Bandersnatch said:
This one rotation of difference is exactly the same difference between the 0:1 and 1:1 rotation : orbit relations.
It would probably be less confusing if you dropped this switching of reference frames. Stick to the inertial frame (i.e. the one used for the sidereal rather than the tropical year).
In order to fully understand the sidereal perspective, then it's imperative to compare the sidereal (OUTSIDE) perspective with the center-point perspective (such as from Earth or from the sun, as the case may be).
Let's review your claim that there's only a difference of one (1) rotation between -0:1 and +1:1 (NOTE - as you suggested, I'm now adding a neg "-" sign for retrograde CW orbits, and a "+" sign for regular CCW prograde orbits).
Clearly, the sidereal (view from the stars) and center-point perspectives (view from Earth, or other primary), they always differ by ONE (1) apparent rotation:
Synodic Motion
The word synodic derives from the Greek word for meeting or assembly. It is motion relative to a conjunction or alignment of sorts. A synodic or solar day is the time it takes the sun to successively pass the meridian (astronomical noon). A mean solar day is 24 hours (the “mean” is there to average over the effect of the analemma). The Earth has to rotate more than 360° for the sun to come back to “noon”.
A synodic year is the time it takes for a planet-sun alignment to reoccur. For the case of the sun, it is the time it takes the sun to come to the same place on the ecliptic (equinox to equinox) and is called a Tropical Year.
A tropical year is 365.242 mean solar days (366.242 sidereal days. It is just over 20 minutes shorter than a sidereal year (again, the effect of precession).
http://astro.unl.edu/naap/motion3/sidereal_synodic.html
If Earth has
366.242 sidereal days, then we need to subtract ONE (1) to determine Earth's actual CCW polar axial rotations, as explained here:
Sidereal Time
Another way to see this difference is to notice that, relative to the stars, the Sun appears to move around the Earth once per year.
Therefore, there is one fewer solar day per year than there are sidereal days. This makes a sidereal day approximately 365.24 ⁄ 366.24 times the length of the 24-hour solar day, giving approximately 23 hours, 56 minutes, 4.1 seconds (86,164.1 seconds).
Venus rotates retrograde with a sidereal day lasting about 243.0 earth-days, or about
1.08 times its orbital period of 224.7 earth-days; hence by the retrograde formula its solar day is about 116.8 earth-days,
and it has about 1.9 solar days per orbital period.
https://en.wikipedia.org/wiki/Sidereal_time
The reason that the sidereal perspective always has one (1) more
apparent 360° rotation per CCW orbit, is because typically from the sidereal perspective the orbiting body's polar axial rotations (if any) are aggregated in with the orbiting body's 360° orbit.
Conversely, for astronomical bodies with a retrograde CW rotation, such as Venus, you instead need to ADD one (1) to their sidereal rotation rate to determine the actual number of their polar axial rotations:
"All the planets of the Solar System orbit the Sun in a counter-clockwise direction as viewed from above the Sun’s north pole. Most planets also rotate on their axis in a counter-clockwise direction,
but Venus rotates clockwise (called “retrograde” rotation) once every 243 Earth days—the slowest rotation period of any planet. To an observer on the surface of Venus, the Sun would rise in the west and set in the east.
"A Venusian sidereal day thus lasts longer than a Venusian year (243 versus 224.7 Earth days). Because of the retrograde rotation, the length of a solar day on Venus is significantly shorter than the sidereal day, at 116.75 Earth days (making the Venusian solar day shorter than Mercury’s 176 Earth days);
one Venusian year is about 1.92 Venusian (solar) days long."
http://blog.world-mysteries.com/science/puzzles-of-the-moon/
Venus has 1.92 actual CW polar axial rotations per each orbit, which is slightly less than two full solar days. However,
Venus only has -0.92 sidereal rotations (224.7 divided by 243 = 0.92). The reason why you need to ADD one (1) for CW rotating bodies, is the same reason for subtracting one (1) for CCW bodies, because the sidereal perspective likewise aggregates together a retrograde body's CW polar axial rotations with the orbiting body's single CCW 360° orbit.
An astronomical body with a prograde 360° CCW orbit with a retrograde 360° CW rotation, these two 360° spins in opposite directions (around two different axes) merely cancel each other out, which is why you need to add one (1) to Venus' -0.92 sidereal rotations to determine Venus' actual 1.92 CW polar axial rotations – it's as simple as that.
Can we now agree that the sidereal (outside) perspective differs from the center-point perspective, by one (1)
APPARENT rotation?
As the below orrery spins, if you were to view it from above, the moon in this orrery would behave exactly like the moon does (on the left) in the above graphic that the poster had asked about:
Let's compare the original poster's above graphic with the orrery:
In normal operation the orrery's faux-moon would match the moon on the left. However, if you reached out and forced the orrery's faux-moon to point at one wall as you cranked that orrery around, then the faux-moon would necessarily be forced to spin CW around its supporting metal spindle (360° one time), as the moon on the right is doing. If you reached out and spun the faux-moon CW 0.92 times per revolution, then that is what Venus is now doing, -0.92 from the sidereal perspective, but 1.92 360° CW rotations from the sun's center-point perspective.
NOTE – When viewing either the orrery or any graphic such as the graphic above, you are necessarily placed in the outside sidereal position, so you need to either add one (1) or subtract one (1) to determine the moon's actual polar axial rotations in these models.
The moon's surface on the right is clearly moving in relation to the planet in the center (and would thus still be experiencing tidal braking forces). Imagine yourself standing on the planet on the right, and clearly you would observe the moon on the right making one 360° CW polar axial rotation per each CCW orbit, so while from the sidereal perspective the moon appears to be pointing in one direction and not rotating, ADD one (1) to that sidereal zero rotation rate, and the moon is actually making one (1) CW polar axial rotation per orbit.
That many people see a zero-rotating moon is just an optical illusion from the sidereal perspective since that moon is actually making TWO 360° spins in opposite directions.
When you're dealing with bodies in motion there are many possible optical illusions arising from the nature of the orbits. E.g., from Earth's perspective, there are times when Mars appears to be traveling backwards compared to the "fixed stars”:
Bandersnatch said:
If Venus has 0.92 clockwise rotations per year, then it has -0.92 counter-clockwise rotations per year. As a convention, the counter-clockwise direction is the direction used for positive values in orbital and rotational periods. So, current rotation : orbit relation for Venus is -0.92:1, and it had passed -1:1 rather than 1:1.
edit: here's me not checking the facts. Venus' rotational period is longer than the orbital period, so it's definitely not -0.92:1. but -1.08:1.
Your 1.08 rotation claim is wrong since 1.08 is what you get by dividing Venus' 225 day orbit into Venus' '
APPARENT' sidereal rotation rate of 243 days:
Venus
sluggishly rotates on its axis
once every 243 Earth days, while it orbits the Sun every 225 days - its day is longer than its year! Besides that, Venus rotates retrograde, or "backwards," spinning in the opposite direction of its orbit around the Sun. From its surface, the Sun would seem to rise in the west and set in the east.
https://solarsystem.nasa.gov/planets/profile.cfm?Object=Venus
243 days divided by 225 days = 1.08
However, Venus' 225 day orbit divided by its 243 day apparent sidereal rotation rate, instead gives the correct answer of 0.92 sidereal rotations per orbit.
1.08 is instead how many times Venus needs to rotate around its polar axis per each sidereal day in relation to a Venusian year (i.e., Venus' sidereal day is a tad longer than a Venusian year):
Sidereal Time
Another way to see this difference is to notice that, relative to the stars, the Sun appears to move around the Earth once per year. Therefore, there is one fewer solar day per year than there are sidereal days. This makes a sidereal day approximately 365.24 ⁄ 366.24 times the length of the 24-hour solar day, giving approximately 23 hours, 56 minutes, 4.1 seconds (86,164.1 seconds).
Venus rotates retrograde with a sidereal day lasting about 243.0 earth-days,
or about 1.08 times its orbital period of 224.7 earth-days; hence by the retrograde formula its solar day is about 116.8 earth-days, a
nd it has about 1.9 solar days per orbital period.
https://en.wikipedia.org/wiki/Sidereal_time
Clearly, Venus currently has 1.92
ACTUAL 360° CW polar axial rotations per complete orbit, (Venus has nearly two (2) solar days per orbit), but if you prefer, we can use sidereal days, which would be one (1) less, or -0.92 sidereal days per orbit.
We still have the same dilemma, if Venus currently has -0.92 CW sidereal rotations per orbit (-0.92:1), then Venus must have recently passed thru
-1:1 to now be at
-0.92:1.
Since Venus also clearly has nearly two (2) actual CW polar axial rotations per orbit (and nearly two solar days remaining), that means Venus has also passed thru a 2 full solar day rotation to wind down to only 1.92 solar days that it has today, which means that Venus has nearly two full polar axial rotations left to lose before being fully despun at your sidereal +1:1 tidally locked rate.
I already explained, from the SIDEREAL perspective, how it would be possible for Venus to lose nearly two (2) actual CW polar axial rotations and go from its current -0.92:1 sidereal rotation rate to a tidally locked rotation rate of +1:1:
CW: -4:1 ~ -3:1 ~ -2:1 ~ -1:1 ~ -0:1 ~ +1:1
If you can explain how Venus can bleed off nearly two full CW polar axial rotations, starting at its current -0.92:1 rate without passing thru that zero sidereal rotation rate, then I'd like to see that done?
Also, if you believe that a tidally locked body has one (1) CCW rotation per orbit (once despun at your
+1:1), then you may want to explain how Venus will not only lose nearly two CW polar axial rotations starting from -0.92:1, but then once Venus is fully despun at +1:1, please do explain how Venus will suddenly start rotating one (1) full time in the opposite CCW direction after Venus becomes tidally locked at +1:1?
The sidereal perspective has its practical uses, but as Venus proves, the sidereal perspective has its quirks, too.
Bandersnatch said:
No. When its rotation in an inertial frame of reference is 0, it necessarily means that its rotational angular momentum is also 0. As tidal interactions continue to accelerate the planet, it gains rotational angular momentum until it settles in a stable 1:1 synchronous rotation.
Are you claiming t
idal interactions can accelerate a planet's polar axial rotation? If you really do mean its rate of rotation, then do you have a citation for that? Yes, tidal braking can increase an orbiting body's orbital speed, but we're talking about decelerating Venus' rotational speed from -0.92:1 down to +1:1. Increased orbital speed is just where the lost rotational energy is transferred to (along with some loss to heating), but that isn't what you appear to be claiming?
As far as I know, whether a planet or moon has either a prograde or retrograde axial spin, tidal braking forces would slow down either type of rotating body. Of course, with a retrograde CW rotating (and CCW orbiting) body, the primary's gravity would be pulling the planet's tidal bulge in the opposite direction of its orbital direction, which may decrease its orbital speed a tad, but not sure about that and I'm just throwing out the possibility? Even so, a planet the size of Venus likely wouldn't have its orbital speed affected too much as it loses only two more CW polar axial rotations.
Bandersnatch said:
The moon on the right rotates only in a non-inertial, rotating reference frame.
There's nothing wrong in using a non-inertial frame to describe motion, as long as you clearly state if you're using it and are consistent about it. The default for most applications in astrodynamics is the inertial frame.
Let's try to keep this simple and explain it in a way a layman can understand. By a "non-inertial frame" you mean from Earth's perspective.
Bandersnatch said:
It's strongly advisable not to switch frames as you analyse motion to avoid confusion and wrong results - for example, while the moon on the right rotates in any rotating reference frame, and in particular rotates at 1 rotation per orbit in a frame rotating with the angular velocity equal to orbital angular velocity of the moon, in the same frame the moon is not orbiting - it is hovering in one place above the observer, supported by a pseudo-force, and has no orbital angular momentum as a result.
The seemingly zero-rotating moon on the right in the above graphic would NOT be hovering in one place above an observer standing on the planet in the center, since such an observer would clearly see that moon both orbiting CCW as well as rotating around its polar axis CW, ONCE per each orbit. The only thing not stable about a seemingly zero-rotating moon (from the sidereal perspective), is that such a moon would still have one last CW rotation left to lose, so it would merely pass thru -0:1, then go to -0.01:1, then -0.02:1, then -0.03:1, then -0.04:1, etc, until stopping at a final +1:1 sidereal rate. As that moon passes thru that -0:1 rate, the background stars would slowly begin to move again in relation to its surface, and gradually increase their movement until the moon reached its final +1:1 rate.
It's only from the sidereal perspective that such a body would seemingly pass thru that transitional -0:1 rate as it was being despun. On planet Venus, its days will just get gradually longer and longer (going from 1.92 days per orbit to zero days), until Venus eventually runs out of steam and locks, at which point Venus will only show one face inwards towards the sun, just as our moon now only shows one face inwards towards Earth.
Unlike our own moon, Venus' backside will be in perpetual darkness one it locks to the sun.
Further, if you stood on that seemingly zero-rotating moon's surface on the right, then the stars wouldn't appear to move much (the stars would move a tad due to librations), but the Earth would rise in the West and set in the East each orbit. If you instead stood on the other moon's surface (the left moon in the graphic), as astronauts have already done, then Earth would hang nearly motionless in the sky, except for minor movements again due to librations, caused by the moon's elliptical orbit, as well as by the tilt of the moon's orbit in relation to Earth's orbital plane.
Bandersnatch said:
I think the bottom line here is: stick to the inertial frames, or at least don't switch frames, and watch the signs. Otherwise you seem to get it right..
I feel I have it exactly right, and it's also necessary to switch between reference frames to help explain which frame better represents the reality of the movements that we're discussing here, as I hope I'm now doing with you.
:)
Bandersnatch said:
By the by, I wasn't aware of the discrepancy in Venus' rotation period. That's interesting. I wouldn't jump to conclusions, though.
Despite being our closest planetary neighbor, since Venus has been shrouded in clouds, it was only relatively recently by using radar that Venus's axial rotation could even be studied, and there doesn't appear to be much published on the planet's unique rotation. In my opinion, to understand what our own moon is doing, then you need to understand what Venus is doing.
For example, as you try to harmonize how Venus can lose nearly two full polar axial rotations, and be despun down from its current -0.92:1 to a tidally locked +1:1, then it may help you to understand what your +1:1 final sidereal rate actually means. The tip to that I already posted above:
If Earth has 366.242 sidereal days, then we need to subtract ONE (1) to determine Earth's actual CCW polar axial rotations.
Likewise, if our moon has a sidereal spin rate of one (1), then subtract one (1) from our moon's apparent sidereal spins, just as you need to do for Earth's 366 sidereal spin total to find the actual polar axial rotations of both:
MOON: 1 – 1 = 0
EARTH: 366.25 – 1 = 365.25
If you consider that our fully despun +1:1 moon now has zero polar axial rotations, then everything makes sense as Venus must lose nearly two rotations to go from -0.92 down to +1:1 sidereal rotations:
CW: -4:1 ~ -3:1 ~ -2:1 ~ -1:1 ~ -0:1 ~ +1:1
I realize what I'm saying here may sound like heresy to you at first blush, but synchronous theory has been disputed for hundreds of years by many notable scientists and astronomers.
If you need further proof, then please try and explain our moon's longitudinal librations within your synchronous theory framework?
Most websites claim our moon has a steady CCW rotation rate that gets out of sync as our moon's orbital velocity varies as it passes thru its apogee and perigee. However,
our moon's two maximum longitudinal librations actually occur midway between apogee and perigee!
That our moon's maximum longitudinal librations occur midway between apogee and perigee can be easily explained if you consider the possibility that our moon is today fully despun –– simply, midway between apogee and perigee, our fully despun moon is merely facing the empty focus of its elliptical orbit.
The sidereal perspective has its practical uses, but it's also not some
'God's Eye' view of reality!
Think about it.
Ken