Sunday, August 7, 2011

Gravity Increased By Lunar Surface Temperature Differential

Abstract presented at April 13-16 APS meeting:
Bulletin of the American Physical Society 58(4) 186 (2013)

Abstract and Introduction
Quantitatively large effects of lunar surface temperature on apparent gravitational force measured by lunar laser ranging (LLR) and lunar perigee may challenge widely accepted theories of gravity. LLR data [1] grouped by days from full moon shows the moon is about 5 percent closer to earth at full moon compared to 8 days before or after full moon. In a second, related result, moon perigees were least distant in days closer to full moon. Moon phase was used as proxy independent variable for lunar surface temperature. These results support the prediction by binary mechanics (BM) [2] that gravitational force increases with object surface temperature [3].

Methods and Results
Fig. 1: Lunar Distance vs Days from Full Moon

The entire LLR data set of 8093 measurements from 1987 to 2004 of the l'Observatoire de la Côte d'Azur (OCA) in France [4] was grouped by day from full moon computed with U.S. Naval Oceanography data [5] (mean and SEM in Fig. 1, Table 1). These two data sets were synchronized by universal times. Earth-moon distance was expressed in laser round-trip time in milliseconds. This raw data and the source code for the analysis software is available from the author.

Table 1: Lunar Distance in Msec vs Day from Full Moon
Day   N    msec   std error
 0    31  2431.88  10.64
 2   195  2456.04   6.67
 3   936  2495.87   3.47
 4   946  2501.72   3.27
 5  1182  2527.47   2.73
 6  1270  2529.71   2.33
 7  1265  2550.60   2.21
 8   884  2559.58   2.64
 9   620  2553.51   3.25
10   477  2552.91   4.29
11   227  2547.95   6.80
Minimum lunar distance was observed in the 24 hour period of full moon (day 0 in Fig. 1 and Table 1) when lunar surface temperature would be expected to be greatest. As solar illumination of the lunar surface facing earth decreases, lunar distance increased up to a maximum at day 8 before or after full moon, representing about a 5 percent decrease in lunar distance at full moon, where (2559.58 - 2431.88)/2559.58 = 0.0499.

In general, a steady increase in lunar distance over days 0 to 8 was seen. This effect appears to plateau over the 7 to 11 day range.

The 11 sample means in msec were all clearly different according to the 2-sample t test of statistical significance, except differences between day pairs 3 and 4, 5 and 6, 9 and 10, and 10 and 11.

Table 2: Lunar Perigee Distance in km vs Day from Full Moon
Day  N    km      std error
 0  17  356890.71   64.66
 1  31  358637.19  172.48
 2  22  362307.00  205.20
 3  17  365739.12  208.10
 4  11  368019.36  130.40
 5   7  369221.71  210.53
 6   4  369613.75  176.81
 7   7  369965.86   86.28
 8   7  369827.14  134.47
 9   8  369307.88   94.73
10   9  367995.44  131.30
11  19  365657.89  196.61
The lunar perigee distance is the shortest distance from earth in each eccentric cycle of the orbit of the moon around earth [6]. Table 2 tabulates these perigees in km by day from full moon for the same Oct, 1987 to Dec, 2004 period of the LLR data shown in Table 1. The product-moment correlation r between day from full moon and perigee distances (Table 2) is 0.716 (N = 12), with r2 = 0.513, which implies that about half of the perigee distance variation may be accounted for by day from full moon.

The calculated perigees (Table 2) were on average some 10788 km less than the distances implied by the LLR measurements, when converted to km (Table 1). Fig. 2 shows the LLR data in km (mean and SEM) as offsets from the calculated perigee mean values on a per day basis. That is, the Y-axis is the deviation of the LLR-perigee difference from the mean difference of the 11 points.

Fig. 2: LLR minus Perigee vs Days from Full Moon
From days 0 to 6 the shortest distances occurred, while longer values were seen on days 7 to 11 from full moon. Perhaps of special interest is the almost linear upward trend in offsets of LLR distance from calculated perigee from day 2 to day 11. Indeed, for these days, the product-moment correlation between day and LLR distance minus perigee is r = 0.97 (N = 10). That is, for days 2 to 11 from full moon, time from full moon accounted for 94 percent of the variance of LLR distance minus calculated perigee values.

The present study aimed to test the hypothesis predicted by BM [3] that observed gravitational force increases with increased object surface temperature.

First, moon phase was used as an indication of the independent variable -- temperature on the lunar surface facing earth, with highest temperature associated with full moon. LLR data was used to operationally define the dependent variable -- earth-moon gravitational force, assumed to be inversely related to lunar distance (Table 1). In short, greater lunar surface temperature in the direction of earth was associated with motion reducing lunar distance.

Second, moon perigees were least distant in days closer to full moon. The orbit of the moon around earth has an approximate 5 percent eccentricity [6]. At lunar perigee, the moon is about 5 percent closer to earth, compared with lunar apogee. Further, the actual lunar distance at perigee also varies substantially. The present study may explain one half (51%) of perigee distance variation in terms of days to full moon in the day 0 to 11 interval (Table 2). That is, the presumed effect of temperature of the surface facing earth on apparent gravitational effects may account for about one half of perigee distance variability.

The approximate plateau from days 7 to 11 (Fig. 1) is not entirely consistent with the present hypothesis, since solar illumination of the lunar surface facing earth continues to decrease in the day 8 to 11 period, suggesting decreased lunar surface temperatures over that lunar surface area. This issue might be resolved by further analysis including the perigee cycles which may explain the present plateau in LLR data as a function of time from full moon in the period studied. Perhaps there is sufficient correlation between the perigee and new moon phases to account for the perigee effect opposing further increases in lunar distance in the reported 8 to 11 day period where lunar surface temperature is thought to continue decreasing.

For example, the LLR distance means may be expressed as offsets from the calculated perigee means, in a composite dependent variable, as shown in Fig. 2. These deviations of mean LLR from mean calculated perigees indicated greater distances over the range from day 2 to 11 as lunar surface temperature presumably decreased, supporting the hypothesis that apparent gravitational force depends on object surface temperature.

Although the results reported exhibit high levels of statistical significance, the OCA data analyzed is only a fraction of available LLR data over longer periods from other observatories, allowing ample opportunity to replicate the reported effects.

Lunar phases reflect changes in the sun-moon-earth angle. At any time, about half of the lunar surface is illuminated and warmed by the sun while the other side of the moon is dark and becomes cooler. Hence, the volume-averaged temperature of the moon may be essentially constant over days before or after full moon shown in Figs. 1 and 2. Therefore, the effect discovered in this report appears to depend on a surface temperature differential comparing near and far sides of the moon as lunar phase changes. Namely, when this temperature difference increases on days closer to full moon, earth-moon distance decreases. The vector from the coolest to the warmest surface area appears to approximate the direction of this motion component.

Conventional treatment of thermal energy as a gravitational mass equivalent fails to account for the reported results. BM is the only physical theory known to the author predicting the present results. Gravity is not a primary force in BM [7], but rather a result of four postulated bit operations -- unconditional, scalar, vector and strong, which define exact time-development of BM states [8]. In this context, objects tend to move in the direction of greater 1-state bit density. Observed gravitational forces are simply a specific instance of this general principle.

With increased surface temperature, an object will tend to radiate more 1-state bits from its surface. At full moon, these emitted 1-state bits will tend to increase bit density between earth and moon, compared to other directions, causing object motion decreasing lunar distance. A similar mechanism may explain the Pioneer anomaly [9] where it may be no coincidence that the direction of anomalous motion is toward the greatest nearby source of radiated 1-state bits -- the sun.

[1] Bender, P. L. et al., "The lunar laser ranging experiment" 1973 Sci 182 229
[2] Keene, J. J. "Binary mechanics" J. Bin. Mech. July, 2010.
[3] Keene, J. J. "Physics glossary" J. Bin. Mech. May, 2011.
[4] l'Observatoire de la Côte d'Azur (OCA). "Lunar ranging results" February, 2005.
[5] U.S. Naval Oceanography (USNO). "Phases of the moon" August, 2011.
[6] Walker, J. "Lunar perigee and apogee calculator" May, 1997.
[7] Keene, J. J. "Gravity looses primary force status" J. Bin. Mech. April, 2011.
[8] Keene, J. J. "Bit operations order" J. Bin. Mech. May, 2011.
[9] Turyshev, S., Toth, V., Kinsella, G., Lee, S. C., Lok, S., Ellis, J. 2012 PhysRevLet 108 (24)
© 2011 James J Keene