Boron on extrasolar rocky planets?

  • Thread starter Thread starter Nik_2213
  • Start date Start date
Click For Summary
SUMMARY

This discussion centers on the availability of boron on rocky planets orbiting old, metal-poor Population II stars compared to younger Population I stars. The ship 'City of Fresno' is conducting a 360º passive mapping scan to identify potential sources of boron, which is crucial for supporting life and manufacturing processes aboard. Boron is rare and primarily produced through cosmic ray spallation, necessitating specific planetary conditions such as sufficient size and tectonic activity for accessibility. The inquiry focuses on whether younger, geologically active systems or older, stable systems provide better boron resources for sustaining the ship's crew and their agricultural needs.

PREREQUISITES
  • Understanding of cosmic ray spallation and its role in element production
  • Knowledge of Population I and Population II star classifications
  • Familiarity with planetary geology and tectonic activity
  • Basic principles of astrobiology and nutrient requirements for plant growth
NEXT STEPS
  • Research the processes of cosmic ray spallation and its implications for element availability
  • Study the characteristics of Population II stars and their planetary systems
  • Investigate the geological features that enhance boron accessibility on rocky planets
  • Explore the nutritional requirements of plants, particularly coffee, in extraterrestrial agriculture
USEFUL FOR

Astronomers, astrobiologists, space mission planners, and anyone interested in the resource availability of extraterrestrial environments for sustaining human life and agriculture.

Nik_2213
Messages
1,218
Reaction score
493
TL;DR Summary: Would rocky planets around old, metal-poor Population II stars have more accessible boron than our younger, Pop l Sol's ??

I'm writing an 'As Hard Science As I Can' about a star-ship far astray in the 'Deep & Dark'.

'City of Fresno' has about 20~~25 LY fuel range as-is, currently doing a 360º/4_Pi passive mapping scan. Then they'll travel about a light year, repeat. Another light-year but skew, repeat. After two more such to complete tetrahedron, they'll have a good map of locale out to their fuel range, with stellar spectra.

Icy moons or Oort comets may be tediously mined for H/D fusion fuel, side-streams should provide a lot of micro-nutrients to top-up the 'Ponics.

But Boron is a 'gotcha': It is remarkably rare, produced by random cosmic ray spalling of eg carbon, then concentrated unto 'accessible' by natural leaching of volcanic materials. So, planet must be big enough or tidally-stirred for tectonics. Even Mars has some borates in ancient crater lakes' clay strata...

The ship's crew need boron / borates to supplement their 'Ponics, especially if they want to grow Coffee, which is famously greedy. Boron is essential for metallurgy, to alloy into the bits and cutters to make the tools to make the tools they'll need. Boron is also essential for boro-silicate glass to do 'bench' and 'prep' chemistry...

So, for boron, are they likely to glean more from a younger 'Pop_l' system, with 'geologically recent' tectonic activity ?
Or from a tired, old, 'Pop_ll' system that's had much more 'deep time' to accumulate cosmic-ray spallation ??
 
  • Like
Likes   Reactions: Bystander
Physics news on Phys.org
Please, any ideas ??
 
That's a question that requires some pretty specific knowledge to answer. Unfortunately I'm not sure you'll find someone on the forums who can answer it.
 
  • Like
Likes   Reactions: Nik_2213
After perusing umpteen arcane arxiv PDFs, turns out that scant few 'Pop ll' systems have rocky planets, so I may strike such from serious consideration...

Fortunately, the ship is in the galaxy 'disk', not an old 'Pop ll' zone, such as bulge, halo or globular cluster...
 
  • Like
Likes   Reactions: Drakkith

Similar threads

  • · Replies 6 ·
Replies
6
Views
4K