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Astronomical coordinates
JRS: In article , dated Thu,
12 Jan 2006 23:30:50 local, seen in news:sci.astro, Jonathan Silverlight posted : In message , Dr John Stockton writes Since the Astronomical Unit is defined as the *mean* distance between earth and sun, ... A bit of rummaging around on the Web shows that the definition is a lot more complex than that. This seems typical " the radius of an unperturbed circular orbit a massless body would revolve about the sun in 2*(pi)/k days (i.e., 365.2568983.... days), where k is defined as the Gaussian constant exactly equal to 0.01720209895." http://neo.jpl.nasa.gov/glossary/au.html That's not even grammatical, at least in our language. Diverted to a group more suited to rational discussion, and accompanied by a suggestion for ST that FAQ W.18 might possibly be modified to give or point to the current authoritative international standard definitions (if there be such). Does/should the Light Year depend on the Tropical Year or the SI/Gregorian one? Is the AU *defined* as 149 597 870 660 000 metres, with "mean separation" being merely icing on the cake - or /vice versa/? In other words, can new radar work change that number, or is it now as fixed as 299 792 458 m/s is? -- © John Stockton, Surrey, UK. Turnpike v4.00 MIME. © Web URL:http://www.merlyn.demon.co.uk/ - FAQqish topics, acronyms & links; Astro stuff via astron-1.htm, gravity0.htm ; quotings.htm, pascal.htm, etc. No Encoding. Quotes before replies. Snip well. Write clearly. Don't Mail News. |
#2
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Astronomical coordinates
http://neo.jpl.nasa.gov/glossary/au.html
At least some guys stand a chance of breaking out of that audacious maneuver of Newton in converting Flamsteed's 1461 day calendrical/celestial sphere average for axial rotation to a geocentric/heliocentric orbital equivalency,this one - "That the fixed stars being at rest, the periodic times of the five primary planets, and (whether of the sun about the earth, or) of the earth about the sun, are in the sesquiplicate proportion of their mean distances from the sun." Newton http://members.tripod.com/~gravitee/phaenomena.htm Even I was impressed,at least for a while,at the way Newton converted the distance along the circumference of an orbit to stretching of orbital distances based on the sidereal average.You get the right answer working off mean Sun/Earth distances however you cannot fit the ..986 degree orbital displacement into an elliptical framework at retain Keplerian motion. Do you not think that the Earth travelling faster at the aphelion is pretty ugly even if you seemingly get the correct answer for stretching and diminishing orbital distances .It was not a bad attempt and to be fair,he was consistent in his misconduct or misjudgement. People are too impressed with mindnumbing significant digits and leave the celestial images,motions and orientations too soon.They can make more informed judgements on what exactly went wrong and where with just a little more attension to the details of the origins of Copernican heliocentricity before making the leap to Keplerian refinements. |
#3
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Astronomical coordinates
In message , Dr John Stockton
writes JRS: In article , dated Thu, 12 Jan 2006 23:30:50 local, seen in news:sci.astro, Jonathan Silverlight posted : In message , Dr John Stockton writes Since the Astronomical Unit is defined as the *mean* distance between earth and sun, ... A bit of rummaging around on the Web shows that the definition is a lot more complex than that. This seems typical " the radius of an unperturbed circular orbit a massless body would revolve about the sun in 2*(pi)/k days (i.e., 365.2568983.... days), where k is defined as the Gaussian constant exactly equal to 0.01720209895." http://neo.jpl.nasa.gov/glossary/au.html That's not even grammatical, at least in our language. Well, "our language" is NASAspeak there :-) Diverted to a group more suited to rational discussion, and accompanied by a suggestion for ST that FAQ W.18 might possibly be modified to give or point to the current authoritative international standard definitions (if there be such). Does/should the Light Year depend on the Tropical Year or the SI/Gregorian one? Is the AU *defined* as 149 597 870 660 000 metres, with "mean separation" being merely icing on the cake - or /vice versa/? In other words, can new radar work change that number, or is it now as fixed as 299 792 458 m/s is? This site seems to have the answers to your questions http://www.vt-2004.org/Background/Infol2/EIS-G3.html The AU is derived and its value may change. The year is the Julian year. |
#4
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Astronomical coordinates
At the accuracy that most distances measured in light years are known. I'm
surprised that it matters which 'year' is used. I'd also be surprised if a light year is not a defined distance rather than calculated from c. and and an earth year, and therefore subject to revision at each redefinition of those units. 'Light years', though a perfectly good unit, are a basically amateur unit, anyway. Professionals tend to use parsecs (Another geocentric unit!) Roger |
#5
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Astronomical coordinates
Proffessional bluffers !, at the level of Newton's
geocentric/heliocentric orbital equivalency (quasi-geocentricity) which generates the mean Sun/Earth distances and subsequently the AU,the details of Newton's misjudgements can be handled comfotably in respect to Keplerian motion.Converting an axial rotational coordinate of .986 deg/3 min 56 sec to an orbital displacement is breathtaking in its audacity however tranfering the differential from mean distances through the center of a planet's orbit to mean Sun/Earth distances and then on to orbital stretching is truly a remarkable exercise* .It effectively wipes out the principles of Copernican heliocentricity and its later Keplerian/Roemerian refinements. If anyone can condone the Newtonian manner in which observed planetary motions are resolved they can believe in anything they want hence the contemporary undisciplined help-yourself-to-a-theory opinions.Professional ditherers relying on definitions is hardly astronomy,at least the amateurs will show you pretty pictures and has some benefits. !. "PHENOMENON V. Then the primary planets, by radii drawn to the earth, describe areas no wise proportional to the times; but that the areas which they describe by radii drawn to the sun are proportional to the times of description. For to the earth they appear sometimes direct, sometimes stationary, nay, and sometimes retrograde. But from the sun they are always seen direct, and to proceed with a motion nearly uniform, that is to say, a little swifter in the perihelion and a little slower in the aphelion distances, so as to maintain an equality in the description of the areas. This a noted proposition among astronomers, and particularly demonstrable in Jupiter, from the eclipses of his satellites; by the help of which eclipses, as we have said, the heliocentric longitudes of that planet, and its distances from the sun, are determined." http://members.tripod.com/~gravitee/phaenomena.htm |
#6
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Astronomical coordinates
You talk rubbish and you can't spell. Go back to school......
oriel36 wrote: Proffessional bluffers !, at the level of Newton's geocentric/heliocentric orbital equivalency (quasi-geocentricity) which generates the mean Sun/Earth distances and subsequently the AU,the details of Newton's misjudgements can be handled comfotably in respect to Keplerian motion.Converting an axial rotational coordinate of .986 deg/3 min 56 sec to an orbital displacement is breathtaking in its audacity however tranfering the differential from mean distances through the center of a planet's orbit to mean Sun/Earth distances and then on to orbital stretching is truly a remarkable exercise* .It effectively wipes out the principles of Copernican heliocentricity and its later Keplerian/Roemerian refinements. If anyone can condone the Newtonian manner in which observed planetary motions are resolved they can believe in anything they want hence the contemporary undisciplined help-yourself-to-a-theory opinions.Professional ditherers relying on definitions is hardly astronomy,at least the amateurs will show you pretty pictures and has some benefits. !. "PHENOMENON V. Then the primary planets, by radii drawn to the earth, describe areas no wise proportional to the times; but that the areas which they describe by radii drawn to the sun are proportional to the times of description. For to the earth they appear sometimes direct, sometimes stationary, nay, and sometimes retrograde. But from the sun they are always seen direct, and to proceed with a motion nearly uniform, that is to say, a little swifter in the perihelion and a little slower in the aphelion distances, so as to maintain an equality in the description of the areas. This a noted proposition among astronomers, and particularly demonstrable in Jupiter, from the eclipses of his satellites; by the help of which eclipses, as we have said, the heliocentric longitudes of that planet, and its distances from the sun, are determined." http://members.tripod.com/~gravitee/phaenomena.htm |
#7
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Astronomical coordinates
In message , L
writes You talk rubbish and you can't spell. Go back to school...... Please don't respond to GK. It's a piece of Artificial Stupidity that only posts the same old script because someone takes the bait. |
#8
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Astronomical coordinates
It is too difficult to tell whether your justifications are inhuman or
subhuman,the idea that the Earth has a variable axial tilt to the Sun/orbital plane would be a joke if it were not that it is the majority view - http://www.diduknow.info/sun/images/high_low_sun.gif http://imagine.gsfc.nasa.gov/docs/as...s/980116c.html You poor creatures, following after Flamsteed and Newton, mistake the changing daylight/darkness asymmetry for the Total length of a day represented by the Equation of Time. http://www.pfm.howard.edu/astronomy/...S/AACHCIR0.JPG I assure you that while parts of Newton's ballistic agenda can be salvaged absolutely nothing remains of the astronomical format built around the sidereal justification .At least Newton was consistent in his misjudgements or misconduct and especially in the way he shifted an axial cordinate to an orbital coordinate to generate his mean Sun/Earth distances.He got his correct answer for Keplerian elliptical geometry alright but you can't fit a .986 degree orbital displacement in an elliptical framework and get Keplerian motion. Squirm all you will,you live with an error so basic that it would be a joke in the era of Galileo and Kepler. |
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