To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

2013 YP139
Near-Earth asteroid 2013 YP139—the six red dots in the composite image by NEOWISE specify the location of the asteroid. The inset is an enlargement of the image of 29 December 2013.
Discovery[1]
Discovered byNEAT[2]
NEOWISE[3]
Discovery sitePalomar Obs.[2]
Earth orbit[3]
Discovery date29 June 2002[2]
29 December 2013[3]
Designations
2013 YP139
2013 YP139 · 2002 MU7
NEO · Apollo · PHA[2][4]
Orbital characteristics[4]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc11.58 yr (4,231 days)
Aphelion4.0373 AU
Perihelion0.7603 AU
2.3988 AU
Eccentricity0.6831
3.72 yr (1,357 days)
61.262°
0° 15m 55.08s / day
Inclination0.8171°
292.13°
83.598°
Earth MOID0.0040 AU (1.56 LD)
Physical characteristics
Mean diameter
0.402±0.026 km[5]
0.650 km[1]
0.025±0.006[5]
21.6[4]

2013 YP139 is a dark sub-kilometer asteroid on a highly eccentric orbit, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 400 meters (1,300 feet) in diameter.[4]

It was first observed as 2002 MU7 by NEAT at Palomar Observatory on 29 June 2002, and by the WISE space telescope on 29 December 2013, under its current, principal provisional designation.[2][3] This object was the first possible discovery of the reinstated NEOWISE program of the WISE telescope, following the program's hibernation in 2011.[1]

YouTube Encyclopedic

  • 1/3
    Views:
    1 787
    4 353
    350
  • New research shows events like Chelyabinsk asteroid may happen more frequently
  • ALERT! Asteroid 2014 AZ5 To Hit the Earth?
  • ANOTHER BUS SIZED ASTEROID GIVES THE EARTH A REALLY CLOSE SHAVE!! May 3, 2014

Transcription

Orbit and classification

2013 YP139 belongs to the Apollo asteroids, which cross the orbit of Earth. They are the largest group of near-Earth objects with nearly 10 thousand known members.

This object orbits the Sun at a distance of 0.76–4.0 AU once every 3 years and 8.6 months (1,357 days; semi-major axis of 2.40 AU). Its orbit has an eccentricity of 0.68 and an inclination of 1° with respect to the ecliptic.[4] Due to this close proximity, NASA has classified this object as a potential threat. At the time of the first WISE observations, this object was moving at a rate of 3.2° per day (for comparison the apparent diameter of the Moon is 0.5°).[6]

Close approaches

2013 YP139 has a minimum orbital intersection distance with Earth of 0.00397 AU (594,000 km; 369,000 mi), which corresponds to 1.6 lunar distances (LD).[4] In August 2002 and December 2013, approached Earth at 4.1 LD and 94 LD, respectively. On 12 December 2069, it will pass Earth at a nominal distance of 0.007911 AU (1,180,000 km; 735,000 mi), or nearly 3 LD.[4] It also makes close approaches to Jupiter, Venus, Mars and the Moon.[4]

First WISE observations

The Wide-field Infrared Survey Explorer's Near-Earth Object WISE (NEOWISE) program was put into hibernation on 1 February 2011, following several program extensions,[7] from which approximately 34,000 asteroids were detected.[1] On 21 August 2013, however, the program was reactivated.[7] The new mission of the NEOWISE was to identify the population of potentially hazardous near-Earth objects.

2013 YP139 was first observed on 29 December 2013, at a distance of 0.235 astronomical units (35,200,000 kilometres; 21,800,000 miles) from Earth, marking the first object detected since the program's reinstatement. The infrared brightness was the primary attribute used for ascertaining the approximate size of the asteroid. Over the course of half a day, the trajectory of the asteroid was observed against the stationary positioning of the stars in the background.[1]

The data from the Wide-field Infrared Survey Explorer was transmitted to the Infrared Processing and Analysis Center at the California Institute of Technology, located in Pasadena, California. To confirm the discovery, researchers at the University of Arizona utilized the Spacewatch telescope at the Kitt Peak National Observatory in Tucson, Arizona. 2013 YP139 is considered by NASA to be the first in what is expected to be thousands of objects to be detected by NEOWISE's new mission.[8] Due to the trajectory of the asteroid, which puts it within a potentially dangerous range in over one hundred years following its discovery, NASA stated that they would keep a watchful eye on it.[1]

Physical characteristics

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, 2013 YP139 measures 0.402 kilometers in diameter and its surface has an exceptionally low albedo of 0.025.[5] Estimates from 2014 gave a somewhat larger diameter of 0.650 kilometers (0.404 miles).[1] Its very dark surface, has an albedo comparable to a piece of coal.[1]

See also

References

  1. ^ a b c d e f g h Agle, DC; Webster, Guy; Brown, Dwayne (7 January 2014). "Recently Reactivated NASA Spacecraft Spots Its First New Asteroid". NASA.
  2. ^ a b c d e "2013 YP139". Minor Planet Center. Retrieved 24 February 2018.
  3. ^ a b c d "List of the Potentially Hazardous Asteroids (PHAs)". Minor Planet Center. Retrieved 24 February 2018.
  4. ^ a b c d e f g h "JPL Small-Body Database Browser: (2013 YP139)" (2014-01-28 last obs.). Jet Propulsion Laboratory. Retrieved 24 February 2018.
  5. ^ a b c Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. Retrieved 24 February 2018.
  6. ^ "NEOWISE's New Find". NASA. 7 January 2014. Retrieved 10 January 2014.
  7. ^ a b "Wide-field Infrared Survey Explorer". Astro.ucla.edu. Retrieved 10 January 2014.
  8. ^ "NEOWISE's New Find". Planetary Science Institute. Retrieved 10 January 2014.

External links

This page was last edited on 12 April 2024, at 02:51
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.