interesting and enlightening article can be read at Google Books (see link at the end of this post).


Experiments as to the Actuality of the, “Canals” observed on Mars.
By J. E. Evans and E. Walter Maunder.The experiments described in the following paper were undertaken in order to ascertain whether the impression of a network of fine lines, such as forms what is now known as the “canal system” of Mars, could be produced upon entirely unbiassed observers without those lines having a real objective existence; and, should this prove to be the case, to find out the conditions most favourable for the creation of such an impression. The experiments were made in the following manner. A circular disc, varying according to circumstances from 3.1 to 6.3 inches in diameter, was given to a class of boys to sketch. The boys in the class were usually twenty in number, and were seated at various measured distances from the disc. These distances varied in the extreme from 15 feet up to 62 feet, but more generally from about 17 feet to 38 feet. The boys were all supplied with a piece of drawing-paper upon which a circle 3 inches in diameter had been described, and were instructed to fill in that circle with all the details which they could perceive upon the disc. No hint was given them that they ought to see lines or dots or any other form of marking ; they were simply urged to draw all that they could see and be sure of, each for himself, without noting what his neighbours were drawing….

….The boys employed in the experiments were from the Royal Hospital School, Greenwich. Their ages ranged from twelve to fourteen for the most part; a few were either a little older or a little younger than these ages. All of them were wholly and entirely ignorant of the appearance of Mars in the telescope, and of the discussions which have taken place as to the markings on his surface. They were simply shown, what was to them, an odd-looking figure, and were told to reproduce it as well as they could. The first series of experiments was made on 1902 July 1, the last on 1903 May 22, the great majority having been made in the spring of the present year….

….Experiments 8 and 9.—Drawing 6.25 inches based upon one by Professor Schiaparelli made 1890 May 16 (La Plancte Mars, p. 474). In this experiment none of the canals shown by Professor Schiaparelli were inserted, but a number of small irregular markings were inserted at haphazard. River-like marks were drawn flowing into Dawes’ Forked Bay and the smaller marking of the same character which Schiaparelli has represented some 30° from it at the mouth of the Phison. The region of Meroe Island was put in in half-tone….

….It appears to us in reviewing the entire series of the experiments that it is impossible to escape the conclusion that markings having all the characteristics of the canals of Mars can be seen by perfectly unbiassed and keen-sighted observers upon objects where no marking of such a character actually exists. They are in a sense truly “seen,” not imagined, because they are the natural rendering by the eye of real markings of a different character….

….Generally speaking, the best draughtsmen, that is to say, those who most truthfully represented the salient features of the drawing, also showed the greatest numbers of canals. It is also worth note that on the whole the agreement as to the canals was greater than the agreement as to the broad features of the original drawing….

….Our conclusion from the entire experiment is that the canals of Mars may in some cases be, as Mr. Green suggested, the boundaries of tones or shadings, but that in the majority of cases they are simply the integration by the eye of minute details too small to be separately and distinctly defined. It would not therefore be in the least correct to say that the numerous observers who have drawn canals on Mars during the last twenty-five years have drawn what they did not see. On the contrary they have drawn, and drawn truthfully, that which they saw; yet, for all that, the canals which they have drawn have no more objective existence than those which our Greenwich boys imagined they saw on the drawings submitted to them.

It seems a thousand pities that all those magnificent theories of human habitation, canal construction, planetary crystallisation, and the like are based upon lines which our experiments compel us to declare non-existent; but with the planet Mars still left, and the imagination unimpaired, there remains hope that a new theory no less attractive may yet be developed, and on a basis more solid than “mere seeming.”


Published in the Monthly Notices of the Royal Astronomical Society, Vol. LXIII, 1903, Pages 488-499 available at Google Books.

Pickering’s Martian Penmanship

Mars

Mars: May – July, 1892
Sketch by Professor William Pickering

This series of Martian sketches was prepared by William Pickering in 1892. They were printed the article, “The Lowell Observatory, In Arizona,” by Edward S. Holden in The Publications of the Astronomical Society of the Pacific, Volume VI, 1894, pages 160-170 at Google Books. Mr. Holden’s article featured Pickerings drawings along with comparison drawings made at the Lick observatory during the same Martian apparition. Holden expressed considerable concern over the conclusions Pickering and Lowell published regarding their observations of Mars:

The very essence of the scientific habit of mind is conscientious caution; and this is especially necessary in referring to matters in which the whole intelligent world is interested—as the condition of the planet Mars, for example. I may take as an example the telegrams regarding Mars sent by cable from South America in 1892 by Professor WILLIAM PICKERING, who is to be the chief observer at the Lowell Observatory in Arizona. I quote two out of many such telegrams:NEW YORK, October 6, 1892. – The Herald correspondent at Valparaiso cables as follows: Professor PICKERING of the Harvard Branch Observatory at Arequipa says that he discovered forty small lakes in Mars.How does he know the dark markings are lakes? Why does he not simply call them dark spots? And is he sure there are forty?

NEW YORK, September 2, 1892. – Professor PICKERING of Harvard College sends the following to the Herald from Arequipa, Peru:

‘Mars has two mountain ranges near the south pole. Melted snow has collected between them before flowing northward. In the equatorial mountain range, to the north of the gray regions, snow fell on the two summits on August 5 and melted on August 7. I have seen eleven lakes near Solis Lacus varying in area from 80 by 100 miles to 40 by 40 miles. Branching dark lines connect them with two dark areas like seas, but not blue. There has been much trouble, since snow melted, in the Arean clouds. These clouds are not white, but yellowish and partly transparent. They now seem to be breaking up, but they hang densely on the south side of the mountain range. The northern green spot has been photographed. Many of SCHIAPARELLI’S canals have been seen single.”*

*Several of these canals were seen not only single but double at Mount Hamilton, do not know that they were so seen in Peru.

How is it known that there are two polar mountain ranges? How does he know that the flow will be northwards? And an equatorial range? Are not the gray regions so extensive that the description is, to say the least, indefinite? What is the evidence of “trouble” in the clouds? Is it certain that no clouds on Mars are white? How about the clouds “twenty miles high” reported by Professor PICKERING? Were they not white?

These and similar telegrams from South America regarding the happenings on Mars in the year 1892 were received by the astronomers at the LICK Observatory with a kind of amazement.

That’s No Moon…

Mars - Cimmerium and Elysium regions

Mars – Cimmerium and Elysium Regions
Sketch and Commentary By Carlos E. Hernandez

I made a pair of observations on December 28, 2007 using my 9-inch (23-cm) F/13.5 Maksutov-Cassegrain. I noted a significant amount of detail over the Mare Cimmerium and Elysium regions of Mars. I welcome any comments on my observations.

Date (U.T.): December 28, 2007
Time (U.T.): 01:20 (left image, IL) and 01:50 (right image, Wratten 38A)
CM: 227.5*W (left image) and 234.9*W (right image)
Ls: 009.0* (Early Northern Spring/Southern Autumn)
De: 0.7* North, p 1.00, Dia. 15.7″
Instrument: 9-inch (23-cm) F/13.5 Maksutov-Cassegrain
Magnification: 163x, 273x, and 359x
Seeing (1-10): 6-7, Antoniadi (I-V): II
Transparency (1-6): 5

Notes:
01:20 U.T. (Left image, CM 227.5*W, IL): The South Polar Region (SPR) appears obscured by a very bright to extremely bright (8-9/10). Mare Australe appears dusky to shaded (4-6/10) north of the haze. Electris, Eridania, and Ausonia appear to be obscured by a bright to very bright (7-8/10) haze. Mare Cimmerium appears dark to dusky (3-4/10) and mottled. The northern border of Mare Cimmerium contains projections (Laestrygonum Sinus, Cyclopum Sinus, and Cerberi Sinus, preceding to following). “Valhalla” was visible north of Mare Cimmerium as a dusky (4/10) band. Hesperia appears as a bright (7/10) diagonal strip between Mare Cimmerium and Mare Tyrrhenum. Mare Tyrrhenum appears dark to shaded (partially obscured by a very bright (8/10) morning limb haze (MLH). Zephyria, Aeolis, Aethiopis, and Aetheria appears bright (7/10). Amazonis and Arcadia appear dusky to shaded (4-6/10) and mottled. A very bright (8/10) orographic cloud is visible over Olympus Mons over the north-preceding (evening) limb. Trivium Charontis, Phlegra, and Azania appear dark to dull (3-5/10). The Propontis Complex (Propontis I and II, Castorius Lacus, and Euxinus Lacus) appears dark to dusky (3-4/10). Elysium appears bright with a very bright (8/10) cloud over it’s north-preceding sector. Panchaia appears bright (7/10) and Lemuria (dusky (4/10). The Hyblaeus Extension appears dark to dull (3-5/10) following Elysium. Syrtis Major appears to be obscured the very bright (8/10) MLH. The North Polar Cap (NPC) appears brilliant (10/10) along the northern limb.

01:50 U.T. (Right image, CM 234.9*W, Wratten 38A (Blue) filter): Mare Cimmerium appears dusky (4/10). The southern limb, preceding (evening) limb, northern limb, and following (morning) limb appear very bright (8/10). A very bright (8/10) orographic cloud appear over Olympus Mons over the preceding limb. A very bright (8/10) cloud appears over Elysium.

The best of luck in your own observations of Mars.

Regards,
Carlos E. Hernandez

Comet, Moon, and Mars

Comet, Moon and Mars

Comet 17/P Holmes, the Moon and Mars
By Carlos Hernandez

I was treated to a rare (at least these days in South Florida with our cloudy weather and tropical storms nearby) clearing of the heavens over the northern sky on October 30, 2007 (07:20 U.T.). I was able to view Comet Holmes (17P) in Perseus (~3.8 degrees from Alpha Persei (Mirfak, 1.78 m)) and I was impressed with the brightness of this interloper (Comet Holmes is currently estimated at magnitude 2.0). Capella (0.06 m) in Auriga was shining brightly nearby. The Waning Gibbous Moon (19.5 days old) was visible towards the east within Gemini close to a brilliant reddish-orange Mars (-0.58 m). The view was facing south and looking upwards (North at top and east to the left).

A digital image produced in Corel Painter X.

The best of luck in your own observations of this interesting comet.

Carlos