Read moreSome worry too much about asteroid impacts, which are among the natural risks that are best understood and easiest to quantify. Moreover, it will soon be possible to reduce that risk by deflecting the path of asteroids heading for the earth. That’s why I support the B612 Sentinel project.
asteroids
Everything you need to know about the Japanese Space Agency (JAXA)’s upcoming Hayabusa2 mission, to rendezvous with an asteroid and bring samples back.
Launching soon! And then we wait til 2020 for its return.
Read moreAmerican geophysicists believe the moon’s Procellarum region, a dark patch more than half the size of Australia, resulted from a magma plume rather than a massive asteroid strike, as previously thought. The finding “deals a big blow to the asteroid theory”, said Brown University, which contributed to the study. Procellarum is the only lunar “sea” big enough to be called an ocean and is one of a number of dark spots on the moon’s surface that, when seen from Earth, resemble a face. Unlike other dark areas such as the Sea of Rains and Sea of Serenity, Procellarum is not surrounded by signs of impact, such as mountains and scars. Scientists have long debated whether Procellarum is so old that the impact signs have been eroded, or was formed by a different process. Now researchers say they have settled the argument, using data from twin NASA spacecraft that orbited the moon in 2012 and mapped its gravity. The team created a high-resolution map showing Procellarum’s border composed of sharp angles that could not have been created by an asteroid. The researchers believe the angular outline was produced by giant tension cracks in the crust as it cooled around magma from deep inside the moon. Maria Zuber, co-author of a paper in the journal Nature, said tthe cracks had formed a “plumbing system” which had allowed magma to meander to the surface and created the dark spots we see.
LINKS: http://www.newscientist.com/article/mg22229753.300-crystal-cocoons-kept-bacteria-safe-in-space.html http://blogs.scientificamerican.com/guest-blog/2013/01/09/the-origins-of-directed-panspermia/ http://www.amazon.com/Echopraxia-Peter-Watts/dp/076532802X EXTRA READING: http://runesoup.com/2012/02/you-are-made-of-books-the-whisky-rant-part-5/ ERRATA: of course Francis Crick was tripping on LSD when he discovered DNA.
Read moreA collage of radar images of near-Earth asteroid 2006 DP14 was generated by NASA scientists using the 230-foot (70-meter) Deep Space Network antenna at Goldstone, Calif., on the night of Feb. 11, 2014.
Delay-Doppler radar imaging revealed that the asteroid is about 1,300 feet (400 meters) long, 660 feet (200 meters) wide, and shaped somewhat like a big peanut. The asteroid’s period of rotation is about six hours. The asteroid is of a type known as a “contact binary” because it has two large lobes on either end that appear to be in contact. Previous radar data from Goldstone and the Arecibo Observatory in Puerto Rico has shown that at least 10 percent of near-Earth asteroids larger than about 650 feet (200 meters) have contact binary shapes like that of 2006 DP14.
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Radar is a powerful technique for studying an asteroid’s size, shape, rotation state, surface features and surface roughness, and for improving the calculation of asteroid orbits. Radar measurements of asteroid distances and velocities often enable computation of asteroid orbits much further into the future than if radar observations weren’t available.
NASA places a high priority on tracking asteroids and protecting our home planet from them. In fact, the United States has the most robust and productive survey and detection program for discovering near-Earth objects. To date, U.S. assets have discovered more than 98 percent of the known near-Earth objects.
Read morethe nature of: asteroid quakes
In 2010, Richard Binzel, a professor of planetary sciences at MIT, identified a likely explanation: Asteroids orbiting in our solar system’s main asteroid belt, situated between Mars and Jupiter, are exposed to cosmic radiation, changing the chemical nature of their surfaces and reddening them over time. By contrast, Binzel found that asteroids that venture out […]
Read more "the nature of: asteroid quakes"Mars-crossers that are also Earth-crossers or grazers
These objects are not catalogued as Mars-crossers in databases such as the Jet Propulsion Laboratory’s online Small-body Database Browser. Instead, they are categorized as Near Earth Objects (NEOs).
- 1566 Icarus
- 1685 Toro
- 1862 Apollo
- 1863 Antinous
- 1864 Daedalus
- 1866 Sisyphus
- 1981 Midas
- 2101 Adonis
- 2102 Tantalus
- 2135 Aristaeus
- 2201 Oljato
- 2212 Hephaistos
- 2329 Orthos
- 3103 Eger
- 3200 Phaethon
- 3360 Syrinx
- 3671 Dionysus
- 3752 Camillo
- 3838 Epona
- 4015 Wilson-Harrington
- 4179 Toutatis
- 4183 Cuno
- (4197) 1982 TA
- 4257 Ubasti
- 4341 Poseidon
- 4450 Pan
- 4486 Mithra
- 4660 Nereus
- (4953) 1990 MU
- 5011 Ptah
- (5131) 1990 BG
- 5143 Heracles
- (5189) 1990 UQ
- (5496) 1973 NA
- (5645) 1990 SP
- (5660) 1974 MA
- (5693) 1993 EA
- 5731 Zeus
- 5786 Talos
- (5828) 1991 AM
- (6037) 1988 EG
- (6047) 1991 TB1
- (6053) 1993 BW3
- 6063 Jason
- (6455) 1992 HE
- 6489 Golevka
- (6611) 1993 VW
- (7025) 1993 QA
- 7092 Cadmus
- (7335) 1989 JA
- (7341) 1991 VK
- (7350) 1993 VA
- (7482) 1994 PC1
- (7753) 1988 XB
- (7888) 1993 UC
- (7889) 1994 LX
- (8014) 1990 MF
- (8035) 1992 TB
- (8176) 1991 WA
- (8201) 1994 AH2
- (8507) 1991 CB1
- (8566) 1996 EN
- (9058) 1992 JB
- 9162 Kwiila
- (9202) 1993 PB
- (9856) 1991 EE
- (10145) 1994 CK1
- (10165) 1995 BL2
- (10636) 1998 QK56
- 11066 Sigurd
- 11311 Peleus
- (11405) 1999 CV3
- (11885) 1990 SS
- (12538) 1998 OH
- 12923 Zephyr
- (13651) 1997 BR
- 14827 Hypnos
- (16816) 1997 UF9
- (16834) 1997 WU22
- (16960) 1998 QS52
- (17181) 1999 UM3
- (17182) 1999 VU
- (17188) 1999 WC2
- (20236) 1998 BZ7
- (20425) 1998 VD35
- (20429) 1998 YN1
- (20826) 2000 UV13
- (22753) 1998 WT
- (22771) 1999 CU3
- (23187) 2000 PN9
- (24443) 2000 OG
- (24445) 2000 PM8
- 24761 Ahau
- 25143 Itokawa
- (25330) 1999 KV4
- (26379) 1999 HZ1
- (26663) 2000 XK47
- (27002) 1998 DV9
- (29075) 1950 DA
- (30825) 1990 TG1
- (30997) 1995 UO5
- (31662) 1999 HP11
- (31669) 1999 JT6
- (35396) 1997 XF11
- (35670) 1998 SU27
- (36236) 1999 VV
- (36284) 2000 DM8
- (37638) 1993 VB
- 37655 Illapa
- 38086 Beowulf
- (38239) 1999 OR3
- (40267) 1999 GJ4
- (41429) 2000 GE2
- (42286) 2001 TN41
- (52340) 1992 SY
- (52750) 1998 KK17
- (52760) 1998 ML14
- (52762) 1998 MT24
- (53319) 1999 JM8
- (53409) 1999 LU7
- (53426) 1999 SL5
- (53429) 1999 TF5
- (53550) 2000 BF19
- (53789) 2000 ED104
- (55532) 2001 WG2
- (65690) 1991 DG
- (65717) 1993 BX3
- (65733) 1993 PC
- 65803 Didymos
- (65909) 1998 FH12
- (66008) 1998 QH2
- (66063) 1998 RO1
- (66253) 1999 GT3
- (67381) 2000 OL8
- (67399) 2000 PJ6
- (68216) 2001 CV26
- (68267) 2001 EA16
- (68346) 2001 KZ66
- (68348) 2001 LO7
- (68372) 2001 PM9
- (68548) 2001 XR31
- 69230 Hermes
- 2007 WD5
- (85640) 1998 OX4
- 2003 BR47
The mammoth asteroid set to fly by Earth last night just disappeared
The most likely explanation is that its orbit was miscalculated. Even with its current whereabouts unknown, the near earth asteroid poses no present danger to Earth — in fact, if anything, its loss indicates that 2000 EM26 is probably further out in space that was originally thought.
The mammoth asteroid set to fly by Earth last night just disappeared
Read more "The mammoth asteroid set to fly by Earth last night just disappeared"Asteroid mining could be useful to space travel
“The question is, ‘What is the most efficient way of colonizing the solar system?’” he said. “And the notion of doing that might be so-called ‘living off the land.’ Instead of bringing resources that we need to colonize Mars, asteroids, etc. all the way from the Earth, what if we were able to actually extract those essential materials that are needed locally?”
With a current cost of about $10,000 per pound to send something into orbit, the possibility of using materials found in space, as opposed to bringing all supplies from Earth, would be the most cost- and energy-effective option available.
This would fit into what Engineering Prof. Brian Gilchrist said is a “resurgence and entrepreneurial mindset of new things we can do in space that haven’t been considered at all.”
Gilchrist’s research focuses on space tethering, which involves connecting two spacecraft with a conductive cable. As the spacecraft orbit in Earth’s electromagnetic field, the cable becomes charged. Solar power is used to add or leak charge from this circuit, causing the two spacecraft to move up or down. This theoretical system would allow the satellites to gain momentum without a propellant, and could have practical applications for tugging asteroids around in the Moon’s orbit.
Apart from colonization of the solar system, another potential purpose for mining asteroids is bringing materials back to Earth for environmental and commercial purposes.
“I think one of the best products from (asteroid mining), whether you’re mining for precious metals that are rare on earth or water for propulsion, is that there’s the opportunity for us to stop destroying the Earth’s environment,” said Engineering senior Bradley Costa.
Costa is currently engaged in a co-op with Planetary Resources, a leading private-sector company that conducts research on asteroid mining.
Along with sustainability benefits, corralling an asteroid could result in long-term economic benefits.
“One study I read says that one asteroid about a mile in diameter has enough precious metal on it to help humanity with all its needs for 10,000 years or so,” said Gallimore.
Asteroid mining could be useful to space travel
Read more "Asteroid mining could be useful to space travel"Finding a comet: the backstory | Rocket Science
“
The comet was actually discovered by my computer here under my desk!
Our human-volunteer TOTAS clickers review all the ‘movers’ found by the software and either confirm or reject them. That task can’t be done by software – but the software can combine the single detections and extract the moving objects.
”
Just one of the ways we’re forming a team with machines and exploring the cosmos.
Finding a comet: the backstory | Rocket Science
Read more "Finding a comet: the backstory | Rocket Science"