1st June 2025

The planet is now remote, well under 6 arcseconds in diameter, and observable only in the evening twilight. However, daily coverage continues by those sufficiently equipped to do so (and not having awkwardly-placed trees or buildings).

No changes in albedo features have been seen. The planet continues to show the usual seasonal behaviour. Dust activity has not been detected since the last blog entry.

The north polar cap is now very small. A very recent image by Nick Haigh (May 28) shows a seasonal rift in the N. polar cap (with a possible brighter patch on the following side). It also shows the continuing equatorial cloud belt, and the summits of Olympus Mons and the Tharsis Montes poking through the extensive white morning cloud. Another view by Clyde Foster (May 26) shows similar effects. The exceptionally dark patch near the cap in these images is Hyperboreus Lacus, a feature of this time of the martian year.

The equatorial cloud belt continues to cause a bluish or greenish tint to the Syrtis Major, especially when near the edge of the disk, and this effect was again reported by Frank Melillo on May 18 and 20. In blue light the Syrtis is invisible even at the CM. David Basey had a similar view on May 15, while Paul Abel observing visually on May 12 caught the bluish tint over the morning Syrtis.

The frost at Hellas mentioned in the last blog entry continues to be visible, and it was confirmed visually by Abel, Stanislas Macsymowicz, Andy Wilson and the Director. Here is an image by Mark Lonsdale (May 25) that shows it, and also confirms that the Olympia region had become seasonally detached from the N. polar cap.

Evening cloud over Olympus Mons and Tharsis Montes continued to be visible. For example, Peter Tickner caught the Olympus Mons cloud near the evening limb on May 19. On the 16th he imaged some light afternoon cloud over Elysium too. And here is an image by Martin Lewis (May 22) which in addition to showing orographic clouds, portrays the small dark dot of Propontis clearly on the NE side of Elysium, following the CM. His image also shows the detached Olympia.

I have received further images of the terminator projection mentioned in an earlier blog post, from Nick Haigh, who caught it on February 27/28.

All observations are welcome, and will continue to be acknowledged. If enough data are received, this blog will continue. We may not be able to record as much detail now, but we wish to monitor as much of the current martian year as we possibly can in order to time the various expected phenomena. By the start of August, the planet’s declination will soon favour the southern hemisphere, but I hope that UK observers can continue for at least a little into June.

1st May 2025

A short update this time. The tiny martian disk has now slipped below 7 arcseconds in diameter, and several observers consequently have now stopped their work for the season. However, daily coverage of most longitudes continues, and to illustrate this here are some images and drawings from the same date, April 17, from C.Foster (Namibia), C.Nuttall (UK), G.Walker (USA) and M.Adachi (Japan).

The band of orange-coloured atmospheric dust over the cap, mentioned in the last post, continued to be visible for some time. For example, images by M.R.Lewis (UK) on April 10 (posted here) and by G.Walker (USA) on April 17 show it clearly. The dust appeared close to the position where the polar area known as Olympia detaches from the rest of the cap.

The seasonal separation of Olympia from the N. polar cap has been observed. Images taken on April 19 (Ls = 73 degrees) onwards by T.Akutsu (Philippines) (and his image of April 22 is posted here) may have been the first to show it clearly on the evening side, and many subsequent images by others have confirmed it. It may have been caught on the morning side a little earlier, though the situation at that time was confused by the presence of the aforementioned streak of dust over the cap. With the current viewing geometry it is easier to spot on the evening side, where the gap between Olympia and the cap is widened by perspective. The seasonal date is typical. For example in 2010 separation was complete by Ls = 74 degrees.

The summits of the Tharsis Montes and Olympus Mons continued to show up through morning cloud. See the images by P.Tickner (UK) on April 19 for an example.

The equatorial cloud belt (or band) has continued to be strongly marked in the images, though not appearing equally intense all around the planet. It is also apparent visually. On April 24 Abel and the Director saw it under CM = 69 degrees. It was brighter in the morning and evening where it joined diurnal clouds, and around Ophir-Candor.

The seasonal brightening of Hellas, due to ground frost deposition, ought to be visible soon. The latest images from April 24 show it light in blue light, paler than the N. polar cap, but not yet bright in red. Akutsu’s April 22 series (see earlier) shows its current wavelength dependence.

I am hoping we shall be able to continue our daily patrol for as long as possible.

April 10th 2025

As Mars rapidly diminishes in size, I am starting with some earlier images by P.W.Maxson (USA) to remind us of the near-opposition period.

Moving ahead in time, an image on Feb 27 by W.J.Leatherbarrow (UK) shows the planet beautifully defined at the moment of our last update. But at the time of writing (April 7), the disk diameter has recently dipped below 8 arcseconds. To partially compensate, we have at least had an exceptionally long run of clear evenings in the UK, and sometimes even some decent seeing. As always, this update is not intended to be a complete analysis.

The south polar hood is now more prominent. Hellas is quite brightened by its presence but is not yet brilliantly white; so, white clouds rather than frost are present there. The equatorial cloud belt (ECB) has been well seen, and when cutting across the Syrtis Major has imparted to it an obvious blue tint. The same tint is imparted to northern Mare Tyrrhenum. Although obvious visually, it is not evident in all the images received, which suggests a lack of proper colour balance. The Mar 7 image by S.Ito (Japan) nicely shows the enhanced brightness along the equator (and the enhanced polar hood) in blue light., while the evening clouds drawn by C.Nuttall (UK) for Mar 14 are typical.

The orographic clouds over Elysium Mons, Olympus Mons, Alba Patera and the Tharsis Montes can still be caught right at the evening limb, but there it is only early afternoon in terms of local time, so those clouds have not yet displayed the brightness that they would do at the evening terminator. See M.R.Lewis’s (UK) Mar 3 image and O.Inoue’s (Japan) of Mar 31.

The NPC continues to shrink, and as of late no detail has been seen within it. But do please look for the detachment of Olympia soon, due to the development of the dark Rima Borealis rift.

There were no surface feature changes, but there has been a little dust activity. The image of M.R.Lewis for Mar 3 (and another of his for Mar 9 at the same spot) suggests some atmospheric activity at the cap edge. On Mar 20 D.A.Peach (UK) imaged two small bright yellow dust clouds at the edge of the cap near Mare Acidalium. His image is posted here. On the same date P.G.Abel (UK) visually saw that there was a light strip between N. Mare Acidalium and the cap edge, and wrote: “Sometimes in the best moments of seeing the brightness took on an orange tone like those of dust clouds.” See his drawing posted here. Abel, F.J.Melillo (USA) and the Director commented that central and southern Mare Acidalium sometimes looked a little fainter than usual, though this must have been due to the slight veiling effect by the ECB (mentioned above, and now close to its seasonal maximum thickness), that crosses part of Mare Acidalium.

The often extensive morning cloud continued to offer the opportunity of catching the summits of the Montes poking through it, and so looking dark by contrast. Despite the small disk the Director was pleased to catch this effect again on Mar 18 (410 mm DK Cass., x410). An image for Mar 22 by G.Walker (USA) is posted. A similar UK view on Mar 19 is provided by N.J.Haigh. In passing, looking at such images forcibly reminds the writer of the observation by J.E.Mellish, around the time of WW1, when with the Yerkes 40-inch OG he claimed to have seen ‘craters’. Could this be what he actually saw? Such an eyepiece view would have been striking and suggestive with a large aperture. But visual observers never explicitly saw this effect before the 1990s, for it requires a large phase defect (and hence a small disk) together with seasonal morning cloud, and it was only rarely suggested in the old photos. (Was it another instance of the “Elephant in the Room’? Something the old observers obviously saw, but didn’t want to see.)

Massimo Giuntoli kindly drew my attention to Italian observations of another terminator projection, this time by P.De Gregorio, V.Mirabella and R.Sedrani for Feb 20-23. With the CM around 300 degrees and hence the Syrtis Major central, a detached cloud is visible near the equator in the longitude of Aram (Thymiamata), just W. of Meridiani Sinus. I have uploaded the results by Mirabella for Feb 23, which include a suitably brightened strip of sequential images. (I have edited out and rearranged parts of the image to keep it to 800 pixels wide.)

A number of new observers brings the total to 88. Can we make it 100? We continue to maintain a round the clock Marswatch, with no days missed.

I will make at least one more update to this blog later, so keep observing and sending your results please. Good observing!

27th February 2025

This latest post offers a very incomplete summary of the main points of interest in the recent observations up to and including February 22.

Since opposition on Jan 16 the British weather has been rather variable, and often cloudy. Early February initially looked promising, but most British observers then endured a long cloudy period of more than a fortnight after Feb 6, which only now may be ending. But worldwide coverage by 79 observers (and our Far Eastern observers have been particularly energetic) ensured that no dates were missed. See the updated list on the main page. (And as usual, I have taken images and drawings from past and previous contributors from a variety of websites, but NOT from individual BAA members’ pages. Those members must SEND me their images to me direct if they are to be included!)

I show some images by two new Section members first: David Brett (notice the evening orographic cloud over Elysium Mons) and Ron Palgrave (Solis Lacus remains large, and the Phasis streak and the little dark spot Gallinaria Silva are well seen following it).

The Director on Jan 20 noticed the blueness of the Syrtis Major upon the morning terminator. Thin cloud surrounded it, and dimmed it slightly. By this time the equatorial cloud belt had thickened. A month or so later on Feb 22 (Ls = 48) the blue scattering effect was perhaps stronger, due to the completion of the ECB after about Ls = 45. Images by Mike Karakas in blue light (for example, Jan 23, Ls = 34) show an example of the as yet incomplete ECB.

I would encourage all imagers to actually look through the eyepiece. In several cases not enough emphasis is being given to the blue channel or to the blue filter in RGB combinations, and the colour balance is unrealistic. At this season, white clouds in the morning and evening are common, but not all observers are recording them.

The wavelength-dependence of the white diurnal clouds is nicely shown by C.Pellier on Feb 1. He adds: “I’m adding a simulation to show where the ring of 6 white patches locate on the surface. The most northerly one corresponds to Alba Patera and the weakest one [just to the south] corresponds to a small dome.” See his image below.

Observers should now be looking along the terminator for any high-altitude clouds that lie beyond it. On Feb 16 Tom Williams took just such an image (which I have annotated).

Once the morning terminator is displayed to advantage after opposition, it is always exciting to be able to catch the summits of the Tharsis Montes as dark spots poking through the surrounding morning white cloud. Without having seen images of the effect this year so far, the Director made such an observation on Feb 5. And an image showing this effect by Mike Hood for Feb 18 is shown here.

We must not ignore the far southern latitudes. Here, patches of white cloud are seen in certain locations. Argyre was mentioned in earlier posts. These isolated patches will later merge to form the S. polar hood. With Hellas just past the CM on Feb 17, the Director noticed white cloud along the S. limb, but even when viewed with a blue filter it hardly impinged upon the south of the basin. And of the other visual observers, David Graham on Jan 18 noted a wide bright area (Eridania and Ausonia) along the S. limb under CML = 222-232. See his drawings below. The Director found Ausonia very bright and conspicuous on the evening side on Feb 22.

Until recently, some observers continued to find traces of a warm tint over the NPC upon their images, due to ongoing minor dust storms and dust fallout. A fine image by Martin Lewis for Jan 15 is shown here: note the thin vertical streak of dust upon the cap near the CM. But this month, activity has been much reduced. The cap too, is considerably reduced in size. Next, observers should watch out for the seasonal separation of Olympia.

In January, Mars was occulted by the Moon. Efrain Morales in Puerto Rico captured the diminutive disk of Mars near the Moon on Jan 14, and for once I will allow north to be uppermost. I noticed that several observers, including Ethan Chappel in Texas, USA, obtained images of an actual occultation.

On Feb 9 observers in the north of Scotland had a chance to see a grazing lunar occultation of Mars, or a full occultation further north. Only Callum Potter (Rousay, Orkney, 59.17 N, 3.06 W) was successful in seeing and filming both ingress and egress with his Seestar S50 (50 mm f/5 OG). His collage is shown here. And Paula Wirtanen in Helsinki, Finland, also succeeded with good images and videos of the event, and one of her stills is appended.

In my experience it is very unusual for a planet to be occulted by the Moon in two successive months. In fact, I can’t actually recall such an instance. Can anyone comment upon this?

Finally, if anyone tried to telephone me in early February they will not have succeeded, as in renewing my contract with BT, the company instead unhelpfully cut off the phone for 16 days. Perhaps this was only to be expected: that, after all, is modern service for you!

2025 January 20th

In the UK, the period around New Year and for nearly a fortnight afterwards was bitterly cold, with noon temperatures often staying a little below zero, and with thick frost upon lawns and foliage. Remaining for very long in the observatory always seemed to be an heroic performance. After a few cloudy days, the temperature has become more bearable. Nonetheless, some fine work has been done. This post includes data submitted up to the day of opposition (January 16).

I am posting a number of results, this time concentrating more upon observations made in the UK and Europe, and have included several from different observers for January 9-10, enabling some comparison of processing methods.

There have continued to be a number of small dust events at the edge of the cap. For example, Robert Stuart has sent me an image for January 15 where a small notch in the cap is shown on the morning side when the Syrtis Major was at the meridian. Others have confirmed this.

In the last few days the Director was struck by the slight blue tint in the Syrtis Major, glimpsed with the marking at the CM on the 15th, but more strikingly visible at the evening terminator days earlier. This coloration is due to the scattering of blue light by the thin cloud which populates the martian equator at this season (though the equatorial cloud belt is not yet complete before around Ls = 45). This effect has been shown by some images, and it has also been noticed over parts of Mare Acidalium with the marking near the morning limb. Paul Abel also remarked upon this. High resolution images have shown a small white evening cloud in the mid-latitude of the Syrtis. The orographic clouds mentioned last time are very prominent. Visually the Director noticed that the dark spot Nodus Alcyonius is still rather small and difficult to see. Will it disappear entirely, as it has in the past? And will Nepenthes ever reappear?

Tom Wiliams has submitted a remarkable video from January 3 which appears to show the shadows of evening white clouds (over Sinus Meridiani) as they rotate and reach the terminator. We have caught the long shadow of the Arsia Mons banner cloud at the appropriate season in the past, but imaging the shadows of the more usual evening equatorial clouds is (I think) a first in groundbased astronomy.

T.Akutsu imaged the martian moons on the date of opposition.

I find that my btinternet address sometimes blocks large group mailings. If you have sent something and have not had a reaction from me, please check! And if you are a new observer posting at the BAA website, please contact me directly by email in order to join the Section.

Now a final word about filenames. Whatever filename you assign to your image, and whatever its orientation, it will normally be archived by me SOUTH UPPERMOST in the following style, ending with the observer’s initials, like: 2025-01-15-2300UT-RJM. I allow variants like m20250115_2300_rjm, and so on, provided that the observer is consistent. But variants like 150125-RJM or 15Jan2025_rjm are NOT permitted. Each observer is assigned their own folder of observations in my filing system, for each apparition, and I need their images to appear in chronological order whenever it is opened. You may wish to add subdivisions of a minute of time, or the initial of any filter used before the final initials. If you want to tell me the camera or telescope or observing location or observing conditions it must all be written upon the image, or sent in an email (once per apparition will do), but not added to the filename.