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Regards
Michael
Yes, I'm aware of this. Of course, I will keep this map scientifically...t00fri wrote:I suppose you are aware of the high-quality and scientifically accurate previous renderings of Phobos.
My Intention is to make the appearance of Phobos a bit more realistic. The current one (in Celestia) looks something strange; a bit like a drawing draft. And the other available map from DLR more as a "limit of knowledge"-map (imho).t00fri wrote:What are the specific improvements over existing results that you are addressing in your ongoing project?
MiR wrote:Fridger,Yes, I'm aware of this. Of course, I will keep this map scientifically...t00fri wrote:I suppose you are aware of the high-quality and scientifically accurate previous renderings of Phobos.My Intention is to make the appearance of Phobos a bit more realistic. The current one (in Celestia) looks something strange; a bit like a drawing draft. And the other available map from DLR more as a "limit of knowledge"-map (imho).t00fri wrote:What are the specific improvements over existing results that you are addressing in your ongoing project?
I'm using both for this work, but there are some differences between these maps(?)
It's a lot of work. Because I try to realize this job as pedantically and meticulously as possible.
The project is still in a start-up phase. From time to time I will publish here the progress of the Phobos map.
And a supervising look on this work by an expert couldn't harm...
Your competent critics and suggestions are always welcome.
I appreciate your work here very much.![]()
Regards
Michael
A very well done model (low- and highpoly) by John Van Vliet is available here:Mynameislol wrote:Your texture is accurate enough, it's the model that is inaccurate. Once again, great work!
Probably you overestimate me. I'm not a very important person here.t00fri wrote:So let me ask again: What specifically are you trying to improve?
I really do not know what's to do with the contents of this file? Is this Phobos? With texture?t00fri wrote: My final result can also be downloaded from thread 2):
http://www.celestialmatters.org/users/t ... os_1.3.zip
Thanks for the links. At the moment I make a short pause; I have to prepare a big presentation for Monday (Very important for my job).t00fri wrote:Let me refer you to some most detailed threads over at our CelestialMatters site as to my work on Phobos quite a while ago. John made also a number of contributions there.
1) Import Scientific Shape Models to CMOD without Blender!
http://forum.celestialmatters.org/viewtopic.php?t=337
In the second thread I have entirely solved the polar pinch problem!
2) Fighting the Polar Pinch (ascii CMOD shape models)
http://forum.celestialmatters.org/viewtopic.php?t=339
The third thread about Phobos is a "photoshooting" with some neat images based on my
Phobos rendering!
3) Fun with my 4k colored Phobos
http://forum.celestialmatters.org/viewtopic.php?t=333
MiR wrote:Fridger,
your model of the Mars moon Phobos is simply fantastic
Probably you overestimate me. I'm not a very important person here.t00fri wrote:So let me ask again: What specifically are you trying to improve?
And as a newbie it was not quite clear to me - at least since I've read the "About Us" part - if people like me are welcome there.
t00fri wrote: My final result can also be downloaded from thread 2):
http://www.celestialmatters.org/users/t ... os_1.3.zip
I really do not know what's to do with the contents of this file? Is this Phobos? With texture?
I knew about John Van Vliet's phobos. But i noticed the model you where using was the standard, as you just told me.MiR wrote:Mynameislol,A very well done model (low- and highpoly) by John Van Vliet is available here:Mynameislol wrote:Your texture is accurate enough, it's the model that is inaccurate. Once again, great work!
http://www.celestiamotherlode.net/catalog/marsmoons.php
I use the standard model (and a minimal configuration) for rendering tests. (Celestia starts faster)
Thanks again for your interest!
Regards
Michael
john Van Vliet wrote:i do not think soBut i noticed the model you where using was the standard, as you just told me.
the default svn "phobos.cmob" is 145.2 KB
the mesh in the Phobos 1.3 zip is 738.2 KB
t00fri wrote:All interested CM users are welcome, of course. Unlike the Motherlode, we have however imposed serious restrictions about submitted contributions.
This is one of the reasons that i do not have all that many posts there
i tend to the "artistic" side of things
MiR wrote:Here I go now...
I am still unsure which one of the available Phobos-map is the best...?![]()
Because they are all different...
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Code: Select all
PDS_VERSION_ID = PDS3
RECORD_TYPE = "FIXED_LENGTH"
RECORD_BYTES = 32
FILE_RECORDS = 16471
^TABLE = "M1PHOBOS.TAB"
DATA_SET_ID = "EAR-A-5-DDR-SHAPE-MODELS-V2.1"
PRODUCT_NAME = "M1 PHOBOS SHAPE MODEL"
PRODUCT_ID = "SHAPE-M1PHOBOS-200202"
INSTRUMENT_HOST_NAME = {"VIKING ORBITER 1", "VIKING ORBITER 2"}
INSTRUMENT_NAME = {"VISUAL IMAGING SUBSYSTEM CAMERA A",
"VISUAL IMAGING SUBSYSTEM CAMERA B"}
TARGET_NAME = "M1 PHOBOS"
START_TIME = 1976-06-22 /* Viking Orbiter Mission Dates */
STOP_TIME = 1980-07-30
PRODUCT_CREATION_TIME = 2000-06-01 /* Peer Review Date */
RECORD_FORMAT = "3(2X,F8.4)"
OBJECT = TABLE
ROWS = 16471
ROW_BYTES = 32
INTERCHANGE_FORMAT = "ASCII"
COLUMNS = 3
DESCRIPTION = "Numerical shape model of M1 Phobos, derived
from Viking orbiter images with some checks with Mariner 9 and
Phobos 2 data. The model has uncertainties of a few hundred meters
in places, especially between 35 and 190 degrees longitude. This
shape model consists of a grid with points every 2 degrees in
latitude and longitude, with a radius in km associated with each
point. The model is written with both 0 and 360 longitude entries.
Coordinates are planetocentric. Generation is described in Thomas
(1993).
Phobos rotates synchronously with its orbital period, with libration
of about 1 degree. Spin pole: RA=317.68, Dec= 52.90 J2000 in degrees.
Prime meridian W = 35.06 + 1128.8445850d in degrees, where d is the
number of days from the standard epoch (JD 2451545.0).
See Davies, et al. (1996) for slight variations with precession;
Duxbury and Callahan (1989) for libration."
...