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Paper summaries #35

Open NirViaje opened 5 years ago

NirViaje commented 5 years ago

Papers

short URL for this page - https://git.io/fpAk3

Target asteroids #3

  1. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-443314506 How to find metal-rich asteroids, 2014, German Aerospace Center
  2. [ ] https://www.google.com/search?q=asteroid+delivery+efficiency
  3. [ ] #34 https://www.google.com/search?q=asteroid+rotation+axis

Solar funace #5

  1. [x] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-444948647 Vasile, Solar Deflection
  2. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-445857015 film lens: MOIRE/MOD-EnMat, etc
  3. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-448868540 Solar pumped laser
  4. [ ] DoE Solar

Target probe #25

  1. [x] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-445441798 MarCO HGA
  2. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-445879704 JAXA solar probe
  3. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-447696268 Cubesat for deep space
  4. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-448755568 Celestial navigation for Cubesat, commercialized cubesat ecology like BCT

Electric propulsion and other methods of propulsion #9

  1. [x] https://github.com/ExponentialDeepSpace/eds-archive/issues/3 Pulsed Plasma Thruster (PPT)
  2. [ ] https://github.com/ExponentialDeepSpace/eds-archive/issues/2 Magneto Plasma Dynamic (MPD) thruster (MPDT), Pulsed Inductive Thruster (PIT), Electrodeless Lorentz Force Thruster (ELF)
  3. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-445876939 MEMS Thruster
  4. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-445942591 Cold gas

Other

  1. [ ] https://github.com/ExponentialDeepSpace/exponentialdeepspace.github.io/issues/35#issuecomment-445877728 1982Lunar #10
  2. [x] film solar cell #21
NirViaje commented 5 years ago

HOW TO FIND METAL-RICH ASTEROIDS

Alan W. Harris and Line Drube German Aerospace Center (DLR) Institute of Planetary Research, Rutherfordstrasse 2, D-12489 Berlin, Germany; alan.harris@dlr.de Received 2014 February 3; accepted 2014 March 8; published 2014 March 24

https://www.researchgate.net/publication/261034084_How_to_find_metal-rich_asteroids

The Near-Earth Asteroid Thermal Model (NEATM; Harris 1998), based on spherical geometry, offers a relatively straightforward means of deriving reasonably accurate diameters and albedos of asteroids and trans-Neptunian objects (in principle all atmosphereless bodies) from thermal-infrared data for objects with unknown physical characteristics. With NEOs in mind, the NEATM was designed to extend the applicability of the thermal model concept described by Lebofsky et al. (1986) to objects with significant thermal inertia and/or rapid rotation. The model incorporates a fitting parameter, η, referred to for historical reasons as the beaming parameter, which allows the model surface temperature distribution to be adjusted to take account of the effects of thermal inertia, spin vector, and surface roughness, thereby giving a better fit of the model fluxes to the measurements.

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NEO Tax. PHA? D(km) pv η ηerr pIR
138359 N 1.09 0.10 2.931 0.105 0.19
1865 S N 1.61 0.14 2.902 0.036 0.27
152931 Q N 1.65 0.24 2.884 0.138 0.24
152978 S: Y 0.53 0.11 2.641 0.116 0.19
365071 Y 0.87 0.15 2.559 0.117 0.28
3554 X, M, D N 3.05 0.09 2.411 0.072 0.19
215442 N 0.79 0.15 2.328 0.325 0.17
152558 S N 1.36 0.18 2.284 0.051 0.28
366774 AS Y 0.86 0.20 2.284 0.059 0.29
250680 Y 0.40 0.15 2.279 0.075 0.30
7822 S Y 1.21 0.13 2.261 0.049 0.30
163243 S, Q Y 1.68 0.17 2.191 0.061 0.23
263976 L Y 0.79 0.13 2.165 0.043 0.18
142464 N 0.89 0.12 2.139 0.044 0.22
2002 NW16 N 0.85 0.16 2.118 0.066 0.26
103067 S Y 1.28 0.25 2.114 0.056 0.29
363024 Y 0.56 0.10 2.055 0.067 0.24
325102 N 0.36 0.12 2.048 0.063 0.18
NirViaje commented 5 years ago

Vasile, Solar Deflection

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De-Starlite from UCSB

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Publication: Massimiliano Vasile https://www.google.com.hk/search?q=Vasile+asteroid https://www.youtube.com/watch?v=mOtIwp86rF0 Vasile-solar-deflection Hazardous asteroid mitigation- Campaign planning and credibility analysis, thesis, Yohei Sugimoto, 2014_2014sugimotophd.pdf

NirViaje commented 5 years ago

Hodges, Richard E. (21 February 2017). "A Deployable High-Gain Antenna Bound for Mars: Developing a New Folded-panel Reflectarray for the First CubeSat Mission to Mars". IEEE Antennas and Propagation Magazine. 59: 39–49. doi:10.1109/MAP.2017.2655561 – via IEEE Xplore Digital Library.

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On board the two CubeSats is an ultra-high frequency (UHF) antenna which is circularly polarized. The EDL information from InSight was transmitted through the UHF band at 8 kbit/s to the CubeSats, and was simultaneously retransmitted at an X band frequency at 8 kbit/s to Earth.[18] MarCO used a deployable solar panel for power, but because of the limitations in solar panel efficiency, the power for the X-band frequency can only be about 5 watts.

In order for the CubeSats to be able to relay information, they need to have a high gain antenna (HGA) which is reliable, meets the mass specs, has low complexity, and is affordable to build. A high gain antenna is one that has a focused, narrow radiowave beam width (directional antenna). Three possible types of antennas were assessed: a standard microstrip patch antenna, a reflectarray, and a mesh reflector. With the small, flat, size required for the CubeSats, the reflectarray antenna type met all of the mission needs. The components of a reflectarray HGA are three folded panels, a root hinge which connects the wings to the body of the CubeSat, four wing hinges, and a burn wire release mechanism. The antenna panels must be able to withstand a varying degree of temperature changes throughout the mission as well as vibrations throughout deployment.[18] MarCO relayed EDL-critical data 8 minutes after the completion of the landing.[19][20]

https://en.wikipedia.org/wiki/Mars_Cube_One#Relay

IRIS Radio

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NirViaje commented 5 years ago

Optical membrane

07a0c3029fbc71ae91df35578ac2742 83a45f1b957060a3748f12b093542dd 3be2559c85fbb472b5322b04c46bdc1 cf5adaba9205e7355d731bef7825206

Membrane optics is a flat lens that employs plastic in place of glass to diffract rather than reflect or refract light. Concentric microscopic grooves etched into the plastic provide the diffraction.[1]

Glass transmits light with 90% efficiency, while membrane efficiencies range from 30-55%. Membrane thickness is on the order of that of plastic wrap.[1]

Diffractive Fresnel Lens

NirViaje commented 5 years ago
NirViaje commented 5 years ago
NirViaje commented 5 years ago

MEMS Thruster

NirViaje commented 5 years ago

image image NASA Lunar 1982

NirViaje commented 5 years ago

IKAROS

image image https://en.wikipedia.org/wiki/OKEANOS image image

NirViaje commented 5 years ago

image image Propellant: R134a and R236fa

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NirViaje commented 5 years ago

-

NirViaje commented 5 years ago

Cubesat for deep space

Cubesat for the moon

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Lunar IceCube

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Xe

液体密度:3057kg·m⁻³(-108.10℃,101.325kpa) 储罐压力:30MPa

Nanosat fleet proposed to 300 asteroids

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Mission details

A single MAT nanospacecraft

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NirViaje commented 5 years ago

Celestial navigation and deep space orbit for Cubesat

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Commercialized CubeSat ecology

BCT

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NirViaje commented 5 years ago

Solar-pumped laser