![]() There is more detail on this and on the CWs for all my books at. Nobody has yet stopped me from writing cross-genre, and if "fake soulbonding in the space military" sounds like it could be your thing, then I appreciate those of you giving it a shot from whichever side of the genre line!ĬONTENT WARNINGS: mind-control, coercion, mental health struggles (self-destructive tendencies and thoughts, self-neglect including chaotic eating habits), imprisonment, mind/body sharing, some drug and alcohol use. I'd categorise this one as slightly more on the SF side of the SF/Romance border. If you're primarily an SF reader you'll probably think it has a lot of romance. □ There is a strong romantic arc and emotions are high, but if you're a romance reader please go in expecting a VERY low heat level. □ It's a space adventure with a military-SF feel (I wouldn't classify it as strict MilSF since the army is mainly the antagonist and the main character spends the whole book trying to get out of it.) ![]() It's in the same universe as Winter's Orbit but there's no overlap in characters or locations. □ The story takes place on the planet Orshan where, as the result of some dodgy experimentation, some people have the ability to read or control minds. Things that you should know about it (expand for CWs): This book includes: a main character who is having a bad day and intends to make it everyone else's problem, psychics behaving badly, pining, space battles, making out during a break-in, awful families, and the terror of being known and then loved in spite of it. I originally pitched this as "like fake dating but with fake soulbonding, also both characters are in the space military." This book includes: a main character who is having a bad day and intends to make it everyone else's problem, psychics behaving b I originally pitched this as "like fake dating but with fake soulbonding, also both characters are in the space military." Even though, at this time of year, we're as close to the Sun as we can get, for the Northern Hemisphere, it will always be winter.1 of 5 stars 2 of 5 stars 3 of 5 stars 4 of 5 stars 5 of 5 stars The difference between the two is 5,003,451 km, (3.3 percent), and not enough to cause the seasons. Aphelion, the greatest distance from the Sun, occurs on July 7, 2007, when the Earth-Sun distance will be 152,097,053 km. The Earth-Sun distance will be 147,093,602 km. The two times can vary by as much as 16 minutes over the course of a year.Įarth reaches perihelion on Janu(Figure C). The equation of time is defined as the difference between true solar time (determined by the Sun's position in the sky) and mean solar time (the time told by your watch). For all points along the curve to the right of the meridian, the sun is "fast," crossing the meridian slightly before noon.Īstronomers call this the equation of time. For all points along the curve to the left of the meridian, the Sun is "slow." It crosses the meridian after 12:00 p.m. The result of this change in speed means the Sun crosses the meridian a little early, or a little late, depending on where Earth is in its orbit. In January, we are closer to the Sun, and Earth speeds up a bit in its orbital progress. In July, we are at our furthest point from the Sun, and Earth moves slower than average along its path. ![]() ![]() If Earth's orbit was a perfect circle, the Sun would cross the meridian at noon every day (ignoring daylight savings time). The meridian runs straight up and over the sky, from due north to due south. Notice the vertical line running up from the south point on the horizon? That's the meridian. That's where our elliptical orbit comes in! Look at Figure A again. Currently, Earth’s eccentricity is near its least elliptic (most circular) and is very slowly decreasing, in a cycle that spans. What about the left-to-right variation in the analemma's curve? When Earth’s orbit is at its most elliptic, about 23 percent more incoming solar radiation reaches Earth at our planet’s closest approach to the Sun each year than does at its farthest departure from the Sun. The difference in the Sun's noontime height in the sky is caused by Earth's tilted axis. The lowest point marks the winter solstice. The highest point on the analemma is the Sun's noon position on the summer solstice. ![]()
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