Showing posts with label JPL. Show all posts
Showing posts with label JPL. Show all posts

13 July 2016

New dwarf planet discovered in our Solar System


New dwarf planet (TNO) discovered in our Solar System!
Via: RT
Astronomers at CFHT (Canada-France-Hawaii Telescope), Maunakea, Hawaii, have announced the discovery of 2015 RR245 as part of the ongoing Outer Solar System Origins Survey (OSSOS).
2015 RR245's orbit is highly eccentric, with a semi-major axis of 81.3AU, perihelion of 33.7AU, aphelion of 128.9 AU, inclination of 7.575 degrees and an orbital period of 733 years.
First observed, retrospectively, on 2015-09-09, 2015 RR245 is estimated to be ±700km / 438 miles in diameter, although Dr. Michele Bannister of the University of Victoria in British Columbia also stated: "it’s either small and shiny, or large and dull"
If any of you have, or have access to, the equipment necessary to observe 2015 RR245, it is currently located at RA:00 23 14.73, DEC:+06 00 35.8 with an apparent magnitude of 21.98 (distance 63.85 AU).  As a rough guide,  2015 RR245 is currently located in the constellation of Pisces, a little to the right of Uranus.
Further, detailed, information is available from 2015 RR245 on JPL's SBDB, and also by visiting JPL's Horizons interface and entering "2015 RR245" as the Target Body.  More information about CFHT can be found here.
Click orbit diagram to enlarge.  The hi-res image of 2015 RR245's orbit --showing comparison to other, known, TNOs is available here.

2016 The THIRD Year of "CERTAIN Uncertainty" ™ / Meteors, Asteroids, Comets, and MORE!

28 February 2016

Asteroid news: NASA's update on 2013 TX68

Asteroid news: NASA's update on 2013 TX68
reported by  meteordetective
Link to article which was updated on Thu 25-Feb-2016 at 14:40 Pacific Time (22:40Z) and was originally posted on Tue 02-Feb-2016.

NASA have refined their "earlier flyby and distance predictions, reconfirming that the asteroid poses no threat to Earth."

But, the 'plot' thickens, as NASA has additionally "..identified an extremely remote chance that this small asteroid could impact on Sep. 28, 2017, with odds of no more than 1-in-250-million. Flybys in 2046 and 2097 have an even lower probability of impact."

I thought I'd investigate further and used Telnet to 'talk' to JPL's "Horizons" system.  However, as you can see (from the copy/paste below), there is no close-approach listed for 2017.  To be clear and specific, I instructed Horizons to show me all the known approaches from 01-Jan-2000 to 01-Jan-2200.

        Date (TDB)      Body   CA Dist  MinDist  MaxDist   Vrel  TCA3Sg  Nsigs  P_i/p
----------------------  -----  -------  -------  -------  ------ ------ ------ -------
A.D. 2001 Feb 12.30797  Venus  .075550  .029997  .430225  10.352 95321. 27737. .000000
A.D. 2013 Oct 13.34047  Earth  .013900  .013840  .013959  14.066   0.34 505.63 .000000
A.D. 2016 Mar 08.00436  Earth  .033383  .000207  .115301  15.324 8719.4 463.31 .000000
A.D. 2024 May 21.93046  Mars   .051950  .039661  .181328  15.950 8218.6 83319. .000000
A.D. 2028 Oct 22.29797  Earth  .092654  .010847  .254975  11.643 36290. 37681. .000000

If you access the asteroid's entry in JPL's SBDB, you'll see the following Close-Approach dates & times listed, which barely correspond to the Telnet session results (above).

2016-Mar-08 00:06, 2056-Sep-18 13:29, 2071-Sep-30 14:02, 2074-Feb-17 05:44, 2084-Oct-20 19:33, 2086-Oct-16 07:11, 2089-Feb-07 09:03, 2089-Mar-14 21:35.

Is something out of sync?

I'd initially intended to comment on the wide variance of 2013 TX68's potential close-approach distances (all relative to Earth's surface), which are remarkable and summarised below:

Nominal (the expected or 'should be' distance): 13.06 LD = 3,099,296.455 miles
Minimum: 0.08LD = 15,282.762 miles
Maxium: 45.09LD = 10,714,428.346 miles

(For reference, 1 LD --aka 1 Lunar Distance-- is equivalent to 382,500 kilometers / 239,062.5 miles (NASA)).

The difference between minimum and maximum values is 7,615,132 miles or 8.19% of the distance from Earth to the Sun...or also equivalent to 3,185.42% the distance from Earth to the Moon....which is a rather large value.

To add a further variable in to this situation, MPC have assigned 2013 TX68 a condition code of 8 for  its orbit uncertainty (10=highly uncertain and 0 = "good"), which is due to the fact that 2013 TX68 was only tracked for 3 days when it was initially discovered/observed - before it was 'lost' again.

Let me make myself perfectly clear:  I'm not suggesting 2013 TX68 will hit Earth, inferring it or stirring-up 'fear-porn'.  I'm just a little perplexed by the apparent of confusion --regarding when it will make its close-approaches to Earth-- and mentioning that there's a very wide margin of 'error' between the distances NASA are reporting for its 08-March-2016 close-approach.

Stay tuned!

Write to:
meteordetective AT gmail DOT com.

2016 The THIRD Year of "CERTAIN Uncertainty" ™ / Meteors, Asteroids, Comets, and MORE!!

18 November 2014

Geologic Maps of Vesta from NASA's Dawn Mission Published

Geologic Maps of Vesta from NASA's Dawn Mission Published
"click on image to enlarge"
This high-resolution geological map of Vesta is derived from Dawn spacecraft data.
Credit: NASA/JPL-Caltech/ASU
This high-resolution geological map of Vesta is derived from Dawn spacecraft data. Brown colors represent the oldest, most heavily cratered surface. Purple colors in the north and light blue represent terrains modified by the Veneneia and Rheasilvia impacts, respectively. Light purples and dark blue colors below the equator represent the interior of the Rheasilvia and Veneneia basins. Greens and yellows represent relatively young landslides or other downhill movement and crater impact materials, respectively. This map unifies 15 individual quadrangle maps published this week in a special issue of Icarus. Map is a Mollweide projection, centered on 180 degrees longitude using the Dawn Claudia coordinate system.

JPL manages the Dawn mission for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. The University of California at Los Angeles (UCLA) is responsible for overall Dawn mission science. Orbital Sciences Corp. in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are international partners on the mission team.

Download Full-Res TIFF: PIA18788.tif (14.26 MB)

Download Full-Res JPG: PIA18788.jpg (1.03 MB)

View all Images

More information about Dawn is online at http://www.nasa.gov/dawn.

"click on image to enlarge"
Vesta Topography Map
Credit- NASA/JPL-Caltech/UCLA/MPS/DLR/IDA/PSI
Vesta Topography Map
This color-coded topography map from NASA's Dawn mission shows the giant asteroid Vesta in an equirectangular projection at 32 pixels per degree, relative to an ellipsoid of 177 miles by 177 miles by 142 miles (285 kilometers by 285 kilometers by 229 kilometers). The color scale extends from 13.96 miles (22.47 kilometers) below the surface in purple to 12.11 miles (19.48 kilometers) above the surface in white. The topographic map was constructed from analyzing more than 17,000 images from Dawn's framing camera that were taken with varying sun and viewing angles.

The Dawn mission to Vesta and Ceres is managed by NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, for NASA's Science Mission Directorate, Washington. The University of California, Los Angeles, is responsible for overall Dawn mission science. The Dawn framing cameras were developed and built under the leadership of the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, with significant contributions by DLR German Aerospace Center, Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The framing camera project is funded by the Max Planck Society, DLR and NASA.

More information on Dawn is available at: http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov .


------

NOVEMBER 17, 2014
Geologic Maps of Vesta from NASA's Dawn Mission Published

Images from NASA's Dawn Mission have been used to create a series of high-resolution geological maps of the large asteroid Vesta, revealing the variety of surface features in unprecedented detail. These maps are included with a series of 11 scientific papers published this week in a special issue of the journal Icarus.

Geological mapping is a technique used to derive the geologic history of a planetary object from detailed analysis of surface morphology, topography, color and brightness information. A team of 14 scientists mapped the surface of Vesta using Dawn spacecraft data, led by three NASA-funded participating scientists: David A. Williams of Arizona State University, Tempe; R. Aileen Yingst of the Planetary Science Institute, Tucson, Arizona; and W. Brent Garry of the NASA Goddard Spaceflight Center, Greenbelt, Maryland.

"The geologic mapping campaign at Vesta took about two-and-a-half years to complete, and the resulting maps enabled us to recognize a geologic timescale of Vesta for comparison to other planets," said Williams.

Scientists discovered through these maps that impacts from several large meteorites have shaped Vesta's history. Asteroids like Vesta are remnants of the formation of the solar system, giving scientists a peek at its history. Asteroids could also harbor molecules that are the building blocks of life and reveal clues about the origins of life on Earth.

The geologic mapping of Vesta is enabled by images obtained by the framing camera provided by the Max Planck Institute for Solar System Research of the German Max Planck Society and the German Aerospace Center. This camera takes panchromatic images and seven bands of color-filtered images. Stereo photos are used to create topographic models of the surface that aid in the geologic interpretation.

Vesta's geologic timescale is determined by the sequence of large impact events, primarily by the Veneneia and Rheasilvia impacts in Vesta's early history and the Marcia impact in its late history. The oldest crust on Vesta pre-dates the Veneneia impact.The relative timescale is supplemented by model-based absolute ages from two different approaches that apply crater statistics to date the surface.

"This mapping was crucial for getting a better understanding of Vesta's geological history, as well as providing context for the compositional information that we received from other instruments on the spacecraft: the visible and infrared (VIR) mapping spectrometer and the gamma-ray and neutron detector (GRaND)," said Carol Raymond, Dawn's deputy principal investigator at NASA's Jet Propulsion Laboratory in Pasadena, California.

The objective of NASA's Dawn mission is to characterize the two most massive objects in the main asteroid belt between Mars and Jupiter - Vesta and the dwarf planet Ceres. The spacecraft launched in 2007. Vesta, orbited by the Dawn spacecraft between July 2011 and September 2012, was thought to be the source of a unique set of basaltic meteorites (called HEDs, for howardite-eucrite-diogenite), and Dawn confirmed the Vesta-HED connection.

The Dawn spacecraft is currently on its way to Ceres, the largest object in the asteroid belt. Dawn will arrive at Ceres in March 2015.

Dawn uses ion propulsion in spiraling trajectories to travel from Earth to Vesta, orbit Vesta and then continue on to orbit the dwarf planet Ceres. Ion engines use very small amounts of onboard fuel, enabling a mission that would be unaffordable or impossible without them.

JPL manages the Dawn mission for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. The University of California at Los Angeles (UCLA) is responsible for overall Dawn mission science. Orbital Sciences Corp. in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are international partners on the mission team.

For more information about Dawn, visit:

http://www.nasa.gov/dawn


Media Contact
Elizabeth Landau
NASA's Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6425
Elizabeth.Landau@jpl.nasa.gov

Robert Burnham
Arizona State University, Tempe, Ariz.
480-458-8207
Robert.Burnham@asu.edu

Press Release 2014-399

2014 The Year of "CERTAIN Uncertainty" ™; Meteors, Asteroids, Comets, and MORE!!

15 November 2014

Newly Released Map Data Shows Frequency of Small Asteroid Impacts, Provides Clues on Larger Asteroid Population

Newly Released Map Data Shows Frequency of Small Asteroid Impacts, Provides Clues on Larger Asteroid Population
Linda Billings & NASA/JPL Near-Earth Object Program Office- November 14, 2014
Map showing the bolide events from 1994 to 2013
It happens all the time: small asteroids impact Earth's atmosphere

Small asteroids near Earth, with sizes of only about a meter, hit the atmosphere and disintegrate with surprising frequency - around every other week, new data show.

Data gathered by U.S. government sensors and released to NASA for use by the science community reveal that these small impact events are frequent and random. A map of these small impact events - known as fireballs or bolides - recently released by NASA shows the frequency and approximate
energy released by bolide events detected from 1994 through 2013. It dwarfs a data-base of small impacts based on infra-sound detections released last fall, but it does not contain all fireballs - objects less than a meter in size - that impacted the Earth during this period.

Over this 20-year interval, U.S. Government assets recorded at least 556 bolide events of various energies. On this world map illustration, the size of the orange dots (daytime events) and blue dots (nighttime events) are proportional to the optical radiated energy of the impact event measured
in billions of Joules (GJ) of energy. An approximate conversion between the measured optical radiant energy and the total impact energy can be made using an empirical relationship provided by Peter Brown and colleagues in 2002. For example the smallest dot on the map represents 1 billion
Joules (1 GJ) of optical radiant energy, or when expressed in terms of a total impact energy the equivalent of about 5 tons of TNT explosives. Likewise, the dots representing 100, 10,000 and 1,000,000 Giga Joules of optical radiant energies correspond to impact energies of about 300 tons, 18,000 tons and one million tons of TNT explosives respectively.

The largest impact energy recorded during this 20-year interval was the recent daytime Chelyabinsk event (440,000 - 500,000 tons of TNT) recorded over central Russia on February 15, 2013. This small asteroid that exploded in the atmosphere near Chelyabinsk, Russia was about 20 meters in size
before it hit the Earth. While that impact focused public attention on the potential hazards of NEO impacts with Earth, space scientists have long known that such events are just a part of Earth's geologic history.

NASA's Near Earth Object (NEO) Observations Program finds, tracks, and characterizes asteroids whose orbits bring them within approximately 50 million kilometers (31 million miles) of Earth's orbit about the sun.

"We now know that Earth's atmosphere does a great job of protecting Earth from small asteroids", said NASA NEO Observations Program Executive Lindley Johnson. The new data will be extrapolated to estimate more precisely the frequency of impacts by asteroids large enough to cause ground damage.
"How big is the population of larger asteroids we really need to worry about? We need to better understand that." Johnson said.

While the new data emphasize that small asteroid impacts with Earth are not unusual, the risk of future impacts is not to be taken lightly. "The aim is to find potentially hazardous asteroids before they find us," said Donald Yeomans, manager of NASA's NEO Program Office at the Jet Propulsion
Laboratory.

NASA's Asteroid Initiative features a Grand Challenge to the community "to create a plan to find all asteroid threats to human populations and know what to do about them."

The NEO Observations Program already has identified more than 96 percent of the estimated population of nearly one thousand one-kilometer or larger
sized asteroids. The Program's current objective is to identify 90 percent or more of the far more numerous NEOs larger than 140-meters in diameter. It is estimated they may be as much as 25 times more numerous than 1 kilometer asteroids.

Every day, Earth is bombarded with more than 100 tons of dust and sand-sized particles from space. About once a year, an automobile-sized asteroid hits Earth's atmosphere, creating a spectacular fireball (bolide) event as the friction of the Earth's atmosphere causes them to disintegrate - sometimes explosively.

Studies of Earth's history indicate that about once every 5,000 years or so on average an object the size of a football field hits Earth and causes significant damage. Once every few million years on average an object large enough to cause regional or global disaster impacts Earth. Impact craters on Earth, the Moon and other planetary bodies are evidence of these occurrences.

Meteor Crater near Winslow, Arizona, is evidence of the impact with Earth's surface of a 50-meter asteroid about 50,000 years ago. Impact of the metal-rich object released energy equivalent to a 10 megaton explosion and formed a 1.2 kilometer-diameter crater. Scientists have identified several dozen
impact craters in North America alone, most masked by erosion and vegetation.

Scientific assessments of the risk of, as well as the hazards posed by, future asteroid impacts with Earth vary. In a 2013 paper published in Nature, Peter Brown and his colleagues reported that "telescopic surveys have only discovered about 500 near-Earth asteroids that are 10-20 meters
in diameter (comparable to the Chelyabinsk asteroid) of an estimated near-Earth asteroid population of around 2 x 10 7 [20 million], implying that a significant impactor population at these sizes could be present but not yet cataloged in the discovered near-Earth asteroid population."

"These newly released data will help NEO scientists construct a more complete picture of the frequency and scope of asteroid impacts with Earth," said Johnson.

In conducting its work, the NEO Observations Program collaborates with other U.S. government agencies, other national and international entities, and professional and amateur astronomers around the world. NASA works closely with the Federal Emergency Management Agency and other federal
government departments and agencies on NEO impact warning, mitigation and response planning. The Program is responsible for facilitating communications between the astronomical community, the federal government and the public about NEO impact hazards and risks. The NEO Observations Program is a lead participant in a newly organized International Asteroid Warning Network.

For more information:
http://neo.jpl.nasa.gov/news/news186.html

http://science.nasa.gov/planetary-science/near-earth-objects/

http://www.nasa.gov/mission_pages/asteroids/overview/fastfacts.html

For a documented list of bolide events, see:
http://neo.jpl.nasa.gov/fireball

References:
P.G. Brown et al., The flux of small near-Earth objects colliding with
the Earth. Nature, vol. 420, 21 Nov. 2002, pp. 294-296

P.G. Brown et al., A 500-kiloton airburst over Chelyabinsk and an enhanced
hazard from small impactors, Nature 503, 14 November 2013

2014 The Year of "CERTAIN Uncertainty" ™; Meteors, Asteroids, Comets, and MORE!!

14 February 2013

LIVE BROADCAST Asteroid 2012 DA14 -NASA to Chronicle Close Earth Flyby of Asteroid 2012 DA14

Asteroid 2012 DA14 - LIVE BROADCAST -NASA to Chronicle Close Flyby Earth Asteroid

(click on image to enlarge)
Asteroid 2012 DA14 Earth Close Flyby
Image courtesy of NASA/JPL
NASA TO CHRONICLE CLOSE EARTH FLYBY OF ASTEROID 15FEB2013PASADENA, Calif. -- NASA Television will provide commentary starting
at 2 p.m. EST (11 a.m. PST) on Friday, Feb. 15, during the close, but
safe, flyby of a small near-Earth asteroid named 2012 DA14. NASA
places a high priority on tracking asteroids and protecting our home
planet from them. This flyby will provide a unique opportunity for
researchers to study a near-Earth object up close.

The half-hour broadcast from NASA's Jet Propulsion Laboratory (JPL) in
Pasadena, Calif., will incorporate real-time animation to show the
location of the asteroid in relation to Earth, along with live or
near real-time views of the asteroid from observatories in Australia,
weather permitting.

At the time of its closest approach to Earth at approximately 2:25
p.m. EST (11:25 a.m. PST/ 19:25 UTC), the asteroid will be about
17,150 miles (27,600 kilometers) above Earth's surface.

The commentary will be available via NASA TV and streamed live online
at:
http://www.nasa.gov/ntv

and
http://www.ustream.tv/nasajpl2

In addition to the commentary, near real-time imagery of the
asteroid's flyby before and after closest approach, made available to
NASA by astronomers in Australia and Europe, weather permitting, will
be streamed beginning at about noon EST (9 a.m. PST) and continuing
through the afternoon at the following website:
http://www.ustream.tv/nasajpl2

A Ustream feed of the flyby from a telescope at NASA's Marshall Space
Flight Center in Huntsville, Ala., will be streamed for three hours
starting at 9 p.m. EST (8 p.m. CST). To view the feed and ask
researchers questions about the flyby via Twitter, visit:
http://www.ustream.tv/channel/nasa-msfc

The NASA Near Earth Objects (NEO) Program at the agency's headquarters
in Washington, manages and funds the search, study, and monitoring of
NEOs, or asteroids and comets, whose orbits periodically bring them
close to the Earth. NASA's study of NEOs provides important clues to
understanding the origin of our solar system. The objects also are a
repository of natural resources and could become waystations for
future exploration. In collaboration with other external
organizations, one of the program's key goals is to search and
hopefully mitigate potential NEO impacts on Earth. JPL conducts the
NEO program's technical and scientific activities.

For more information, including graphics and animations showing the
flyby of 2012 DA14, visit:
www.nasa.gov/asteroidflyby 

For more information about asteroids and near-Earth objects, visit:
http://www.jpl.nasa.gov/asteroidwatch

----------------
Press Release: Feb. 13, 2013

Steve Cole
Headquarters, Washington
202-358-0918
stephen.e.cole@nasa.gov

D.C. Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov

MEDIA ADVISORY: M13-031
2013 THE Year of Meteors, Asteroids, Comets, and MORE!!

05 February 2013

NASA to Host Asteroid 2012 DA14 Flyby Media Telecon 07FEB2013

2013 THE Year of Meteors, Asteroids, Comets, and MORE!!

JPL/NASA News 


News advisory: 2013-043  Feb. 4, 2013

NASA to Host Feb. 7 Media Telecon on Asteroid Flyby - 2012 DA14

NASA to Host Feb. 7 Media Telecon on Asteroid Flyby

















The full version of this story with accompanying images is at:

http://www.jpl.nasa.gov/news/news.php?release=2013-043&cid=release_2013-043


PASADENA, Calif. -- NASA will hold a media teleconference at 11 a.m. 
PST (2 p.m. EST), on Thursday, Feb. 7, to discuss an asteroid, 150 feet
 (45 meters) in diameter, that will pass close, but safely, by Earth on Feb. 
15. The flyby creates a unique opportunity for researchers to observe 
nd learn more about asteroids.


The teleconference participants are: --Lindley Johnson, program 
executive, Near-Earth Object (NEO) Observations Program, NASA 
Headquarters, Washington --Timothy Spahr, director, Minor Planet
 Center, Harvard-Smithsonian Center for Astrophysics, Cambridge, 
Mass. --Donald Yeomans, manager, NEO Office, Jet Propulsion 
Laboratory, Pasadena, Calif. --Amy Mainzer, principal investigator, 
NEOWISE observatory, Jet Propulsion Laboratory --Edward Beshore, 
deputy principal investigator, Origins-Spectral Interpretation-Resource 
Identification-Security-Regolith Explorer Asteroid Sample Return 
Mission, University of Arizona, Tucson


Audio of the teleconference will be streamed live at:

and


Related images will be available at the start of the teleconference at:
http://www.nasa.gov/mission_pages/asteroids/news/telecon20130207.html .


For detailed information concerning the Earth flyby of 2012 DA14, visit:
http://www.nasa.gov/topics/solarsystem/features/asteroidflyby.html .


A Ustream feed of the flyby from a telescope at NASA's Marshall Space
 Flight Center in Huntsville, Ala., will be broadcast from 6 p.m. to
 9 p.m. PST (9 p.m. to midnight EST) on Feb. 15. To view the feed
 and ask researchers questions via Twitter about the flyby, visit:

http://www.ustream.tv/channel/nasa-msfc .


DC Agle 818-393-9011

Jet Propulsion Laboratory, Pasadena, Calif.

agle@jpl.nasa.gov

--------
Dwayne Brown 202-358-1726

NASA Headquarters, Washington

Dwayne.c.brown@nasa.gov
---------

Nancy Neal Jones 301-286-0039

Goddard Space Flight Center, Greenbelt, Md.

nancy.n.jones@nasa.gov

01 September 2012

NEOs Asteroids Close Approach September 2012

NEOs Asteroids Close Approach September 2012

September 2012 will be an active month for fireballs and meteors.  Many more NEOs are yet to be discovered before the month is over; so check back as this table below is likely to have additions. Get outside and observe when able on clear nights.  The best time for viewing is from 10pm-4:30am.
Enjoy the night sky, stars, moon, planets, etc. and if luck several meteors! If you have a sighting of a meteor, fireball or bolide please file a sighting report and document with others. Thank You!
-LunarMeteorite*Hunter...Tokyo,Japan

UPCOMING CLOSE APPROACHES TO EARTH
AU = ~150 million kilometers
1 LD = Lunar Distance = ~384,000 kilometers
Object
Name
Close
Approach
Date
CA
Distance*
(AU)
CA
Distance*
(LD)
Estimated
Diameter**
H
(mag)
Relative
Velocity
(km/s)
(2012 QZ17) 2012-Sep-010.100138.922 m - 50 m25.45.88
(2012 LU7) 2012-Sep-020.120046.7430 m - 970 m18.98.16
(2012 FS35) 2012-Sep-020.154560.12.3 m - 5.2 m30.32.87
(2012 HG31) 2012-Sep-030.071627.9440 m - 990 m18.910.33
(2012 PX) 2012-Sep-040.045017.562 m - 140 m23.210.02
(2012 QC18) 2012-Sep-050.068426.642 m - 93 m24.06.08
(2012 EH5) 2012-Sep-050.161362.838 m - 84 m24.29.75
(2011 EO11) 2012-Sep-050.103440.29.0 m - 20 m27.48.81
(2007 PS25) 2012-Sep-060.049719.323 m - 52 m25.38.50
(2005 RZ2) 2012-Sep-070.099338.760 m - 130 m23.27.32
329520 (2002 SV) 2012-Sep-080.107641.9300 m - 670 m19.89.17
(2012 QD8) 2012-Sep-090.043516.965 m - 150 m23.119.58
(2012 PK24) 2012-Sep-090.064725.250 m - 110 m23.610.52
(2012 PM28) 2012-Sep-100.128750.168 m - 150 m23.017.64
(2011 ES4) 2012-Sep-100.179269.820 m - 44 m25.712.96
(2008 CO) 2012-Sep-110.184771.974 m - 160 m22.84.10
(2012 PZ19) 2012-Sep-130.090935.429 m - 66 m24.87.57
(2012 QG42) 2012-Sep-140.01917.4230 m - 520 m20.311.04
(2007 PB8) 2012-Sep-140.168265.5150 m - 340 m21.214.51
226514 (2003 UX34) 2012-Sep-140.188273.2260 m - 590 m20.025.74
(1998 QC1) 2012-Sep-140.164263.9310 m - 690 m19.717.11
(2012 QC8) 2012-Sep-140.058322.7690 m - 1.5 km17.920.37
(2002 EM6) 2012-Sep-150.183371.3270 m - 590 m20.018.56
(2002 RP137) 2012-Sep-160.162463.266 m - 150 m23.07.31
(2009 RX4) 2012-Sep-160.170166.215 m - 35 m26.28.35
(2001 QM142) 2012-Sep-170.046818.273 m - 160 m22.811.81
(2005 UC) 2012-Sep-170.199277.5280 m - 630 m19.97.55
(2012 FC71) 2012-Sep-180.107441.824 m - 53 m25.23.51
(1998 FF14) 2012-Sep-190.092836.1210 m - 480 m20.521.40
331990 (2005 FD) 2012-Sep-190.191474.5320 m - 710 m19.615.92
(2012 QG49) 2012-Sep-190.083932.681 m - 180 m22.69.44
(2009 SH2) 2012-Sep-240.146256.928 m - 62 m24.97.52
333578 (2006 KM103) 2012-Sep-250.062624.4260 m - 590 m20.08.54
(2002 EZ2) 2012-Sep-260.192274.8270 m - 610 m20.06.76
(2012 QF42) 2012-Sep-270.109942.8140 m - 300 m21.58.69
(2009 SB170) 2012-Sep-290.178969.6200 m - 440 m20.732.39
(2011 OJ45) 2012-Sep-290.133952.118 m - 39 m25.94.24
(2012 JS11) 2012-Sep-300.071227.7260 m - 590 m20.012.60
Source: NASA,JPL, - http://neo.jpl.nasa.gov/ca/

2012 THE Year of Meteors!

06 August 2012

Curious? Curiosity Has Landed on MARS! 05/06AUG2012

NASA Lands Car-Size Rover Beside Martian Mountain
Curiosity sends a VERY clear image from its Martian surroundings!
(CLICK on image to enlarge)
Source: NASA, JPL,CalTech



Curiosity`s First Photo From Mars
Source: NASA/JPL/CalTech
The full version of this story with accompanying images is at:
http://www.nasa.gov/mission_pages/msl/news/msl20120805c.html


PASADENA, Calif. -- NASA's most advanced Mars rover Curiosity has landed on the Red Planet. The one-ton rover, hanging by ropes from a rocket backpack, touched down onto Mars Sunday to end a 36-week flight and begin a two-year investigation.

The Mars Science Laboratory (MSL) spacecraft that carried Curiosity succeeded in every step of the most complex landing ever attempted on Mars, including the final severing of the bridle cords and flyaway maneuver of the rocket backpack.

"Today, the wheels of Curiosity have begun to blaze the trail for human footprints on Mars. Curiosity, the most sophisticated rover ever built, is now on the surface of the Red Planet, where it will seek to answer age-old questions about whether life ever existed on Mars -- or if the planet can sustain life in the future," said NASA Administrator Charles Bolden. "This is an amazing achievement, made possible by a team of scientists and engineers from around the world and led by the extraordinary men and women of NASA and our Jet Propulsion Laboratory. President Obama has laid out a bold vision for sending humans to Mars in the mid-2030's, and today's landing marks a significant step toward achieving this goal."

Curiosity landed at 10:32 p.m. Aug. 5, PDT, (1:32 a.m. EDT Aug. 6) near the foot of a mountain three miles tall and 96 miles in diameter inside Gale Crater. During a nearly two-year prime mission, the rover will investigate whether the region ever offered conditions favorable for microbial life.

"The Seven Minutes of Terror has turned into the Seven Minutes of Triumph," said NASA Associate Administrator for Science John Grunsfeld. "My immense joy in the success of this mission is matched only by overwhelming pride I feel for the women and men of the mission's team."

Curiosity returned its first view of Mars, a wide-angle scene of rocky ground near the front of the rover. More images are anticipated in the next several days as the mission blends observations of the landing site with activities to configure the rover for work and check the performance of its instruments and mechanisms.

"Our Curiosity is talking to us from the surface of Mars," said MSL Project Manager Peter Theisinger of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "The landing takes us past the most hazardous moments for this project, and begins a new and exciting mission to pursue its scientific objectives."

Confirmation of Curiosity's successful landing came in communications relayed by NASA's Mars Odyssey orbiter and received by the Canberra, Australia, antenna station of NASA's Deep Space Network.

Curiosity carries 10 science instruments with a total mass 15 times as large as the science payloads on the Mars rovers Spirit and Opportunity. Some of the tools are the first of their kind on Mars, such as a laser-firing instrument for checking elemental composition of rocks from a distance. The rover will use a drill and scoop at the end of its robotic arm to gather soil and powdered samples of rock interiors, then sieve and parcel out these samples into analytical laboratory instruments inside the rover.

To handle this science toolkit, Curiosity is twice as long and five times as heavy as Spirit or Opportunity. The Gale Crater landing site places the rover within driving distance of layers of the crater's interior mountain. Observations from orbit have identified clay and sulfate minerals in the lower layers, indicating a wet history.

The mission is managed by JPL for NASA's Science Mission Directorate in Washington. The rover was designed, developed and assembled at JPL. JPL is a division of the California Institute of Technology in Pasadena.

For more information on the mission, visit: http://www.nasa.gov/mars andhttp://marsprogram.jpl.nasa.gov/msl .

Follow the mission on Facebook and Twitter at: http://www.facebook.com/marscuriosity And http://www.twitter.com/marscuriosity .

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