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That is a strawman, starthaus. The authors said
If [itex]ds_1[/itex] and [itex]ds_2[/itex] are the arc lengths subtended by differential angular element [itex]d\alpha[/itex] and if [itex]a[/itex] is small compared to R11
[tex]dm_i = \lambda ds_i \simeq l_i \lambda d\alpha \qquad\qquad(2)[/tex]
The astute reader will note that Eq. (2) will not be valid for values of [itex]a\sim R[/itex], since the angle [itex]d\alpha[/itex] would subtend a mass larger than [itex]ds_i[/itex] by a factor of [itex](\cos \alpha)^{-1}[/itex]. Since the orbits of Venus and Mercury differ by approximately a factor of 2, we repeated the calculation including the [itex](\cos \alpha)^{-1}[/itex] term. An exact solution could not be found, but a series expansion to terms of order [itex](a/R)[/itex] showed that the errors introduced by ignoring the [itex](\cos \alpha)^{-1}[/itex] term were of order of 2.3%.In other words, the authors explicitly acknowledged that this is an approximation and they checked the validity of the approximation.
If [itex]ds_1[/itex] and [itex]ds_2[/itex] are the arc lengths subtended by differential angular element [itex]d\alpha[/itex] and if [itex]a[/itex] is small compared to R11
[tex]dm_i = \lambda ds_i \simeq l_i \lambda d\alpha \qquad\qquad(2)[/tex]
The astute reader will note that Eq. (2) will not be valid for values of [itex]a\sim R[/itex], since the angle [itex]d\alpha[/itex] would subtend a mass larger than [itex]ds_i[/itex] by a factor of [itex](\cos \alpha)^{-1}[/itex]. Since the orbits of Venus and Mercury differ by approximately a factor of 2, we repeated the calculation including the [itex](\cos \alpha)^{-1}[/itex] term. An exact solution could not be found, but a series expansion to terms of order [itex](a/R)[/itex] showed that the errors introduced by ignoring the [itex](\cos \alpha)^{-1}[/itex] term were of order of 2.3%.