Newly Discovered Trans-Neptunian Dwarf Planet

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In summary, astronomers have discovered a new dwarf planet, designated V774104, which is three times farther from the Sun than Pluto and is currently the most distant known object in the solar system. However, previous discoveries such as 90377 Sedna have been found to have a Semi-Major Axis of 506 AU and an Aphelion estimated to be ≈937 AU. Efforts to find new trans-Neptunian objects have not been successful, with surveys only detecting objects that were already known. There is still potential for new discoveries to be made in the outer solar system, especially with the upcoming launch of the James Webb Space Telescope.
  • #1
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Newly discovered dwarf planet is solar system’s most distant object

Astronomers have found a dwarf planet three times farther away from the Sun than Pluto, making it the most distant known object in the solar system. Designated V774104, the trans-Neptunian object is 500 to 1000 kilometres in diameter — half the size of Pluto — and currently lies 15.4 billion kilometres (9.6 billion miles) or 103 astronomical units (AU) from the Sun, but its exact orbit is yet to be determined.

Source: http://astronomynow.com/2015/11/12/...-planet-is-solar-systems-most-distant-object/


Contrary to what the article above states, before this discovery was made 90377 Sedna (2003 VB12) was the furthest trans-Neptunian dwarf planet in our solar system with Semi-Major Axis of 506 AU, and an Aphelion estimated to be ≈937 AU. The 103 AU distance the above article gives for V774104 is its estimated Perihelion.

Sources:
http://www.space.com/31100-most-distant-dwarf-planet-found.html
https://www.newscientist.com/articl...ystem-object-yet-could-hint-at-hidden-planet/
http://news.sciencemag.org/space/20...-solar-system-could-point-other-rogue-planets
http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=Sedna
 
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Thanks Glitch, for the interesting news and links! :smile:
 
  • #4
I think in the next few decades, well develop the technology to start detecting TNOs by the boatload. Maybe someone can correct me if I'm wrong, but I would think that our telescopes are currently seeing them, we just don't have the computer algorithms to be able to pull them out of the random background fluctuations.
 
  • #5
Given the large number of precovery images found for various objects: quite likely. We probably have observational data to discover thousands of objects in the solar system (mainly main-belt asteroids) - if there would be a way to combine and analyze everything together with unlimited CPU time.
 
  • #6
Once a planetary disk develops instabilities, orbits become elliptical and entropy in the system increases.
Objects mostly end up being launched to the outer edges of the solar system or are simply tossed out.
Gravitational capture or collision are statistically unlikely and bigger objects are less likely to be in unstable orbits.
Didn't anyone create a statistical distribution graph yet that plots object mass vs. the likelihood it is found at a certain distance from the main star?
 
  • #7
mfb said:
Given the large number of precovery images found for various objects: quite likely. We probably have observational data to discover thousands of objects in the solar system (mainly main-belt asteroids) - if there would be a way to combine and analyze everything together with unlimited CPU time.

This was already done. Mike Brown with colleagues pulled data from several wide-field surveys and ran it through software to find TNOs. They found all big known TNOs, but no unknown ones. Here's the post where he announced this sad result:

http://www.mikebrownsplanets.com/2008/09/end.html

I've seen a more detailed post where he explained in much more details what they did. Unfortunately, I failed to find it now. IIRC, the source survey data was down to ~19 magnitude. To find new TNOs, we need deeper surveys. I think there aren't (yet) wide field surveys to ~25 mag.

Edit: found it. In fact, found *them*.

They performed their own survey on 1.2 m Samuel Oschin Telescope at Palomar Observatory and here are the results published in 2010:

http://www.astro.yale.edu/mschwamb/Site/Publications_files/2010Schwamb.pdf

Then they processed data from other surveys, a bit less sensitive but covering more of the sky:

http://www.mikebrownsplanets.com/2015/01/ten-years-of-eris.html

They did not find any new bright TNOs:

"After 6 months of processing of 7 years worth of data, we found all of the bright Kuiper belt objects that we already knew (...).

And, so, a decade after that discovery of Eris, a decade after that moment in life when it seemed that the next huge discovery could be a single click away, I have to announce that it is really true: we are through with discoveries of bright new objects in the outer solar system."
 
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  • #8
nikkkom said:
This was already done. Mike Brown with colleagues pulled data from several wide-field surveys and ran it through software to find TNOs. They found all big known TNOs, but no unknown ones. Here's the post where he announced this sad result:

http://www.mikebrownsplanets.com/2008/09/end.html

I've seen a more detailed post where he explained in much more details what they did. Unfortunately, I failed to find it now. IIRC, the source survey data was down to ~19 magnitude. To find new TNOs, we need deeper surveys. I think there aren't (yet) wide field surveys to ~25 mag.

Edit: found it. In fact, found *them*.

They performed their own survey on 1.2 m Samuel Oschin Telescope at Palomar Observatory and here are the results published in 2010:

http://www.astro.yale.edu/mschwamb/Site/Publications_files/2010Schwamb.pdf

Then they processed data from other surveys, a bit less sensitive but covering more of the sky:

http://www.mikebrownsplanets.com/2015/01/ten-years-of-eris.html

They did not find any new bright TNOs:

"After 6 months of processing of 7 years worth of data, we found all of the bright Kuiper belt objects that we already knew (...).

And, so, a decade after that discovery of Eris, a decade after that moment in life when it seemed that the next huge discovery could be a single click away, I have to announce that it is really true: we are through with discoveries of bright new objects in the outer solar system."
I am amazed in this day and age that anyone would claim there would be no new discoveries to be made, when so many have said the same thing in the past and have been repeatedly proven wrong. The one constant seems to be that there are always new discoveries to be made.

I am looking forward to the new discoveries to be made by the James Webb Space Telescope.
 
  • #9
Glitch, please do not misrepresent what I (and Mike Brown) have said.
 
  • #10
nikkkom said:
Glitch, please do not misrepresent what I (and Mike Brown) have said.
If he did not find any new TNOs, clearly he missed V774104. Then to make a statement that "we are through with discoveries of bright new objects in the outer solar system" is difficult to misrepresent.
 
  • #11
|Glitch| said:
If he did not find any new TNOs, clearly he missed V774104. Then to make a statement that "we are through with discoveries of bright new objects in the outer solar system" is difficult to misrepresent.

Which part of word "bright" you do not understand?

V774104 has apparent magnitude of about 24. Mike Brown's surveys were sensitive to 21 at max.
 
  • #12
nikkkom said:
Which part of word "bright" you do not understand?

V774104 has apparent magnitude of about 24. Mike Brown's surveys were sensitive to 21 at max.
Apparently both you and Mike Brown have forgotten the aphorism "the absence of evidence is not the evidence of absence."
 
  • #13
Thread closed temporarily for Moderation...

EDIT -- Thread will remain closed.
 
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What is a Trans-Neptunian Dwarf Planet?

A Trans-Neptunian Dwarf Planet is a celestial body that orbits the Sun beyond Neptune, but is not large enough to be classified as a planet. It is typically smaller than the eight major planets in our Solar System and is composed mostly of ice and rock.

How was this Newly Discovered Trans-Neptunian Dwarf Planet found?

This newly discovered Trans-Neptunian Dwarf Planet was found using telescopes and other astronomical instruments. Scientists observed its movement and orbit around the Sun, and were able to confirm its existence based on its physical characteristics.

What makes this Newly Discovered Trans-Neptunian Dwarf Planet unique?

This newly discovered Trans-Neptunian Dwarf Planet is unique because it is the first of its kind to be found in this specific region of our Solar System. Its size, composition, and orbit differ from other known Trans-Neptunian Dwarf Planets, making it a valuable discovery for scientists.

Could this Newly Discovered Trans-Neptunian Dwarf Planet support life?

Currently, there is no evidence to suggest that this newly discovered Trans-Neptunian Dwarf Planet could support life. It is too far from the Sun to receive enough heat and light to sustain life, and its composition is mostly ice and rock. However, further research and exploration may reveal more about its potential for supporting life.

What implications does this Newly Discovered Trans-Neptunian Dwarf Planet have for our understanding of the Solar System?

This newly discovered Trans-Neptunian Dwarf Planet expands our knowledge and understanding of the vastness of our Solar System. Its discovery raises questions about the formation and evolution of our Solar System, and may provide insights into the existence of other similar celestial bodies that are yet to be discovered.

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