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The Spider Stellar Engine: a Fully Steerable Extraterrestrial Design? (2411.05038v1)

Published 6 Nov 2024 in astro-ph.HE

Abstract: A long-lived civilization will inevitably have to migrate towards a nearby star as its home star runs out of nuclear fuel. One way to achieve such a migration is by transforming its star into a stellar engine, and to control its motion in the galaxy. We first provide a brief overview of stellar engines and conclude that looking for technosignatures of stellar engines has taken two roads: on the observational side, hypervelocity stars have been the target of such searches, but without good candidates. On the theoretical side, stellar engine concepts have been proposed but are poorly linked to observable technosignatures. Since about half the stars in our galaxy are in binary systems where life might develop too, we introduce a model of a binary stellar engine. We propose mechanisms for acceleration, deceleration, steering in the orbital plane and outside of the orbital plane. We apply the model to candidate systems, spider pulsars, which are binary stars composed of one millisecond pulsar and a very low-mass companion star that is heavily irradiated by the pulsar wind. We discuss potential signatures of acceleration, deceleration, steering, as well as maneuvers such as gravitational assists or captures. Keywords: Pulsars: Spiders, Technosignatures, Stellar engine, Interstellar travel

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Summary

  • The paper proposes the Spider Stellar Engine, a novel concept for interstellar migration that leverages binary star systems, particularly spider pulsars, as steerable engines.
  • The model details potential propulsion mechanisms using pulsar wind and magnetic manipulation, requiring precise orbital maneuvers within the binary system to achieve acceleration and steering.
  • The research offers testable hypotheses for SETI, suggesting that observable anomalies in pulsar velocity and behavior could serve as technosignatures of such cosmic-scale engineering.

The Spider Stellar Engine: A Novel Approach to Extraterrestrial Stellar Migration

The paper presented by Clément Vidal explores the concept of a "Spider Stellar Engine" as an innovative mechanism for interstellar migration of civilizations. In the context of long-lived civilizations needing to relocate as their home star exhausts its nuclear fuel, Vidal proposes a design leveraging binary star systems to transform into steerable stellar engines. This exploration advances the discourse on stellar engines by integrating binary systems and specifically applying concepts to "spider pulsars"—millisecond pulsars paired with low-mass companions.

Overview of Stellar Engines

Stellar engines have long been a speculative avenue in the discussion of alien technosignatures. Traditionally, these designs focus on moving singular stars, but Vidal's paper introduces the novelty of binary systems into this paradigm. A binary stellar engine inherently presents different dynamics due to its orbital nature, involving significant mass (more than ~1 M☉). Vidal surveys prior models, highlighting the limitations in linking these theoretical frameworks to observable technosignatures and sets the stage for the Spider Stellar Engine model.

Binary Stellar Engine Model

Vidal's model postulates mechanisms for acceleration, deceleration, and steering, contextualized within the "spider pulsars." These binary stars consist of a millisecond pulsar and a low-mass star heavily irradiated by the pulsar wind—often categorized as either redbacks or black widows based on companion mass. The model indicates techniques such as pulsed bursts of thrust at strategic orbital positions, leveraging radiation and magnetic manipulation to achieve propulsion. Numerical estimates show the feasibility of achieving significant velocities with proposed thrusting techniques.

The model stands out in its consideration of the binary configuration, where operations are constrained by the orbital mechanics, demanding well-timed manoeuvres for acceleration and course alteration. It substantially expands the conceptual space for stellar engines by making it applicable to a prevalent star system architecture—binaries constituting roughly half of all galactic star systems.

Signatures and Technosignatures

The paper makes a bold prediction that spider pulsars could be in action as stellar engines today, offering testable hypotheses for technosignature searches. These include distinct movement patterns, potentially altered spin axes, and propulsion signatures observable through telescopes. Vidal approaches the phenomena of pulsar wind acceleration and its potential for exerting the necessary escape velocities to eject mass from the companion in enabling the desired stellar propulsion.

The observational data, while sparse on ideal candidates, suggests potential avenues for further paper and verification. Vidal points out that anomalies in pulsar velocity and behaviors, such as change in proper motion and alignments, might be indicative of such engineered propulsion efforts.

Implications and Future Directions

The practical implications of this model are significant for the Search for Extraterrestrial Intelligence (SETI), providing a framework for identifying advanced engineering on a cosmic scale. It extends the class of technosignatures possibly detectible with modern astrophysical tools and suggests that our current observational datasets might already contain such signatures.

Theoretically, the paper enriches the discourse on the capabilities necessary for an interstellar migration strategy leveraging indigenous stellar bodies. It speculates on sophisticated manipulation of binary dynamics, positing a higher level of control and energy economy for a migrating civilization.

Looking ahead, the research calls for more refined models to predict technosignatures under varied stellar and companion configurations, offering a fertile ground for both theoretical exploration and observational follow-up.

In conclusion, Vidal's "Spider Stellar Engine" extends the conversation on stellar engines by marrying it with binary dynamics and focusing on realistic, observable signatures. As our capability to observe and interpret stellar phenomena matures, such models could provide essential frameworks in decoding potential cosmic-scale engineering.

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