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Our table below lists the requirements for missions to particular asteroids in the published literature. There are probably many more analyses which are unpublished to date. If you know of any, please forward the information or source to us.
A list of NEO's can be found at http://cfa-www.harvard.edu/iau/lists/Unusual.html though that site does not give delta-v analysis for missions, and is not interested in such issues. (As of July 2001, their tables were still not formatted.) This list may be useful for calculating transport requirements, and checking to see if anyone's analyzed these targets for potential missions.
Another issue is an educated guess about the properties of the target as analyzed by telescopic spectroscopy. Is there a source on the internet for this data? Shall we do it here?
The following are a list of particularly interesting asteroids:
|
Target |
Outbound |
Outbound |
Date |
Inbound |
Inbound |
Date |
Total |
Total |
Lunar |
Source |
Comments |
|
Moon |
6000 |
3 |
any |
2500 |
1 |
any |
8500 |
short |
n.a. |
||
|
Phobos-Deimos |
4400 |
270 |
biannual |
1800 |
270 |
biannual |
6200 |
540 |
Scarbrough (1999) |
||
|
Mars |
4800 |
270 |
biannual |
5700 |
270 |
biannual |
10,500 |
540 |
Scarbrough (1999) |
||
|
1982 DB Nereus |
4450 |
210 |
60 |
480 |
4510 |
690 |
Lewis & Lewis (1987) |
From Scarbrough. C? type from spectra? |
|||
|
1982 XB |
5300 |
220 |
220 |
470 |
5770 |
690 |
Lewis & Lewis (1987) |
From Scarbrough |
|||
|
1982 HR |
5300 |
180 |
260 |
320 |
5560 |
500 |
Lewis & Lewis (1987) |
From Scarbrough |
|||
|
1980 AA |
5270 |
390 |
390 |
290 |
5660 |
680 |
Lewis & Lewis (1987) |
From Scarbrough |
|||
|
1998 KY26 |
small |
small |
small |
small |
Ostro |
30 m diameter, water rich from radar data |
|||||
|
1991 JW |
6873 |
fast |
2009-12-05 |
4705 |
fast |
2009-11-18 |
10.89 |
190 |
T.D. Jones et al. (1994) |
Human mission to/from surface, not HEEO |
|
|
1979 VA Wilson-Harrington |
~ 5 years |
Kuck |
Comet in 1949 |
Notes: Gaps in the table need to be filled in. Trip times can be improved at the cost of delta-v. Delta-v varies for dates with NEOs with large cycles. Future changes may eliminate the column on source, turn it into superscripts in other columns, once we get multiple sources
A table comparison is only a rough comparison. The context and details of each one of these cases needs to be discussed. For example, the mission to 1991 JW was optimized to minimize travel time due to human missions, and the return delta-v is to Earth's surface, not to HEEO as the table column states. It's worth pointing out that the total delta-v is less than to the lunar surface. It is suggested that this be a steppingstone mission to Mars in the NASA program, rather than a "return to the Moon" as a steppingstone.
This page was last updated: 30 July 2001
Copyright © 1983-1999 by Mark Prado, All Rights Reserved except where specifically stated otherwise.
Source: www.permanent.com
Projects to Employ Resources of the Moon and Asteroids Near Earth in the Near Term