From William SHEEHAN
@. . . . . . . . . Hope you will forgive the
intrusion -- I know you are very busy, but I wanted to pass along my greetings
and to thank you for the interest in the Edom flare top which Tom Dobbins and I
were able to call the advance attention of the astronomical world, and which
Tom and his team of observers were able to verify successfully from the Florida
Keys. It was also a great thrill to see
the observations of Saheki and other leading Japanese observers confirmed
-- Tom has mentioned that you even had a
suspicion of a brightening at
I have the
greatest respect and admiration for your wonderful work on Mars and that of
your colleagues at the OAA. It will be a
privilege if we have the opportunity to meet up sometime.
Meanwhile,
I am awaiting word of your observations of
Incidentally, I would be very happy to send you a copy of my Mars books
– “The
Planet Mars”, published by U of Arizona Press, 1996, and
“Mars:
the Lure of the Red Planet” (with Stephen James
O'Meara), just published, in the event they may be of interest to you and your
colleagues. They do not contain any
information about the
Kind
regards,
(
@. . .
. . . . . . . Dear Masatsugu,
I sent Tom's images of
Kind regards,
Bill
------------------------------------------
Well! Isn't that something? Thanks for sending those pictures --
they
certainly are remarkable.
To begin with, I note that the "flash" is clearly an unresolved
instrumental point-spread function; you can see it's a little broader
on the frame where the seeing is a little fuzzier. So it's clearly
something on Mars and not some kind of instrumental artifact.
From the contrasty images, I assume these were taken at some fairly
long wavelength in the deep red, though the lack of limb-darkening is
surprising -- can you supply information about the passband used? And
what was the phase angle? What kind of processing has been applied to
the image?
The bright spot seems brighter than anything else on Mars, but not by
more than a factor of 2. So the average brightness of the PSF is about
that of a light gray (say, "white") piece of paper the same
size. As
this is roughly 10^5 times dimmer than an image of the Sun, we can
assume that only something like 10^(-5) of the area is filled by
reflecting objects if they reflect like a perfect mirror. If they are
ice crystals or mica flakes with a reflection on the order of 10%, then
about 0.01% of the area of the PSF is filled with them. The PSF is
about 1/20 of the diameter of the planet, so if all the reflectors are
together in a coherent area (unlikely) this area is about 1/20 x 1/100
of the diameter of Mars across, or 1/2000 of 6800 km, or about 3 or 4
km across (assuming ice or mica). If the reflectors are more spread
out, the peculiar area on Mars is somewhat larger, but of course no
larger than the projected PSF of about 340 km diameter.
These sizes sound about like the diameter of a medium-sized impact
crater; it may turn out to be a funny-looking crater floor?
In the old days we would gladly have read this as the leaves of some
Martian heliotrope-field blowing in the wind; but such an
interpretation today seems highly unlikely. The most pressing problem
is to understand the short timescale -- much less than the time
required for the solar image to pass across a stationary reflecting
surface. So salt flats with well-developed crystal faces, and frost on
the ground, are not possible interpretations. I would be inclined to
favor some temporary alignment of crystals suspended in the air; but
then the problem is to tilt them synchronously over such a large area,
to make the "flash" wink on and off coherently.
Perhaps a Martian geyser is erupting here, and its plume is turning to
ice crystals in a few seconds. But then it's hard to get the crystals
to grow large enough to have well-developed faces, needed to give the
desired directionality to the reflection. If it were simply a steam
plume from geothermal -- er, areothermal -- activity, then how do we
get it to cover such a large area (now we are talking about a temporary
white spot some 100 km or more across) and yet to disappear again in a
minute or so?
Might we be dealing with a dust cloud stirred by a major Marsquake?
This might account for the timescale: seismic waves travel a few
km/sec, so in 10 sec or se we can easily shake an area large enough to
make the bright spot. If the dust is merely stirred a few meters into
the air, it can fall out again on a similar time scale. Ask the
geologists if the terrain suggest earthquake country.
My own inclination is to favor some such widespread brightening of the
surface, rather than a localized glint of Sun on moving surfaces. But if
the brightening is mild and spread over many tens or a few hundred km,
a mechanism is needed to synchronize the display over that region, and I
think the speed of sound on Mars (about 200 m/sec) is a bit slow to
accomplish this with an atmospheric driver. If the phenomenon is
basically atmospheric, then we need something that can appear and
disappear in a few tens of seconds at most. A steam vent doesn't look
promising at first glance, but maybe there is a way to make it serve.
A very remote possibility is a specular reflection from something in
orbit around Mars. The problem then is that it has to be over a
kilometer across, and tumbling enough to account for the temporal
modulation. But then why hadn't it been noticed before, and why hadn't
the physical librations been damped out?
You certainly have a puzzler here!
-- Andy
(
@. . . . . . . . . Wonderful to have your kind
comments and to read of your interest in my previous book, “The Planet Mars”. It shall be a signal honor for me to send you
copies of both of these books, with my added inscriptions. It would be a tremendous satisfaction for me.
I have
reread your comments about the 1954 observations and apologize for not
comprehending them fully at first -- they are perfectly clear as you stated
them. I am gratified to learn of your
having observed the planet as early as July 1954.
I returned
to the comments I had made about Herschel's Mars observations. He made the
observations of Mars in 1777 at Datchet, before he moved to
Herschel's
observation on this occasion was made well before opposition.
As for your
other points. I do think the "blue
clearing" is really little more than an opposition effect. E. C. Pickering was the older brother of W.
H. Pickering, director of the Harvard College Observatory for many years and a
leading spectroscopic student of the stars.
I shall be gratified to try to answer any other questions you may wish
to put to me.
Once again,
my heartfelt salutations! -- I am honored to be in communication with one of
the greatest of living Mars observers, whom I have long admired from afar. I am impressed also by the high level of
accomplishment of Japanese observers of Mars generally. Perhaps oneday I shall have reason to revise
one or the other of the Mars books and include a fuller account of your
important work -- ideally after having a chance to meet and discuss Mars with
you in Okinawa!
The books
go out first thing tomorrow!
Your
fellow MARTIAN,
(
@. . . . . . . . . . The books went out
yesterday. Meanwhile, thanks much for
the news of the recent dust-storm. I'll
begin to monitor.
Regarding
the flashes on Mars, you may find this of interest. A comment from Walter Haas about Percival
Lowell logging thousands of hours and not seeing anything jogged my memory. Now
I'm sure you will find this of compelling interest, and we ought to mention it
in our paper. Percival Lowell, in *Mars*,
pp. 86-87: "An interesting phenomenon occurred in the cap on
(
@. . . . . . . . . Won't detain you long -- I'm sure
you're unbearably busy. Have been
following your reports of the spreading dust clouds now covering the hemisphere
of Mars visible from the Orient. On July 5, I looked with my 12 1/2 cm and 30
cm Schmidt- Cassegrains at
The
Syrtis Major was clearly visible; the north extension was quite dark, the rest
faded. The region extending from
Hard to say
-- but even with the naked-eye I have thought the planet appears to be more
yellow than it seemed in early June before the dust began to make its appearance.
Hope to make
more observations tonight.
(
@ . . . . . . . .We continue to follow the dust
storms on the Occidental hemisphere of the planet. Today I wrote up (for the Astronomical
Society of the Pacific's journal *Mercury*) something on the Martian flare observations. Please comment if you would. Best,
(
@. . . . . . . I have made some changes to the
article (The Flare from Mars Seen Round
the World) in the light of your fascinating and kindly response. I know you are highly pressed at the moment
-- but I wanted to thank you at once.
Perhaps I shall one day visit
Best wishes,
(
Bill SHEEHAN (
MN