In my post https://hunterfiftyfour.blogspot.com/2026/06/i-found-rahu-point-in-sky.html , (with the help of AI Claude) I found a spot in the sky that could be a Rahu point.
However, I was plagued by the thought how Rahu (and Ketu) would journey across the sky. In other words, what would be the moon's orbit about the Earth's orbit, or the ecliptic? In my mind's eye I envisioned as a corkscrew motion about the ecliptic. But that wouldn't cut the ecliptic. The moon's motion would in that case hover round the ecliptic, and not cut it. The second intuition was that of a bird's wings flutter relative to its path in flight. More about that as we go through this post.
To help clear my head I bounced my ideas with AI Claude, and elicited replies from it. Here is the conversation:
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Me:
There is a visualisation problem that I face. As per my visualisation, the Moon's move forward in space should be like a corkscrew motion around the ecliptic line. Then, how does it cut the ecliptic?
Claude:
What a great question — and your corkscrew intuition is almost right, which is exactly why it creates a visualisation problem. Let me fix the mental model. Great question! Your corkscrew intuition is actually very close to correct — the issue is just one subtle detail about the geometry of the corkscrew.
The key geometric idea
Rahu and Ketu are defined by the line of intersection of two planes:
-The ecliptic plane
-The Moon's orbital plane
Two flat planes always intersect along a single straight line. That line stabs through the ecliptic circle at exactly two opposite points — Rahu and Ketu, always 180° apart.
Without precession, that intersection line is frozen in space — so Rahu and Ketu are frozen too, even as the Moon corkscrews forward through them month after month.
Precession slowly rotates that intersection line — which is why the two stabbing points drift backward through the zodiac over 18.6 years.
So your corkscrew intuition was exactly right — the forward motion is real, but it's the tilt direction of the corkscrew axis that determines where the crossings happen in the zodiac. Without precession, same tilt direction = same two crossing points, forever.
Me:
Bit difficult to imagine. Is there a video that explains how the moon's orbit cuts at different points, yet points remain fixed relative to the background stars?
Claude:
Best video/animation resources
1. NASA Scientific Visualization Studio — most relevant to your question
The NASA SVS page for the 2017 eclipse shows the Moon's orbital plane as a light blue circle, and the ecliptic as an olive-coloured square. The darker half of the lunar orbit plane is below the ecliptic, and the dividing line between light and dark is the line of nodes. Critically — the radial grid on the lunar orbit plane is stationary relative to the stars, which is exactly what you're trying to visualise.
https://svs.gsfc.nasa.gov/4324/ — this is the one to watch
2. YouTube — Rahu and Ketu in under 2 minutes
A short animation specifically explaining the nodes: https://www.youtube.com/watch?v=pcbdUJGYxtM
3. SkyMarvels — Moon Orbit Variability
SkyMarvels has two animations showing the lunar orbit's wobble around Earth — the Moon doesn't continually trace the same path; its orbital plane wobbles, and the line of nodes precesses backwards roughly every 18.5 years.
https://www.skymarvels.com/infopages/vids/Moon%20Orbit%20Variability.htm
The key phrase to hold in mind while watching
Look for what NASA calls the "line of nodes" — it is the intersection of the Earth-Moon plane and the ecliptic plane, and it is this line that determines eclipse seasons. When the Sun aligns with this line, eclipses become possible.
Your geometric intuition — that the corkscrew crosses at different points along the ecliptic as the Moon progresses, yet the crossing points stay fixed relative to the stars — is precisely what the NASA animation makes visible. The line of nodes is like a skewer passing through the Earth, pointing at two fixed star-positions. The Moon's corkscrew passes through that skewer twice per month, always at the same two star-positions — until precession slowly rotates the skewer.
Me:
Skymarvels was more clear to me than NASA. To me it looks like this:
The journey of the moon's orbit looks like the wings of a bird fluttering about the journey of the moon along its orbit: the moon circumambulates along its orbit, and the orbit itself flutters like the wings of the bird taking the journey. Because of the flutter of the wings of that imaginary bird, the orbit of the bird always cuts the orbit of the earth (ecliptic), albeit at different points in space. And the orbit of the moon as a whole advances along the ecliptic, along with its flutter of course. Please give your thoughts on my analogy.
However, questions arise with the phases of the moon as given in the skymarvel's animation:
1. As in the images uploaded, why are we seeing no moon, although the earth and moon seem to be in each other's line of sight? We should be seeing full moon every night as per this image.
2. From the animation of skymarvel can we predict the eclipses?
Claude:
Your bird-wing analogy is excellent, and these two phase questions are exactly the right thing to be confused about — they expose a genuinely common misreading of that Solar System Simulator view. Let me take them in order.
Your bird-wing analogy
This is a lovely and pretty accurate image. Breaking down why it works:
- The bird's body following a path = the Moon orbiting the Earth-Sun line, advancing along the ecliptic over a year
- The wings fluttering up and down = the 5° tilt of the Moon's orbital plane, flapping above and below the ecliptic twice per month
- The wingtips brushing the ground at the bottom of each flap = the two nodal crossings (Rahu/Ketu) each orbit
- The flutter rate slowly changing phase relative to the body's path over a long flight = nodal precession, 18.6 years
The one refinement I'd add: the flutter isn't quite synced to the forward motion in a fixed way — it's almost but not exactly two flaps per "step" forward, which is precisely why the crossing points slowly slide backward instead of repeating in place. But as a mental picture, this is genuinely a very good one.
Your phase question — this is the important one
You've caught something real. Look at your image carefully: this is a view from the SUN, looking down at the Earth-Moon system. The label confirms it: "View of EARTH BARYCENTER from SUN."
That changes everything about how to read the picture.
In Image 1 (June 18, 2026), the Moon is on the far side of Earth, away from the Sun. If you're standing at the Sun looking toward Earth, and the Moon is behind Earth from your viewpoint... think about what that means for us on Earth looking at the Moon: the Sun is fully behind us, and the Moon is in front of us, fully lit from our perspective. That should be a Full Moon, not what's shown.
But the "Phase We See From Earth" box shows a thin crescent. Let's check what's actually going on: This confirms what the simulator was already telling you, and now I can resolve the puzzle properly.
Why "no moon" when Earth and Moon look "in line"
Real-world data confirms: on June 18, 2026 the Moon is a Waxing Crescent, 15% illuminated, 3.73 days old. Just three days earlier there was a New Moon (June 15). So a thin crescent is exactly correct — and the mystery is why your geometric intuition expected a Full Moon instead. Here's the resolution:
The trap is the word "line of sight." In your image, the Moon appears to be on the opposite side of Earth from where the orbit curve bends toward the viewer — but the Sun isn't in that picture at all. This is a view from the Sun, looking at Earth. The Sun itself is implicitly behind the "camera," i.e., on the near side, between you (the viewer) and Earth.
So re-read the geometry: if you (the camera) are at the Sun, and the Moon is on the far side of Earth, away from you — that means the Moon is on the far side away from the Sun too. That's New Moon geometry: Sun–Earth–Moon are roughly aligned, with the Moon "behind" Earth as seen from the Sun. From Earth, we'd be looking toward the Sun's direction to see the Moon, and the Moon's far side (away from the Sun) is what faces us — hence almost no illumination. That matches your image perfectly: a thin crescent, 3-4 days after New Moon.
I made an error in my first-pass reasoning above (in the part I "thought aloud" before checking) — I want to flag that directly since it's worth being explicit about: my initial instinct was that "Moon behind Earth as seen from Sun" should mean Full Moon. That's backwards. Full Moon happens when the Moon is on the far side of Earth away from the Sun, with Earth in between — i.e., visually, in a Sun-viewpoint image, Full Moon is when the Moon appears in front of Earth (near side, same side as the camera/Sun), not behind it.
So the rule for reading these Sun-viewpoint images is:
- Moon appears on the near side (toward the Sun/camera) → Full Moon (Earth's day side, sunlit Moon face, points toward us)
- Moon appears on the far side (away from Sun/camera) → New Moon
In your two images, the Moon is on the far side both times (slightly different ecliptic-crossing position), confirming both are near New Moon — consistent with the actual calendar: New Moon was Monday, June 15, 2026.
Can eclipses be predicted from this animation?
Yes — and this is actually the perfect tool for it. Here's the logic, building directly on your bird-wing analogy:
An eclipse requires two conditions simultaneously:
1. Sun-Earth-Moon must be aligned (New Moon for solar eclipse, Full Moon for lunar eclipse) — visible in this Sun-viewpoint image as the Moon being almost exactly in front of or behind Earth.
2. The Moon must be at or very near a node (Rahu/Ketu) — visible in this image as the Moon's orbit crossing the horizontal ecliptic line at the same place where the Moon currently is, not 90° away from it.
Look again at your Image 1 (June 18): the Moon is near the far end, close to where the tilted orbit ellipse crosses the flat ecliptic line. That's actually informative! If, at New Moon or Full Moon, you see the Moon sitting almost exactly on that ecliptic-crossing point in this exact Sun-viewpoint image — that's an eclipse. If the Moon is near New/Full phase but visibly off the ecliptic line (above or below it, at the "wingtip" of the flutter), no eclipse happens that month.
So your bird's flutter analogy gives you the eclipse rule for free: eclipses happen only when the New or Full Moon coincides with a moment when the wingtip is just brushing the ecliptic line** — i.e., conditions 1 and 2 above happening together. Most months, the Moon is near-aligned for phase but off the ecliptic (mid-flutter), so no eclipse occurs — exactly as you'd expect from a creature flapping while flying forward, only occasionally having its wingtip exactly graze the ground at the same moment it's also directly ahead or behind.
Me:
Before we go further: I am getting little confused on 'far side' and 'near side'. So what is the alignment of far side: Sun (camera) > earth > moon, or, Sun (camera) > moon > earth?
Claude:
Good catch — that's exactly the ambiguity worth nailing down before going further.
"Far side" (the New Moon case) = Sun (camera) → Earth → Moon
The Moon is positioned beyond Earth, farther from the Sun/camera than Earth is. So from the Sun's viewpoint, the Moon appears to sit behind Earth, partially or fully hidden in the image by Earth's position (though in your screenshots the orbit is tilted/edge-on enough that you can still see the Moon poking out beyond Earth rather than directly behind it).
Why this is New Moon: the Moon's far side (away from the Sun) is unlit, and that's the side facing Earth. Sun → Earth → Moon also means Earth sits between the Sun and Moon — which is the literal definition of New Moon alignment (even though "new moon" sounds like it should be the dramatic one, it's actually the dark one).
"Near side" (the Full Moon case) = Sun (camera) → Moon → Earth
Here the Moon is between the Sun and Earth in terms of distance from the camera — it appears in front of Earth, closer to the viewer/Sun. The face of the Moon getting sunlight is the same face pointed back toward Earth, so we see it fully lit. That's Full Moon.
A quick sanity check you can use going forward: whichever body is closer to the Sun (camera) in the image is the one whose Earth-facing side is lit as seen from Earth. Closer-to-camera Moon = Full Moon; farther-from-camera Moon (tucked behind Earth) = New Moon.
Me:
I could be getting ahead of myself, but here is my confusion: Sun(camera) > moon > earth is full moon, yet eclipse should happen when earth's shadow falls on moon, that is, Sun > earth > moon. And, I believe, eclipse occurs during full moon.
Claude:
You're not getting ahead of yourself — you've actually spotted a genuine subtlety that trips a lot of people up. Let's untangle it carefully, because you're right about both pieces, and they're not actually contradicting each other once we separate two different things being discussed.
The key distinction: phase vs. eclipse
These are two separate questions:
1. What causes the Moon's phase (how much of it looks lit from Earth)? — This depends on the Sun-Moon-Earth angle as seen broadly.
2. What causes a lunar eclipse specifically? — This requires Earth's shadow to fall on the Moon.
Resolving the apparent contradiction
You're right that a lunar eclipse needs Sun → Earth → Moon (Earth in the middle, casting its shadow onto the Moon). And you're also right that eclipses happen during Full Moon.
So here's the resolution: Sun → Earth → Moon alignment IS the Full Moon alignment. I gave you the wrong pairing in my last message. Let me fix it cleanly:
- Sun → Earth → Moon (Earth in the middle) = the Moon is on the far side of Earth, away from the Sun = the Moon's near face (facing Earth) is fully lit by the Sun = Full Moon. When this alignment is exact, Earth's shadow falls on the Moon = lunar eclipse.
- Sun → Moon → Earth (Moon in the middle) = the Moon is on the near side, between Sun and Earth = the Moon's face toward Earth is the unlit far side = New Moon. When this alignment is exact, the Moon's shadow falls on Earth = solar eclipse.
So I had the near/far labels backwards relative to the phases in my previous message. Thank you for catching this through your own reasoning rather than taking my labelling at face value — this is a good example of why checking a stated rule against a known fact (eclipses happen at Full Moon) is a great way to catch an error.
The corrected sanity check
Whichever body is positioned farther from the Sun/camera in the image (tucked behind Earth) → that's Full Moon, and that's when lunar eclipses can occur.
Whichever body is positioned closer to the Sun/camera (in front of Earth) → that's New Moon, and that's when solar eclipses can occur.
This also now correctly reframes your original screenshots: the Moon in both your images was on the far side (behind Earth, away from Sun) — meaning they should be Full Moon, not New Moon as I'd claimed. But the real-world data confirmed June 18, 2026 was a thin Waxing Crescent, not Full. So something is still inconsistent — likely the visual "far/near" judgment from the 2D projection in that simulator image is harder to read directly than I was treating it, since perspective/orbital tilt can make the near/far distinction visually ambiguous in that particular rendering.
Me:
So, does full moon happen due to the enormity of the size of the sun compared to earth, and sunlight reaches moon although it is on the far side of the earth?
Claude:
Yes — exactly right, and this is the piece that resolves any lingering geometric worry.
Why Earth doesn't block sunlight from reaching the "far side" Moon
The Sun is enormous compared to Earth — about 109 times Earth's diameter, and 149.6 million km away. Because of this huge size and distance, Earth's shadow is a long, narrow cone, not a wide blocking wall. Sunlight spreads out past Earth on all sides except directly within that narrow shadow-cone.
The Moon, even when it's roughly "behind" Earth from the Sun's perspective, is usually not inside that narrow shadow cone — it's off to the side of it, still bathed in direct sunlight. So the Moon's Earth-facing side gets fully lit by the Sun even though Earth is "in between" in a loose directional sense. That's Full Moon, happening almost every month, with sunlight reaching the Moon unobstructed.
So when does Earth's shadow actually hit the Moon?
Only when the alignment is precise enough that the Moon passes exactly through that narrow shadow cone — which requires the Moon to be both:
1. At Full Moon (Sun-Earth-Moon roughly aligned), and
2. Very close to a node (Rahu/Ketu) at that moment, so it's not off to the side of the ecliptic plane
This is exactly the bird's-wingtip-touching-the-ground condition from your earlier analogy. Most Full Moons, the Moon is a few degrees above or below the ecliptic (mid-flutter) and misses Earth's narrow shadow cone entirely, sailing past it just above or below — fully lit, ordinary Full Moon, no eclipse.
Only on the rare occasions when the wingtip grazes the ecliptic at the same moment as Full Moon does the Moon actually thread through that narrow cone of shadow — producing a lunar eclipse.
So you've now got the complete picture: Earth's smallness relative to the Sun is why eclipses are rare events rather than a monthly occurrence, despite Full Moon happening every month.
Would you like to actually scrub through simulator-style dates together (day by day) to visually locate the node crossing nearest August 28 and confirm the alignment?
Me:
Yes, that will give a good mental picture of day by day progression.
Claude:
Let's build this as a day-by-day scrubber so you can see the flutter and the Full Moon timing converge visually. I'll set it up so you can step through dates around late August 2026.Now I have real eclipse data to anchor the scrubber. Let me build an interactive day-by-day visualization where you can move a slider and watch the Moon's flutter (its position above/below the ecliptic) converge with the node exactly as the calendar approaches August 28, 2026.Drag the slider through the days, or hit Auto-play and watch it flow. Here's what to look for as you scrub from early August toward the 28th:
-The vertical guide line (light blue, dashed) shows the Moon's offset from the ecliptic — that's your ±5.14° flutter. Watch it shrink toward zero as you approach day 20.
- The "Eclipse condition" card flips to ✅ only when both things line up at once: the Moon is essentially Full and it's sitting right on the ecliptic line (within the node window).
- Jump to Eclipse snaps straight to August 28 so you can see the convergence instantly, then scrub backward/forward from there to feel how narrow that window actually is — just a day or so on either side.
This is a simplified, illustrative model (sinusoidal approximation, not a JPL ephemeris), but the geometry and timing are tuned to match the real event: greatest eclipse occurs on 2026 Aug 28 at 04:14 TD, with the Moon in Aquarius, at the ascending node, and it's a partial lunar eclipse with umbral magnitude 0.93 — consistent with the Moon being very close to, but not perfectly centered on, the node-and-Full-Moon coincidence in the scrubber.
Try scrubbing slowly through days 18–22 and watch how quickly the "✅ Both met" state appears and disappears — that narrow window is exactly the ±1 day estimate from the 11–12° eclipse limit.
Me:
Got it thanks.
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