Please help me calculate acceptable planet sizes & eclipse shadows cast by my binary planet system

Question

I've been reading here for a little while, but this is my first question. I am trying to come up with either a concrete set of numbers for a single answer for a binary planet system, or a simple formula that allows me to play within a range of acceptable numbers that answer my question. Math and I don't really get along anymore, so the less complex your solution, the better. Even a solution via simple 3D modeling / illustration on spheres or geometric drawings is welcome if it also provides numbers that fulfill the solution.

ALSO I'd like to keep this within the realm of plausibility, so sources for creating my system are listed after the question. I don't mind if the science pushes the boundaries of what we know. Unusual, rare, unlikely, and unique solutions are welcome; impossible ones are not.

Here are the shadows I'm trying to achieve:

Figure 1: The two possible shadows cast by each planet when all three bodies are in alignment

I'm going to leave my inaccurate drawings above for now because they better illustrate the landmasses and ocean areas on both planets. I'll replace them when I'm able. More accurate yet simpler sketches below along with (hopefully) improved wording.

Requirements:

1. Binary planets (tidally locked to each other) orbit an M0 parent star at the outermost edge of its habitable zone. (See note1) Neither planet, nor the binary system as a whole, supports a moon.

2. Both of these planets must be theoretically capable (liquid surface water / atmosphere / pressure / mass / density-wise) of supporting a range of humanoid and other life forms (akin to Tolkien's world, minus mankind as an example), and share biomes.
   They must not be closer to each other than 3 times the radius of Planet B. (See note2)

3. Planet B must be larger than Planet C and not be wider than 12000 km in diameter (slightly smaller than Earth size); however, I strongly prefer Planet B to be as small as possible within the given constraints.

4. Planet C must not be smaller than 6000 km in diameter. (See note3)

5. During A-B-C alignment (Fig 1)
   - A being floating in the center of the night side (it's in the middle of the ocean) of Planet B (point b) will see only a circle of darkness blocking the stars (behind Planet C) when looking toward Planet C. (Fig 1a) Planet C should fall well within the umbra cast by Planet B.
   - A being standing at point c will see a total eclipse of Star A by Planet B when looking starward. Only the corona should be visible (Fig 1b)

   
   

6. During A-C-B alignment, (Fig2)
   - A being standing in the center of the night side of Planet C (point c) will see Planet B as a thin blue ring – with an apparent width not wider than 1/6 the radius of Planet B – with northern polar ice visible. More temperate landmass may be visible closer to the northern side of the equator.(Fig 2a)
   - A being standing at point b will see an annular eclipse of Star A by Planet C because Planet C is not large enough to eclipse it totally (Fig 2b)

7. Rotation period for the two planet system should not be less than 16 hours nor more than 64.

Is this plausibly realistic?

I simultaneously hope this question is not too long and that I've provided enough info. If not, please me know what I can to do improve.

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(note1) ~0.5 solar masses.  See Habitable Planets for Man by Stephen Dole (second edition) American Elsevier Pub. Co. - 1970 pg. 81.  “For a special rare class of planets with extremely large or close satellites, there is an extension of the lower permissible primary mass [of the parent star] down to 0.35 solar masses.” My star falls well with this range, and the binary planet system fulfills the large/close satellite requirement.

(note2) Can binary terrestrial planets exist? at Phys.org

(note3) Jim2B’s wonderfully detailed answer to Worldbuilding question Smallest possible habitable planet? (also taking density into account)

Answer 1

Is It Possible?

Yes, this arrangement is possible. The rest of the answer is how to figure this stuff out:

Let's talk about angular diameter.

Angular Diameter is how big something looks: small things, but up close to the observer, can look just as large as something very large but very large away. This "apparent size" is called angular diameter. (Also yes, you can call it "apparent size," and "angular diameter," and other names...)

If the angular diameter is the same as something behind it, they will perfectly block each other. The relationship is:

$$\delta = \arctan(\frac{d}{2D})$$ Where d is the diameter of the object in question, and D is the distance from some chosen observation point and the midpoint of the object in question.

Determining Your System

I've made a little diagram showing you your situation:

Remember, the little d's represent the diameter of the bodies in question, and big D's represent the distance between a middle point and the midpoint of the things in question. $d_3$ is the diameter of the shadow.

You should also note that sum $D_1+D_3$ is not (always) the distance between the planets, but the distance between the planet making the shadow and the edge of the shadow on the other planet. Also, this point which everything is measured from is not the point about which the two planets revolve. (That point depends on the mass of both bodies.) Also, it should be noted that $D3$ is really an absolute value- the shadow (d3) could be going the other way, inside the cone.

For case 1, where the big planet overshadows the other one, the smaller planet's radius must be less than $d_3$ and $D_1+D_2$ is (at least) the distance between the two planets.

For case 2, where the small planet puts a shadow on the large one, the distance $D_1+D_2$ is the distance between the small plant's center and the center of the ring formed by edge of the planet's shadow. To make a ring, the larger planet's radius must be larger than $d_3$

Using this information, you can figure out what the diameters and distances of your planets should be.