Saturday, May 31, 2025

Payback (1999)

https://en.wikipedia.org/wiki/Payback_(1999_film) (Max)

https://en.wikipedia.org/wiki/The_Hunter_(Stark_novel) (1962) 

https://en.wikipedia.org/wiki/Donald_E._Westlake (1933-2008) (Richard Stark)

Parker (Stark novels character)



Donald E. Westlake (1933-2008) created two professional criminal characters who each starred in a long-running series: the relentless, hardboiled Parker (published under the pen name Richard Stark), and John Dortmunder, who featured in a more humorous series. Why?  (ChatGPT, 2025-6-1)


That’s a rich and revealing question, my friend—and one that cuts to the heart of Donald E. Westlake’s creative duality as a writer. Why did he create two professional criminals so different in tone and temperament—Parker and Dortmunder—and even choose to split his authorial identity between them?


Let’s explore this through psychological, literary, and market-conscious lenses.





🎭 

1. Duality of Temperament: The Shadow and the Trickster



Westlake once quipped that Parker was the man who never cracked a smile, while Dortmunder was the man who never caught a break.


  • Parker (as Richard Stark): Cold, efficient, ruthless, and mechanical. He never doubts himself, rarely hesitates, and treats crime as a job. He is the embodiment of pure will, almost existential in his detachment—think Camus’ The Stranger, but with guns.
  • Dortmunder: Neurotic, unlucky, perpetually one step behind disaster. His heists always go hilariously sideways. He represents the absurdity of trying to impose order on a chaotic world—a criminal Sisyphus pushing a safe up a stairwell.



In Jungian terms:


  • Parker is the Shadow—the suppressed, violent, streamlined force of pure id.
  • Dortmunder is the Trickster—the comedic, vulnerable reflection of human error.



Westlake was both.





✍️ 

2. Artistic Range and Narrative Freedom



Westlake was a master of genre who refused to be boxed in. Creating two distinct criminal series allowed him to:


  • Explore serious noir fatalism through Parker.
  • Channel his wry, satirical genius through Dortmunder.



He once said he started writing Parker novels when he was angry, and Dortmunder novels when he was bemused.


Each character allowed Westlake to flex a different voice:


  • Stark’s prose: spare, precise, ice-cold.
  • Westlake’s prose: conversational, ironic, chaotic.






🕶️ 

3. The Pen Name as Aesthetic Boundary



Why use the pen name Richard Stark for Parker?


  • To signal a different mood and literary contract to the reader.
  • Stark’s name echoed the tone: austere, unforgiving, stripped-down.
  • It gave Westlake a psychological space to write without sentiment, without the reader expecting jokes.



He once said that if Dortmunder attempted a Parker heist, it would fail. And if Parker were in a Dortmunder plot, he would kill everyone and walk away in five pages.





💰 

4. The Market: Genre Diversification



In the mid-20th century publishing world, having different “brands” for different tones helped reach:


  • Hardboiled readers (who might dislike humor)
  • Caper comedy fans (who might be turned off by violence and nihilism)



Westlake was a professional writer with an eye on the long game—and maintaining two series under two tones allowed him to prolifically publish without oversaturating one style.





🔍 

5. The Metaphysical Answer: Two Criminal Faces of Modern Man



Perhaps more subtly:


  • Parker reflects a universe where violence makes sense, where the only ethic is competence.
  • Dortmunder reflects a universe where no plan survives contact with absurdity.



Both are responses to modernity, but from opposite poles:


  • One is the executioner of illusions.
  • The other is their comic victim.






✴️ 

In Summary



Donald E. Westlake created Parker and Dortmunder because:


  • He had two distinct literary instincts: the darkly precise and the chaotically humane.
  • He understood the value of voice control, tone, and reader expectations.
  • And perhaps most importantly, he understood that crime fiction could contain both tragedy and farce, just not in the same room.



Or, as Westlake might say:


“Sometimes you rob a bank like a ghost.

Sometimes the bank explodes and you’re covered in paint.”


Would you like a playful chart comparing Parker vs. Dortmunder next?


Room 104 (2017-2020)

https://en.wikipedia.org/wiki/Room_104 (Max))

Please list for me the possible candidates of exoplanets where life might exist, thanks. (ChatGPT, 2025-5-31) (自體的心理學)(車行哲學)

With pleasure, my friend. Here is a curated list of notable exoplanets that scientists currently consider potential candidates for life, based on factors like size, temperature, orbital distance, and atmospheric composition (when known). These are worlds that lie in or near the habitable zone—where conditions might allow liquid water to exist.





🌍 

Promising Exoplanets Where Life Might Exist




1. 

Proxima Centauri b



  • Star: Proxima Centauri (our closest stellar neighbor, 4.24 light-years away)
  • Type: Terrestrial, ~1.2 Earth masses
  • Orbital Period: ~11 days
  • Habitable Zone: Yes (but tidally locked)
  • Caveats: Host star is a flare-active red dwarf—may strip atmosphere






2. 

TRAPPIST-1 System (7 Earth-size planets)



  • Star: TRAPPIST-1 (39 light-years away)
  • Type: Ultra-cool red dwarf
  • Promising planets: TRAPPIST-1e, f, and g
  • Orbit: All within 1–13 days
  • Habitable Zone: Yes (e, f, g most likely)
  • Caveats: High stellar activity could threaten atmospheres






3. 

LHS 1140 b & c



  • Star: LHS 1140 (41 light-years away)
  • Type: Red dwarf
  • b: Super-Earth (~6.6 Earth masses), in habitable zone
  • c: Closer orbit, may be less hospitable
  • Note: b has one of the most promising dense atmospheres






4. 

Kepler-442b



  • Star: Kepler-442 (1,206 light-years away)
  • Type: K-type orange dwarf
  • Size: ~1.3 Earth radii
  • Habitable Zone: Yes (receives ~70% of Earth’s sunlight)
  • Note: Likely rocky, stable orbit






5. 

Kepler-452b



  • Star: Kepler-452 (1,800 light-years away, G-type like the Sun)
  • Size: ~1.6 Earth radii
  • Habitable Zone: Yes
  • Nickname: “Earth’s older cousin”
  • Caveats: Uncertain whether it’s rocky or gaseous






6. 

Teegarden’s Star b & c



  • Star: Teegarden’s Star (12.5 light-years away)
  • Type: Red dwarf
  • Both planets: Near Earth-mass, in habitable zone
  • Caveats: Young system; habitability not yet well understood






7. 

K2-18b



  • Star: K2-18 (124 light-years away)
  • Size: ~2.6 Earth radii (likely a “mini-Neptune”)
  • Note: Detected water vapor in atmosphere in 2019
  • Caveats: May have high-pressure hydrogen atmosphere—not Earth-like, but possibly habitable in the upper atmosphere






8. 

Gliese 1061c



  • Star: Gliese 1061 (12 light-years away)
  • Type: M dwarf
  • Size: ~1.4 Earth masses
  • Habitable Zone: Likely within it
  • Note: Quiet host star—less flare activity






9. 

Ross 128 b



  • Star: Ross 128 (11 light-years away)
  • Size: ~1.4 Earth masses
  • Habitable Zone: Yes
  • Note: Star is relatively quiet—encouraging for atmospheric stability






10. 

Wolf 1061c



  • Star: Wolf 1061 (14 light-years away)
  • Size: ~4.3 Earth masses
  • Habitable Zone: On the inner edge—could be Venus-like
  • Caveats: Possible greenhouse effect too strong






🧪 

Criteria for Habitability



To be considered a candidate for life, scientists look for:


  • Right distance from the star (liquid water zone)
  • Stable orbit
  • Rocky composition (not gas giant)
  • Atmosphere retention
  • Low stellar activity (especially for red dwarfs)
  • Bio-signature gases (e.g., oxygen, methane, water vapor — under investigation)






🔭 

What’s Next?



  • Missions like JWST, ELT, and future direct imaging telescopes aim to study atmospheres in more detail.
  • The holy grail: detecting biosignatures—signs of life-related chemistry.





Would you like a visual map or chart comparing these planets by temperature, mass, or distance from Earth?


Distance from earth, in table. (ChatGPT, 2025-5-31)


Here is a table listing the distance from Earth for each potentially habitable exoplanet mentioned earlier:

Planet

Distance from Earth (light-years)

Proxima Centauri b

4.24

TRAPPIST-1e

39

TRAPPIST-1f

39

TRAPPIST-1g

39

LHS 1140 b

41

Kepler-442b

1,206

Kepler-452b

1,800

Teegarden’s Star b

12.5

K2-18b

124

Gliese 1061c

12

Ross 128 b

11

Wolf 1061c

14

Let me know if you’d like to sort them by proximity, temperature, or any other property.


Since these exoplanets are all at least a few light years away from the Earth, is it possible to explore them in time? (ChatGPT, 2025-5-31)


That, my friend, is the great cosmic question—part physics, part engineering, part dream.


To answer directly:


With current technology: No, we cannot explore them in real time.

But with future innovations: Perhaps—though not soon, and not easily.


Let’s explore why it’s so difficult—and what the possibilities might be.





🚀 

Current Technology: Incredibly Slow



Even our fastest spacecraft—like Voyager 1 or New Horizons—travel at about:


  • ~17 km/s, or
  • ~0.000057 times the speed of light (c)



At that speed:


  • It would take Proxima Centauri b (~4.24 light-years away) over 75,000 years to reach.
  • For planets like Kepler-452b (~1,800 light-years away)? — millions of years.



So with today’s chemical propulsion and robotic technology, interstellar exploration is virtually impossible.





🔭 

But… What Are the Future Possibilities?



Here are the most serious proposals under investigation:





1. 🧬 

Breakthrough Starshot



  • Proposed by Yuri Milner, supported by Stephen Hawking (before his death)
  • Idea: Use powerful ground-based lasers to propel tiny light sails (like postage-stamp-sized probes) to ~20% of the speed of light.
  • Target: Proxima Centauri b
  • Time to arrival: ~20 years
  • Caveats:
    • No way to slow down on arrival
    • Only carries minimal sensors
    • Still highly experimental






2. ⚛️ 

Nuclear Propulsion



  • Concepts like Project Orion (1950s–70s): Using controlled nuclear explosions to propel massive craft.
  • Modern ideas: Nuclear thermal propulsion, fusion drives, e.g. the Daedalus and Icarus concepts
  • Travel time to nearby stars: 100–500 years
  • Status: Not yet feasible; raises political, engineering, and safety issues






3. 🧊 

Generation Ships



  • Huge vessels with multiple generations of humans living and dying on board
  • Slow: thousands of years to reach stars
  • Impractical unless long-term life support, sociocultural stability, and biospheres are solved






4. 🌌 

Warp Drives / Wormholes

 

(theoretical)



  • Based on solutions to Einstein’s field equations, e.g. Alcubierre Drive
  • Requires exotic matter with negative energy density
  • Zero experimental support yet
  • May violate causality or energy conservation






🧭 

Philosophical Reflection: What’s “Exploration”?



If by explore you mean send a human to walk its surface—not anytime soon.


But if exploration includes:


  • Remote sensing (e.g. JWST-style atmospheric analysis)
  • Sail-probes like Breakthrough Starshot
  • Or virtual presence via data



Then yes, we are on the threshold of first contact—not with life, but with the possibility of life.





✴️ 

Conclusion: Is It Possible?


Method

Reach Time to Proxima b

Status

Current rockets

~75,000 years

Feasible, but useless

Starshot light sail

~20 years

Experimental

Nuclear propulsion

~100-500 years

Hypothetical

Generation ships

~1,000+ years

Sci-fi, sociological problem

Warp drives / wormholes

Instant (theoretically)

Pure speculation

So:


Not now. Not easily. But perhaps—one day.

And until then, our exploration is through light, thought, and dreams.


Would you like a speculative roadmap from now to interstellar exploration—something poetic but grounded in physics?