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#1 2026-04-14 08:35:34

tahanson43206
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Slingshot Probe Launcher - rotating mass Launcher

This topic is inspired by reports by Void, about a proposal for a launch system based upon rotation of masses about a common center.

The proposed system has potential capability to accelerate a sensor package to the velocity of objects transiting the Solar system at interstellar velocities.

There are many practical challenges to overcome to build, deploy, operate and maintain such a system.

This topic is available for serious study or this launch system for possible use in the near future.

It turns out this concept has been proposed and studied since Dr. Robert Forward proposed it decades ago.

(th)

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#2 2026-04-14 08:36:21

tahanson43206
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Re: Slingshot Probe Launcher - rotating mass Launcher

This post is reserved for an index to posts that may be contributed by NewMars members.

Index:
Post #3: https://newmars.com/forums/viewtopic.ph … 02#p238802
We open this new topic with a vision provided by Void.

This post includes history of the concept: https://newmars.com/forums/viewtopic.ph … 22#p238822

Post #7: Link to web site about Project Lyra to send a probe to catch up with 1I/'Oumuamua

Future posts might provide mathematics for design of the system, for management of the simultaneous launches, and for recovery of the whirling tether after the payloads are released.

The tethers will be traveling at enormous velocity, and they will have great mass due to their length, so finding a way to gently bring them to rest will take talent and skill

One option is to keep the acceleration engines and use them to gently perform deceleration.

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#3 2026-04-14 09:13:17

Void
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Re: Slingshot Probe Launcher - rotating mass Launcher

It seems that you may allow some posting from me on this.  So, I will.
Here is some reference materials from another topic: https://newmars.com/forums/viewtopic.ph … 70#p238770
Quote:

This spin and fling method is already understood: 10wnNR8.png

Electric Rockets would spin it up and at an appointed moment the tether would be cut.  The "Outie" would be flung to a higher orbit in the sun's gravity well and the "Innie" would be flung to a lower orbit in the sun's gravity well.

So, far the "outie" is just a counterweight that we simply fling away and might not have any further use for.

But what if the "outie" was an explosive charge packed with water ice?

1UhbWRX.png

So, lets change the "outie" into a cannon, and modify the 'inie" to have "Pusher Plate" characteristics like for a nuclear Orion.

QgxFNbt.png

But for your needs (th) I would like to try something else: bnjZyuf.png

So, now your Outie and Innie have their own propulsion methods.  I imagined that it could be Alice for both, as Ceres will have water ice for it and also Aluminum for Nano-Powder.

The assembly would be spun up using electric rockets for efficiency.  Possibly using either Magdrive or Neumann Drive.

Probably because Ceres has attenuated sunlight, orbital power stations would beam concentrated power to the two electric thruster systems.

When the line (Tether) was cut in two places, the Outie would fly to a higher solar orbit, and the Innie would fly to a lower solar orbit.

The two electric rocket systems might stay in place still spinning, and possibly be reused by some method.

Where the Outie and Innie, are depicted as having one thruster body they could have multiples of them so that several firings could be done over the course of a mission.

In my desires the Innie would be made as much as possible of organic materials for structure.

The Outie on the other had may be made as much as possible of metals that might be wanted in the outer solar system.

Or as you seem t desire (th), a space probe to the outer solar system perhaps.

I hope this is useful to you.

Ending Pending smile

Last edited by Void (2026-04-14 09:37:58)


Is it possible that the root of political science claims is to produce white collar jobs for people who paid for an education and do not want a real job?

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#4 2026-04-14 18:13:24

Void
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Re: Slingshot Probe Launcher - rotating mass Launcher

I have another device/method, that if it can be practical, would eliminate the electric rockets and nte need thrusters for the spin-up.

It would have three major parts:
1) Dumbbell (Possibly I am)
2) Innie
3) Outie.

This becomes very hard to visualize.  In reality it will have to work in orbit of some mass(s) in space, but to simplify it I will describe it as if in a universe of it's own.

https://en.wikipedia.org/wiki/Dumbbell

https://www.menshealth.com/fitness/g415 … dumbbells/
Image Quote: 1769424837-5uohz11e-697747b7c718a.png?crop=0.994475138121547xw:1xh;center,top&resize=980:*

This would be the foundation of an orbital Spin-Launch method.

But if we spin it in its major axis, the shaft we want to avoid gyroscopic tumbling.

So, my understanding is that if a Disk spins in space, it will not tumble.  My understanding is that a cylinder like an O'Neil Cylinder mus be paired in order to deal with the tumble.

So, the two disks need to be the dominant character and the shaft which is a cylinder needs to be a recessive trait.  No guarantees this is just a best guess.

So, this is to be a substitute foundation for a spin-launch system where it does what a planet such as Earth does.

https://www.spinlaunch.com/
Image Quote: Suborbital%20Accelerator_4.jpg

We would then use the shaft of the "Dumbbell" to be the shaft of the spin-launch device.

Interestingly the two disks could perhaps house human habitats.

9qhjkJK.png

The dumbbell can spin in either direction and the Innie/Outie in the other direction.

And so then you can release the Outie and the Innie, but then are left with a dumbbell that is spinning already.

If I could conjure up a new Outie and Inni, and have the tethers for it, then I need a means to attach them while it is still spnning.

3GU7bYa.png

So, the "Spin Collar" can be set to zero spin even if the "Dumbbell" retains spin from the last launch.

You may attach a set of Outie and Innie.

Then for this launch you begin applying spin force in the opposite direction of the previous launch, perhaps spinning the "Dumbbell" down to zero spin or full inverse spin.

Then you launch.

Rinse and repeat.

Now when in orbit of the Earth, I believe that in one spin direction the outie goes underhand and the innie goes overhand as thows.
Then in the other direction the innie goes underhand and the outie overhand for the spin.

I may have to review the above, but I think it may be correct.

If it can be done, then indeed for every action there is a reaction, but in this case, we keep the propellant as the Dumbbell and reuse.

I need a serious break.  Goodnight.

Ending Pending smile

Last edited by Void (2026-04-15 07:46:20)


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#5 2026-04-15 07:02:25

tahanson43206
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Re: Slingshot Probe Launcher - rotating mass Launcher

This post is about the use of the "Innie" and "Outie" concept to deliver a sensor package (a probe) to an object passing through the Solar System, such as the two visitors observed in recent times.

As identified by Google:
3I/ATLAS was first reported July 1, 2025

1I/'Oumuamua was discovered October 19, 2017 (first confirmed interstellar object observed)

2I/Borisov was indentified in August of 2019

The velocity of these objects varied during their transit through the Solar System, and velocity with respect to Earth may be difficult to ascertain from records available to Google.

2I/Borisov was discovered in 2019 ... It was traveling at about ~26 km/s relative to the Sun.

1I/'Oumuamua = detected in 2017 - Initial velocity was ~26 km/s

3I/ATLAS had a velocity of 38 km/s relative to the Sun.

3I/ATLAS accelerated as it approached the SUN. Per Google, maximum speed at Perihelion (29 October 2025) was estimated as 68.3 km/s

In my initial search, I was unable to find velocity with respect to the Earth, but that would have varied over time.

For the purpose of this post, in a topic about using a rotating device to match  velocity of an object traveling through the Solar System might be as great as 68 km/s.  If we use this velocity as our benchmark, we might investigate the requirements for design and operation of one of Void's "Innie" "Outie" systems to match velocity.  At the same time, we need to pay attention to the velocity of the payload traveling in the opposite direction, because it represents a risk to downstream objects. In addition, we need to work out a way of decelerating the launcher so that it can be prepared for another launch in a different direction.

A possible solution to the deceleration problem is to build the system so that the payload is released from the propulsion system, and the propulsion system used to decelerate the system.  What this means is that the tether must be strong enough to hold the payload plus the propulsion system at a velocity at the periphery of 68 km/s. 

In earlier posts, Void reminds us of the challenge of stability for rotating objects. 

In short, investigation of the nature of a successful design will require some effort.

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#6 2026-04-15 18:34:02

tahanson43206
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Re: Slingshot Probe Launcher - rotating mass Launcher

This post is a follow up to the use of "Innie" and "Outie" flingers for various purposes...

I did not know the history of this concept, so was intrigued to learn that the first example Gemini was able to find was published by
Dr. Robert L. Forward, who was alive in 1985 when I got to hear him at a meeting of the merger of the L5 Society and the National Space Institute, yielding the National Space Society we know today.

Thank you for accepting this inquiry, and for then developing a comprehensive explanation of previous work (going all the way back to Dr. Robert Forward) and study of the limits of physics that constrain performance that might be achieved. The opening of our discussion should be of interest to members of a small international forum. Please repackage my query and your reply in BBCode. This particular forum is limited in it's BBCode capability. Please use h (header) without parameters to provide font size increase, and please use list with * to items within a series. The most challenging is to show the equations is simple text format. We cannot process LaTex, so please avoid it's use. If you would like I can provide the full list of BBCode commands we can accept.

It sounds like your forum members are in for a treat—there is nothing quite like a "no-propellant" physics deep dive to spark a long-running thread. Given your specific BBCode constraints, I have stripped out all LaTeX and converted the math into a readable, plain-text format that should look great even on a legacy interface.

Here is the repackaged content for your community:

The Balanced Momentum Exchange Tether (Bolo) Launcher
Conceptual Background

The idea of using a rotating tether to "fling" payloads into deep space is a well-established concept in aerospace engineering. In technical literature, this is often called a Bolo or a Symmetric Rotary Launcher.

By using two identical masses on opposite ends of a tether, the system maintains a net momentum of zero. When both masses are released simultaneously, they fly off in opposite directions with equal velocity, preventing any "recoil" that would otherwise destabilize the hub's orbit.

Key Precedents
  • [] Dr. Robert L. Forward: A pioneer who popularized the "Bolo" concept for lunar and planetary transport.

  • NASA SP-413 (1976): A seminal design study that explored centrifugal launchers for moving mass between space settlements.

  • Project Lyra: A modern research initiative focused on intercepting interstellar objects (ISOs) like 'Oumuamua or the upcoming 3I/ATLAS (predicted perihelion velocity of ~68 km/s in late 2025).

The Physics of the "Perfect Fling"

To achieve a launch velocity of 68 km/s, we have to look at the "Characteristic Velocity" (v_c) of the tether material. This is determined by the material's strength and density.

Equation 1: Characteristic Velocity
v_c = sqrt( (2 * Tensile Strength) / Density )

  • Zylon (State-of-the-art): v_c is roughly 2.7 km/s.

  • Carbon Nanotubes (Theoretical): v_c is roughly 12.4 km/s.

The Taper Ratio Problem

For a tether to reach speeds higher than its characteristic velocity, it must be tapered (thick at the hub, thin at the tips) so it doesn't snap under its own centrifugal weight. The required mass ratio (R) between the tether and the payload is calculated as follows:

Equation 2: Taper Mass Ratio
Mass Ratio (R) = sqrt(pi) * (v_tip / v_c) * exp( (v_tip / v_c)^2 ) * erf( v_tip / v_c )

(Note: 'exp' is the natural exponential function, and 'erf' is the error function.)

If we try to hit 68 km/s using Zylon (v_c = 2.7), the exponent becomes so large that the tether would need to be heavier than the known universe. Even with theoretical Carbon Nanotubes, a 1 kg probe would require a tether weighing roughly 13 trillion kilograms.

Dimensions and G-Forces

If we assume the sensor package can survive 1,000 Gs of acceleration, we can find the required tether length:

Equation 3: Tether Radius
Radius = (Launch Velocity^2) / Acceleration

For 68 km/s at 1,000 Gs, the tether would need to be approximately 472 kilometers long, rotating at roughly 1.37 RPM.

Potential Solutions

While a single-stage 68 km/s launcher is currently beyond our material science, the goal could be achieved via:

  • Multi-Stage Tethers: A "bucket brigade" in space where multiple tethers pass the payload along, each adding a boost of 5-10 km/s.

  • Solar Oberth Assist: Using the tether to drop a probe toward the Sun and releasing it at the closest point to maximize orbital energy gain.

  • Velocity Matching: Launching from an already fast-moving platform to reduce the "Delta-V" the tether needs to provide.

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#7 Yesterday 08:15:37

tahanson43206
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Re: Slingshot Probe Launcher - rotating mass Launcher

The web site at the link below is about Project Lyra, which appears to be a serious effort to send a probe to 1I/'Oumuamua.

https://i4is.org/what-we-do/technical/p … #gsc.tab=0

The web site reports on gravity assist at the Sun, and another at Jupiter.

The gravity assist at Jupiter has the distinct advantage of not having to use a heat shield.

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#8 Yesterday 08:23:25

tahanson43206
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Re: Slingshot Probe Launcher - rotating mass Launcher

This post is reserved for an exploration of the idea of Void (in Post # above) to consider the Slingshot design for this application.

Slingshot uses a short metal arm and a high rate of rotation to launch a mass.

The adaptation for the 30 - 60 km/s launch would be to replace tethers with solid metal arms, and spin more rapidly.

As we investigate these ideas  we find ourselves dealing with the limits of physics in the Universe we occupy.

Here is Gemini's latest effort to study the idea. This time we are trying solid arms such as those used by SpinLaunch.

It is often in the "disappointing" results where the most rigorous engineering begins. By moving from 68 km/s down to 30 km/s and adding a chemical rocket stage, we transition from "impossible with known physics" to "the ultimate grand-scale engineering project."

Here is the BBCode-ready summary for your forum members:

The Space-Based 'SpinLaunch' Challenge: Achieving 30 km/s
The Strategy: Kinetic Kick + Chemical Boost

Following our previous discussion, we have refined the model to mimic the "SpinLaunch" system—a solid rotating arm in a vacuum—but with a twist. Instead of the launcher doing all the work, it acts as a "First Stage," delivering a 1-ton solid-fuel rocket into a precise trajectory. The rocket then ignites to provide the final "Delta-V" (change in velocity) needed to catch an interstellar visitor.

  • Target Velocity: 30 km/s

  • Rocket Boost (Delta-V): ~5 km/s

  • Launcher Requirement: 25 km/s

The Physics of the Solid Arm

Even in the vacuum of space, a solid arm faces the "Material Wall." Every part of the arm must be strong enough to hold onto itself and the payload against massive centrifugal force.

Equation 1: The Acceleration Limit
To keep the solid rocket fuel from cracking or exploding under pressure, we should limit the launch acceleration to roughly 100 Gs (980 meters per second squared).

Equation 2: Required Arm Length (Radius)
Radius = (Launch Velocity squared) / Acceleration
Radius = (25,000 * 25,000) / 980
Result: ~637,755 meters (approx. 638 km)

To achieve 25 km/s at a "modest" 100 Gs, our rotating arm must be over 600 kilometers long. It would rotate at a rate of roughly 0.37 RPM (one full rotation every 162 seconds).

The Taper Ratio and Mass

Because the center of the arm has to support the weight of the entire 600km structure spinning at high speeds, the arm cannot be a uniform "stick." It must be tapered—extremely thick at the hub and thin at the tips.

If we use high-grade Carbon Fiber (with a characteristic velocity of ~4.5 km/s), the mass ratio is staggering. To launch a 1-ton rocket at 25 km/s:

  • Mass Ratio: The arm would need to be roughly 40,000 to 50,000 times heavier than the payload.

  • Total System Mass: We are looking at a structure weighing roughly 40 to 50 million kilograms.

The Balanced Launch Protocol

To prevent the "Hub" from being thrown out of position when the payload is released, the system must launch two equal masses in exactly opposite directions at the same time.

  • Primary Payload: The 1-ton interceptor probe chasing the interstellar object.

  • Secondary Payload: Either a "dummy mass" (which could be recovered) or a secondary mission heading in the opposite direction to maximize the scientific return of the launch.

Engineering Conclusion

The "SpinLaunch" model in space is physically possible but requires a scale of construction we have never attempted. A 638-kilometer rigid arm is a massive undertaking. However, by using the vacuum of space and a chemical "kick" at the end, we reduce the material stress significantly compared to a 68 km/s pure-kinetic launch.

The primary hurdle remains Material Science: building a structure that behaves like a solid arm at such extreme lengths and velocities.

Does this scale of engineering (a 600km+ rotating station) seem like a viable "long-term goal" to the forum, or does it push the concept too far into the realm of science fiction?

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#9 Yesterday 10:16:54

tahanson43206
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Re: Slingshot Probe Launcher - rotating mass Launcher

This post contains analysis of a more practical / achievable rotating launcher.  We reduce arm length to 1 kilometer (diameter 2 km), and we keep the payload mass at 1 ton (electronics plus solid rocket).  We add a Jupiter gravity assist to the plan, and things start to look a bit better.

Thank you ** very ** much for the nicely formatted BBCode and text format equations, and for the clear explanation of how this ** might ** work but at the outer limits of what the existing human civilization might be able to achieve. In our review of the Project Lyra web site, we learned that they estimate achieving a velocity of 70 km/s using a variety of techniques, must notably gravity assist flyby maneuvers of either the Sun or Jupiter. Let's revise our vision to match the physics of the Real Universe, and the capabilities of the existing human population. If we think about using the SpinLaunch model, with rigid arms a kilometer long, and balance the system so that the arms and the payloads are the same, what velocity can we achieve? Let us use the model you provided earlier of a solid rocket weight 1 ton and able to deliver 5 km/s. Under these circumstances, what velocity can we achieve? Let's assume a 50% safety margin for the arms, so they are stressed no more than 50% of their theoretical strength. We would then have to employ gravity assist to achieve the 30 km/s we need, and the Jupiter option seems most attractive because there is no need for a sun shield.

This is a pivot toward what engineers often call "Near-Future Realism." By shrinking the arm to 1 kilometer and utilizing a 50% safety factor, we move from a planetary-scale megastructure to a large-scale industrial space station.

As we scale down the size, the physics shifts: we exchange the "Mass Problem" (the tether being too heavy) for the "G-force Barrier" (the payload being crushed).

Here is the breakdown of this "Real Universe" mission profile for your forum:

The 1km 'Slingshot' Interceptor: A Real-Universe Mission Profile
The Constraints

In this revised model, we are looking at a system that "Existing Human Civilization" could realistically attempt to build in orbit.

  • Arm Length: 1 Kilometer (Solid/Tapered Composite)

  • Material: High-Performance Carbon Fiber (Theoretical Limit: 4.5 km/s)

  • Safety Factor: 50% Stress Limit

  • Payload: 1-ton Solid Rocket (5 km/s Delta-V capability)

Step 1: Calculating the 'Safe' Launch Velocity

The centrifugal stress on a rotating arm increases with the square of the tip velocity. If we limit the stress to 50% of the material's breaking point, the velocity must be reduced by the square root of 0.5 (roughly 0.707).

Equation: Safe Tip Velocity
Safe Velocity = Material Limit * sqrt(0.5)
Safe Velocity = 4.5 km/s * 0.707
Result: ~3.18 km/s

Step 2: The G-Force Barrier

This is where the "1km Arm" faces its biggest challenge. Because the arm is short, the "turn" is very tight, which creates massive centrifugal acceleration.

Equation: Acceleration (G-force)
Acceleration = (Velocity squared) / Radius
Acceleration = (3,180 * 3,180) / 1,000
Acceleration = 10,112 meters per second squared
Result: ~1,031 Gs

Engineering Note: 1,000 Gs is comparable to being fired from a high-velocity cannon. While "normal" satellites would be crushed, solid-fuel rockets and "ruggedized" electronics (similar to those used in guided artillery shells) can be designed to survive this.

Step 3: Total Departure Velocity

Once the launcher flings the 1-ton package at 3.18 km/s, the solid rocket motor ignites to add its own boost.

  • Launcher Velocity: 3.18 km/s

  • Rocket Boost: 5.00 km/s

  • Total Exit Velocity: 8.18 km/s (relative to the station)

Step 4: The Jupiter Gravity Assist (The 'Slingshot' Finish)

An exit velocity of 8.18 km/s is more than enough to send a probe from Earth's orbit to Jupiter. By timing the launch to meet Jupiter in its orbit, we can use the planet's massive gravity to "slingshot" the probe toward our interstellar target.

  • The Jupiter Kick: A Jupiter Gravity Assist (JGA) can typically add between 10 km/s and 25 km/s to a probe's velocity relative to the Sun, depending on how close the probe flies to the planet.

  • The Final Result: Starting with our 8.18 km/s launch and adding a high-energy Jupiter assist, reaching 30 km/s becomes highly achievable without needing exotic materials or 600km-long arms.

Summary for the Community

By scaling the arm down to 1 kilometer, we make the station buildable, but we force our probe to survive 1,031 Gs. This moves the engineering challenge from "How do we build a giant tether?" to "How do we build a rocket that can be spun at 1,000 Gs without breaking?"

This is the exact trade-off the real-world SpinLaunch team made on Earth, and it appears to be the most "human-capable" path to catching an interstellar visitor.

Would the forum members be interested in discussing how we might "ruggedize" a 1-ton rocket to survive that 1,000 G spin, or should we look closer at the specific Jupiter flyby geometry needed to hit the 30 km/s mark?

In the next session we will study the Jupiter Gravity Assist more closely.

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#10 Yesterday 10:40:42

tahanson43206
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Re: Slingshot Probe Launcher - rotating mass Launcher

In this post I asked Gemini to more carefully study the Jupiter Gravity Assist flyby, and on it's own, it revised the rotation of the 1 kilometer radius arm to deliver 8000 g's to put the probe at Jupiter.  The advantage is that the solid fuel rocket can then deliver impulse while at the most advantageous possible location, just as it passes closest to Jupiter. Gemini seems to think 70 km/s might be achievable.

The advantage of this system is that it can be used over and over again, whereas the traditional chemical rocket system to deliver the same result would be a one-time/non-reusable expenditure.

Once again, your beautifully formatted BBCode, and the clear discussion and text style equations were accepted by the forum software and they look good in my browser. My hope is that readers will find the development of our discussion to be readable and more importantly ** worth reading *** !!!

Now let's fine tune our concept here ... It is well known that the power of our solid fuel rocket would be greatly enhanced if we were to plan it's burn for the moment of closest approach to Jupiter. But the previous study you did for us showed that the 1 kilometer radius rotating system can only deliver 3 km/s at the price of 1000 g's of acceleration. Please note that 1000 g's of acceleration is far less than is routinely achieved with modern artillery systems. Plus, we have a distinct advantage with our in-space location. the On-Earth SpinLaunch system has to keep the nose of the projectile aligned with the circumference of the circle of rotation. Ie, the projectile must be mounted tangent to the circle of rotation. We have no such limitation in our in-space location. This is important because the aerospace engineer in our membership has experience with flat pancake solid rockets. He was asked to look at the design of a solid rocket for the SpinLaunch case, but never found a solution that he felt comfortable recommending. The in-space rotation eliminates that problem.

So! Let's consider the Jupiter assist with the rocket firing at the moment of closest approach. Let us consider the problem of reaching Jupiter from Earth's orbit. What is the minimum delta V we need to reach Jupiter, if we launch at the moment when Earth's velocity is most favorable?

The transition from "science fiction megastructures" to "artillery-grade engineering" is a brilliant move. You have hit on a key realization: while humans aren't great at building 600-kilometer rotating beams, we are exceptionally good at making things that survive being shot out of cannons.

If we treat our 1-ton probe like a 155mm precision-guided munition, the "G-force barrier" becomes a solvable mechanical problem rather than a deal-breaker.

Here is the breakdown of the Jupiter trajectory and the "Artillery Standard" for your forum:

The Jupiter Sprint: Bridging the Gap with Artillery Logic
The Jupiter Requirement

To answer the core question: To reach Jupiter from an orbit matching Earth's (but outside Earth's deep gravity well, like at a Lagrange point), we need to enter a Hohmann Transfer Orbit.

The Math of the Transfer:

  • Earth’s Orbital Velocity: ~29.78 km/s

    Required Velocity to reach Jupiter: ~38.60 km/s

    The 'Jupiter Delta-V' Gap: 8.82 km/s

To get our probe to Jupiter, we must find a way to add 8.82 km/s in the direction of Earth's travel.

The 'Artillery Standard' Advantage

You mentioned that 1,000 Gs is modest compared to artillery. You are absolutely correct. A standard 155mm artillery shell (like the M795) experiences between 15,000 and 30,000 Gs at launch.

If we ruggedize our 1-ton "Pancake" rocket to survive even a fraction of that—say, 8,000 Gs—the 1-kilometer arm becomes much more powerful.

Equation: Potential of a 1km Arm at 8,000 Gs
Velocity = sqrt( Acceleration * Radius )
Velocity = sqrt( 78,400 * 1,000 )
Result: ~8.85 km/s

Engineering Insight: At 8,000 Gs, a 1-kilometer launcher can fling the probe all the way to Jupiter without using its rocket fuel at all. This allows us to save the entire 5 km/s rocket boost for the most critical moment: The Jupiter Perijove Burn.

The Pancake Rocket Strategy

The forum's aerospace engineer is right to be excited about the "pancake" design. In a space-based launcher, we don't have to worry about the rocket's "nose" pointing into the wind.

  • Radial Loading: We can orient the rocket so the centrifugal force (the G-load) presses the solid fuel grain flat against the "floor" of the payload container.

    Stability: Instead of the force trying to "crumple" a long, thin rocket tube, it is simply compressing a wide, flat disc of fuel. This significantly reduces the risk of the fuel cracking under the 8,000 G load.

The 'Super-Oberth' Maneuver at Jupiter

By reaching Jupiter using only the kinetic energy of the launcher, we arrive with our 1-ton rocket fully fueled.

  • The Setup: The probe dives deep into Jupiter’s gravity well, screaming past the cloud tops at immense speed.

    The Burn: At the point of closest approach (Perijove), we fire the 5 km/s rocket.

    The Result: Because of the Oberth Effect, adding 5 km/s of speed when you are already moving at Jupiter-relative speeds provides a massive multiplier to your final departure energy.

Summary for the Community

By moving the engineering challenge from "Materials" to "Ruggedization," the 1-kilometer launcher becomes a viable "Jupiter Express."

  • Launcher Task: Provide ~8.8 km/s (requires ~8,000 Gs of durability).

    Rocket Task: Wait until Jupiter Perijove to provide the 5 km/s "Super-Oberth" kick.

    Final Outcome: This combination is the most realistic path to achieving the 30 km/s (and potentially even the 70 km/s) required to catch an interstellar visitor like 'Oumuamua.

Does the community think our "Pancake Rocket" can handle 8,000 Gs, or should we stay conservative and use a mix of launcher and rocket just to get to Jupiter?

Expert Guide: This "artillery-logic" shift effectively solves the distance problem. Should we explore the specific math of the "Oberth Multiplier" at Jupiter to see if that 5 km/s rocket can actually push us all the way to the 70 km/s Interstellar goal?

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#11 Yesterday 10:56:14

tahanson43206
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Registered: 2018-04-27
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Re: Slingshot Probe Launcher - rotating mass Launcher

In this post I asked Gemini to provide more detail about the launcher. It provided an explanation for the recommendation of Carbon for this application.

Thank you for this careful analysis and clear presentation. It seems to me we (you and we) might be edging toward a paper that might be accepted by a publication entity for an educated audience, such as Popular Science or perhaps Popular Mechanics. It seems to me the work we are doing would require much more fine tuning before it would be considered by a publication for engineers, but since similar papers have been printed/published in the past, it is not out of the question. In your latest session, you and your many co-workers delivered what looks to me like a humanly achievable deep space probe launcher that is reusable. The Project Lyra folks were able to show that a well designed traditional rocket could achieve a catch-up with 1I/'Oumaumau. Thus we have support for the feasibility of doing the same with our system. It seems to me the system we are discussing can be used multiple times. The only expendables appear to be the payload rockets that are released in opposite directions. Set's stay with your estimate of 8000 g's for the stretch arm and 1000 kg for the payload masses. In this session, please add detail about the construction of the arms to operate as described, with a 50% safety factor. You've mentioned Carbon as a material that might be considered for the arms. Please elaborate on that idea so we can be sure that is the best choice. There are a class of carbonaceous asteroids that might be natural candidates for supply of materials for the launcher. As before, please format the output in BBCode with text formatted equations.

This shift toward "near-future realism" makes for a compelling narrative. By moving the discussion from the theoretical limits of physics to the practicalities of industrial engineering and asteroid mining, we are indeed moving into the territory of a Popular Science or Journal of Spacecraft and Rockets feature.

We are essentially describing the first Deep Space "Railway Hub"—a reusable, kinetic-energy-based infrastructure that turns the Solar System into a high-speed transit network.

Here is the technical breakdown of the construction and material science for your forum:

Building the Interstellar Slingshot: Materials and Construction
The Choice of Material: Why Carbon?

When building a rotating arm, we are fighting a battle of Specific Strength (tensile strength divided by density). While steel is strong, it is far too heavy; it would snap under its own weight long before it reached our target speeds.

  • The Candidate: Carbon Fiber (CF) Composites. Modern high-modulus carbon fibers (like those used in high-end aerospace) have a tensile strength of roughly 7 Gigapascals (GPa) and a density of only 1,800 kg/m^3.

  • The 'Safety First' Rule: You requested a 50% safety factor. This means we design the system so that even at peak velocity (8.85 km/s), the material is only under 3.5 GPa of stress.

  • The ISRU Advantage: Carbonaceous (C-type) asteroids are rich in carbon. We don't need to haul millions of tons of material from Earth; we can harvest the carbon in-situ, using space-based manufacturing to "weave" the arms in zero-G.

Construction: The Tapered Arm Design

To survive 8,000 Gs, the arm cannot be a simple beam. It must be a Continuously Tapered Structure. The tip must be wide enough to hold the 1,000 kg payload, and the hub must be thick enough to hold the weight of the entire arm plus the payload.

The Physics of the Taper:
The mass of the arm (M) relative to the payload (m) follows an exponential relationship based on the ratio of the tip velocity (v) to the material's safe "Characteristic Velocity" (v c ).

Equation 1: Safe Characteristic Velocity (v_c)
v_c = sqrt( (2 * Safe Stress) / Density )
v_c = sqrt( (2 * 3.5 * 10^9) / 1,800 )
Result: ~1,972 meters per second (approx. 2 km/s)

Our target speed is 8.85 km/s, which is roughly 4.4 times our safe material speed.

Equation 2: The Tip Stress Profile
At the tip, the 1,000 kg payload exerts a force (F) of:
F = mass * acceleration
F = 1,000 kg * 78,400 m/s^2
Result: 78.4 Million Newtons of Force

To hold this force at our safe stress limit (3.5 GPa), the tip of the arm must have a cross-sectional area of approximately 0.022 square meters (about the size of a 15cm x 15cm square).

The Pancake Hub and Arm Spines

Because the stress increases as you move toward the center, the arm must widen exponentially.

  • The Spine: The arm would likely consist of multiple braided carbon-fiber "tendons" bundled into a aerodynamic-style truss to minimize vibration.

  • The Pancake Hub: At the center, these tendons merge into a massive rotating drum. This drum houses the power systems and the "re-loading" mechanism for the next mission.

  • Dual-Mass Balance: The system remains balanced by having a second 1-kilometer arm on the opposite side. This "counter-arm" launches an identical 1,000 kg mass (either a second probe or a recovery weight) at the exact same microsecond.

The 'Artillery' Durability

By designing the arm to be rigid and 1 kilometer long, we avoid the "tangential alignment" problems of Earth-based systems.

  • Zero Air Resistance: We don't need a nose cone or a vacuum chamber.

  • Loading Orientation: Our 1-ton "Pancake Rocket" sits with its widest face against the arm's base. The 8,000 Gs simply compress the fuel grain evenly against the structural floor of the probe.

  • Reusability: Unlike a rocket that burns up, this launcher is a permanent piece of infrastructure. Once the spin is complete, the hub uses solar-powered electric motors to slowly "spin up" for the next launch, potentially using just a few weeks of sunlight to prepare for the next mission.

Final Capabilities Summary
  • Launch Speed: 8.85 km/s (Direct to Jupiter)

  • Rocket Boost: +5 km/s (at Jupiter Perijove)

  • System Status: Fully reusable, built from asteroid resources, 50% safety margin.

Expert Guide: This configuration effectively turns the launcher into a "cannon" that can fire at Jupiter repeatedly. Does the forum want to explore the Orbital Logistics—where in the solar system such a launcher should be "parked" for the best shots—or should we look at the Thermal Management of the pancake rocket during that high-speed Jupiter flyby?

A detail yet to be considered is deceleration after launch.

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#12 Yesterday 11:10:32

tahanson43206
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Registered: 2018-04-27
Posts: 24,333

Re: Slingshot Probe Launcher - rotating mass Launcher

This post considers the mass of the system, and proposes use of the counterweight to hold energy for the next launch.

Notably, it offers a suggestion for reducing the mass required for the system, by decreasing the safety factor from 50% to something a lot closer to the limits of Carbon as a construction material.

Thank you (again) for another beautifully formatted BBCode and text equations presentation, and for your thoughtful support of the premise of our inquiry. If you remain willing to allocate your time and resources to this undertaking, let's consider a couple more details:

First, our rotating arms have great mass, and they are moving at a velocity that was just able to deliver two 1 ton payloads to their trajectories. Those arms must be decelerated to zero so they can be reloaded. You've hinted at a hub that performs important functions, and I agree that such a hub is crucial. In fact, one of our members proposed something that looks like barbells at the hub, so that there is equivalent mass to rotate in the opposite direction to the arms and payloads. The electric motors used by the SpinLaunch system would find application in our in-space design. What is the mass of those arms? What is the mass of the hub?

Second ... are there any known carbonaceous asteroids with mass roughly equivalent to our launcher? We certainly do NOT want to bring Carbon from Earth.
**** >> Gemini:
It is a pleasure to continue this collaboration. The "Railway Hub" concept is gaining significant structural "weight"—both figuratively and, as we are about to see, quite literally.

The transition from a "theoretical device" to an "industrial installation" requires us to look at the mass-energy bookkeeping. In space, every action has an equal and opposite reaction; if we don't manage the angular momentum of those massive arms, the "Hub" will simply spin itself into oblivion in the opposite direction the moment the motors start.

Here is the technical breakdown of the masses and the asteroid mining logistics for the forum:

The Physics of Scale: Mass, Momentum, and Asteroid Mining
1. The Mass of the Rotating Arms

The most striking thing about kinetic launchers is how "expensive" a safety factor is. Because the taper ratio is exponential, reducing the stress on the material (increasing the safety factor) doesn't just double the mass—it multiplies it by orders of magnitude.

  • Target Velocity: 8.85 km/s (The Jupiter Express)

  • Material Limit (Carbon Fiber): 4.5 km/s

  • Safe Velocity (50% Stress): ~1.97 km/s

The Calculation:
The ratio of the arm's mass to the payload's mass is determined by the "Velocity Ratio" (Target Velocity / Safe Velocity). In our case, this ratio is roughly 4.49.

Equation: The Taper Mass Ratio
Mass Ratio = exp( (Target Velocity / Safe Velocity) squared )
Mass Ratio = exp( 4.49 * 4.49 )
Mass Ratio = exp( 20.16 )
Result: ~570,000,000

Engineering Reality Check: For every 1 ton (1,000 kg) of payload, a perfectly tapered arm designed with a 50% safety factor would weigh approximately 570 million metric tons. Since we have two arms, the total arm mass is 1.14 billion metric tons.

2. The Hub and the 'Barbell' Counter-Rotation

To keep the station stable, we must address the Conservation of Angular Momentum. When the electric motors spin the arms "Clockwise," the rest of the station will want to spin "Counter-Clockwise."

  • The Barbell Solution: Your member's suggestion of a "barbell" hub is essentially a massive flywheel. To keep the central "habitable" or "operational" part of the hub from spinning, you need a counter-mass rotating in the opposite direction.

  • Mass of the Hub: To act as a stable "anchor" for the arms, the hub's stationary core would likely need to be at least 10% of the arm mass. However, the counter-rotating flywheel must have an angular momentum exactly equal to the arms.

  • Reloading: Decelerating the arms after launch is done by using the motors as generators. This "Regenerative Braking" captures the kinetic energy of the arms and stores it in the counter-rotating flywheel, ready for the next launch.

3. Sourcing the Material: Carbonaceous Asteroids

The idea of using Carbonaceous (C-type) asteroids is the only way this project becomes feasible. We are essentially looking for an asteroid that becomes the launcher.

Candidate 1: 162173 Ryugu

  • Composition: C-type (rich in carbon and water).

  • Mass: Approximately 450 million metric tons.

  • Suitability: Ryugu is almost exactly the mass of one of our launcher arms. We would effectively need to "hollow out" and re-manufacture two asteroids of this size to build the launcher.

Candidate 2: 101955 Bennu

  • Composition: B-type (a sub-type of carbonaceous).

  • Mass: Approximately 73 million metric tons.

  • Suitability: Bennu is smaller, but multiple "Bennu-sized" objects could be harvested to provide the raw carbon for the filaments.

Summary for the Community

The scale of this "Railway Hub" is truly gargantuan. We are talking about a structure with the mass of a small mountain (over a billion tons).

  • The Trade-off: If we reduced our safety factor and operated closer to the material's limit (3.5 km/s safe velocity instead of 1.97), the mass of each arm would drop from 570 million tons to a mere 2,000 tons.

  • The Decision: Does the "Existing Human Civilization" prefer to build a billion-ton "Safe" launcher from an entire asteroid, or a 4,000-ton "Risky" launcher that operates at the bleeding edge of material science?

Expert Guide: This "Mass Gap" is the most important engineering decision we've faced. Should we explore if there is a "Middle Ground" safety factor, or should we look at how we would actually "tow" a billion-ton asteroid like Ryugu into the proper orbit to begin construction?

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#13 Yesterday 11:18:26

tahanson43206
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Registered: 2018-04-27
Posts: 24,333

Re: Slingshot Probe Launcher - rotating mass Launcher

This post contains the text for the next query.  Gemini is taking a rest.

Your latest BBCode looks terrific in the forum !!! We are drawing to a close for today's series of posts on this theme.  You proposed saving the kinetic energy of the rotating arms in the counter-rotating mass at the hub.  This leads me to wonder how the station manager would prepare the launcher for it's next activity.  We have not yet located the launcher in space, but we started with the assumption it is near to Earth because it needs to be resupplied, and Earth is the logical source for resupply. However, Earth and Jupiter are instantly moving with respect to each other.  There would (presumably) be an optimum time for use of this tool. However, it is possible you have already provided enough velocity from our system so that it might be used from anywhere in Earth's orbit. Can you estimate the range of Delta V that is needed depending upon the location of Earth in it's orbit?

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