Posted on 01/03/2010 7:26:46 PM PST by SunkenCiv
Our understanding of the Kuiper belt has changed dramatically in these past five years. The best example of this change comes, I think, from the discovery of a large Kuiper belt object that was announced just a few days ago... But, by decoding the numbers, I could tell it was something that had just been discovered a few days before. Like anyone else, my first attempt to know more was a quick trip to Google.
Ah ha! A new large Kuiper belt object found from a telescope Chile, by David Rabinowitz! Yes, the same David Rabinowitz from the Haumea discovery. He has moved on to Chile to try to make newer discoveries from there, discoveries in parts of the sky that we didn't look at back when we were working at Palomar Observatory outside of San Diego.
Based on preliminary information, it looked likely the 9th largest Kuiper belt object ever found. David was clearly on to something good here...
Based on its brightness it might well be a perfect size to test one of my new theories about medium-sized Kuiper belt objects. I feel like I now understand the largest objects, and I fear that I will never understand the smallest objects, but the middle ones are within grasp, if we can just find a few more to test some pet theories about them. For 2009 YE7 to be a good candidate for my theory we need to know if it has a moon, what color it is, and what materials are on its surface. Then we'll see. I started thinking about where 2009 YE7 is in the sky, what telescopes I could use to point at it, how to time the observations.
(Excerpt) Read more at mikebrownsplanets.com ...
Discovery[1]
|
|
---|---|
Discovered by | David Rabinowitz |
Discovery date | December 17, 2009(?) |
Designations
|
|
MPC designation | 2009 YE7 |
Minor planet category |
TNO Cubewano[2] Haumea family?[3] |
Epoch December 15, 2009 (2455180.5) | |
Aphelion | 51.1 AU (Q) |
Perihelion | 35.9 AU (q) |
Semi-major axis | 43.5 AU (a) |
Eccentricity | 0.17 |
Orbital period | 287 yr |
Mean anomaly | 180° (M) |
Inclination | 29.2° |
Longitude of ascending node | 138° |
Argument of perihelion | 96° |
Satellites | ? |
Physical characteristics
|
|
Dimensions | 440[4]-945[5] km[2][6] |
Albedo | assume 0.7 to 0.15 |
Apparent magnitude | ~20(?)(JPL Horizons) |
Absolute magnitude (H) | 2.8[2] |
|
2009 YE7 is a trans-Neptunian object with an absolute magnitude of 2.8.[2] This qualifies it as a dwarf planet candidate. It was discovered by David Rabinowitz on December 17, 2009 at the La Silla Observatory in Chile. 2009 YE7 is the first bright KBO found from the southern hemisphere.
Discovery[1]
|
|
---|---|
Discovered by | David Rabinowitz |
Discovery date | December 17, 2009(?) |
Designations
|
|
MPC designation | 2009 YE7 |
Minor planet category |
TNO Cubewano[2] Haumea family?[3] |
Epoch December 15, 2009 (2455180.5) | |
Aphelion | 51.1 AU (Q) |
Perihelion | 35.9 AU (q) |
Semi-major axis | 43.5 AU (a) |
Eccentricity | 0.17 |
Orbital period | 287 yr |
Mean anomaly | 180° (M) |
Inclination | 29.2° |
Longitude of ascending node | 138° |
Argument of perihelion | 96° |
Satellites | ? |
Physical characteristics
|
|
Dimensions | 440[4]-945[5] km[2][6] |
Albedo | assume 0.7 to 0.15 |
Apparent magnitude | ~20(?)(JPL Horizons) |
Absolute magnitude (H) | 2.8[2] |
|
2009 YE7 is a trans-Neptunian object with an absolute magnitude of 2.8.[2] This qualifies it as a dwarf planet candidate. It was discovered by David Rabinowitz on December 17, 2009 at the La Silla Observatory in Chile. 2009 YE7 is the first bright KBO found from the southern hemisphere.
· join · view topics · view or post blog · bookmark · post new topic · subscribe · | ||
Google news searches: exoplanet · exosolar · extrasolar · | ||
Real Occult Science: Hubble Spots Smallest Comet Vagabond by Ray Villard, Wed Dec 16, 2009 02:47 PM ET
Discovery[1]
|
|
---|---|
Discovered by | David Rabinowitz |
Discovery date | December 17, 2009(?) |
Designations
|
|
MPC designation | 2009 YE7 |
Minor planet category |
TNO Cubewano[2] Haumea family?[3] |
Epoch December 15, 2009 (2455180.5) | |
Aphelion | 51.1 AU (Q) |
Perihelion | 35.9 AU (q) |
Semi-major axis | 43.5 AU (a) |
Eccentricity | 0.17 |
Orbital period | 287 yr |
Mean anomaly | 180° (M) |
Inclination | 29.2° |
Longitude of ascending node | 138° |
Argument of perihelion | 96° |
Satellites | ? |
Physical characteristics
|
|
Dimensions | 440[4]-945[5] km[2][6] |
Albedo | assume 0.7 to 0.15 |
Apparent magnitude | ~20(?)(JPL Horizons) |
Absolute magnitude (H) | 2.8[2] |
|
2009 YE7 is a trans-Neptunian object with an absolute magnitude of 2.8.[2] This qualifies it as a dwarf planet candidate. It was discovered by David Rabinowitz on December 17, 2009 at the La Silla Observatory in Chile. 2009 YE7 is the first bright KBO found from the southern hemisphere.
Astronomy ping!
Disclaimer: Opinions posted on Free Republic are those of the individual posters and do not necessarily represent the opinion of Free Republic or its management. All materials posted herein are protected by copyright law and the exemption for fair use of copyrighted works.