Motion of a substantial part of the superfast exoplanets is found to be in the close resonance with the well-known “solar” timescale $$P_{0} \approx 0.11$$P0≈0.11 days and/or the timescale 2$$P_0$$P0/$$\pi \approx 0.07$$π≈0.07 days (at 99.9% confidence for exoplanet periods $$P < 2$$P<2 days). There is also a noticeable lack of the exoplanetary “unstable” orbits with $$P \approx 3 \pi$$P≈3π$$P_0$$P0$$\,\approx 1.05$$≈1.05 days, which copies the famous “period gap” of the cataclysmic variables at $$P \approx 0.11$$P≈0.11 days; strangely enough, the ratio of the central periods of these two gaps is equal to $$\pi ^2$$π2. The exoplanet phenomenon is supposed to be caused by a coherent, with the $$P_0$$P0 timescale, oscillation of gravity, operating within the extra-solar planetary systems.

中文翻译：

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超快系外行星和 9600 秒

大部分超快系外行星的运动被发现与众所周知的“太阳”时间尺度 $$P_{0} \approx 0.11$$P0≈0.11 天和/或时间尺度 2$$P_0 密切共振$$P0/$$\pi \approx 0.07$$π≈0.07 天（对于系外行星周期 $$P < 2$$P<2 天的置信度为 99.9%）。也明显缺乏 $$P \approx 3 \pi$$P≈3π$$P_0$$P0$$\,\approx 1.05$$≈1.05 天的系外行星“不稳定”轨道，它复制了著名的灾难性变量的“周期差距”在 $$P \approx 0.11$$P≈0.11 天；奇怪的是，这两个缺口的中心周期之比等于 $$\pi ^2$$π2。系外行星现象应该是由在太阳系外行星系统内运行的具有 $$P_0$$P0 时间尺度的重力振荡引起的。