Newly Discovered Trans-Neptunian Dwarf Planet

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Discussion Overview

The discussion centers around the discovery of a newly identified trans-Neptunian dwarf planet, designated V774104, which is reported to be the most distant known object in the solar system. Participants explore the implications of this discovery, the technology for detecting trans-Neptunian objects (TNOs), and the challenges associated with finding new celestial bodies in the outer solar system.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants note that V774104 is three times farther from the Sun than Pluto, with a diameter estimated between 500 to 1000 kilometers.
  • Others argue that the article's claim about V774104 being the most distant object is misleading, as 90377 Sedna was previously considered the furthest known TNO.
  • There is speculation about the future capabilities of technology to detect TNOs more effectively, with some suggesting that current telescopes may already be capturing data on these objects, but algorithms may not yet be able to identify them.
  • One participant mentions that significant observational data exists that could potentially reveal thousands of objects, contingent on the ability to analyze this data comprehensively.
  • Concerns are raised regarding the statistical likelihood of finding objects at various distances from the Sun, with a call for a distribution graph to illustrate this relationship.
  • Some participants reference past surveys conducted by Mike Brown and colleagues, noting that while they found known TNOs, they did not discover any new bright objects, leading to a claim that future discoveries may be limited.
  • Another participant expresses skepticism about the assertion that no new discoveries remain, citing historical instances where such claims have been proven wrong.
  • Disagreement arises over the interpretation of Mike Brown's findings, particularly regarding the apparent magnitude of V774104 and the sensitivity of previous surveys.

Areas of Agreement / Disagreement

Participants exhibit disagreement regarding the implications of Mike Brown's surveys and the potential for future discoveries of TNOs. While some express confidence in ongoing discoveries, others challenge the notion that the search for new objects has reached its limit.

Contextual Notes

Participants reference various sources and past surveys, highlighting limitations in current observational capabilities and the need for deeper surveys to discover new TNOs. The discussion reflects uncertainty about the definitions and classifications of celestial objects.

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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:
 
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.
 
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.
 
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?
 
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."
 
Last edited:
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.
 
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
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