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cover of episode Finding Pluto’s Potential Replacement with a Giant New Telescope

Finding Pluto’s Potential Replacement with a Giant New Telescope

2025/1/10
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Clara Moskowitz
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Rachel Feltman
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Clara Moskowitz: 我认为我们太阳系中可能存在一颗我们从未见过的第九行星。这颗行星的大小可能是地球的五到十倍。虽然我们目前还没有直接观测到它,但一些海王星外天体的奇特轨道暗示了它的存在。这些天体的轨道非常长且倾斜,这很难用现有的模型解释,除非存在一个大型天体对其产生影响。薇拉·鲁宾天文台的建成将极大地提高我们发现更多太阳系外围天体,甚至第九行星本身的可能性。它将扫描整个南天,并创建详细的天体运动图谱。如果我们发现更多具有相似奇特轨道的物体,这将支持第九行星的存在。反之,如果发现的物体轨道随机,则会削弱第九行星的假设。即使我们无法直接观测到第九行星,如果我们收集到足够的数据,通过计算机模拟证明这些天体的运动只有在存在第九行星的情况下才能解释,那么它的存在将得到广泛认可。 此外,薇拉·鲁宾天文台的观测结果将有助于我们更好地了解暗物质和暗能量,并发现潜在的危险小行星。 Rachel Feltman: 我很好奇,冥王星被降级的原因是什么?为什么假设中的第九行星如果存在,仍然可以被认为是行星?冥王星被降级的原因与第九行星的假设有关。2005年,天文学家发现了比冥王星更大的天体埃里斯,这引发了对行星定义的重新思考。国际天文联合会制定了新的行星定义标准,包括围绕恒星运行、自身引力使其呈球形以及清除轨道附近其他天体的三个条件。冥王星未能清除其轨道附近的其他天体,因此被降级为矮行星。而第九行星的假设,则源于对海王星外一些天体奇特轨道的观察。这些天体的轨道非常长且倾斜,这很难用现有的模型解释,除非存在一个大型天体对其产生影响。因此,如果我们能找到足够多的证据来证明存在一个大型天体影响着这些天体的轨道,即使我们没有直接观测到它,第九行星的假设也可能得到广泛认可。

Deep Dive

Key Insights

What is the Vera Rubin Observatory, and why is it significant in the search for Planet Nine?

The Vera Rubin Observatory is a new telescope set to come online in 2025, located in Chile. It features the largest camera in the world and will scan the southern sky every few days, creating detailed maps. This capability makes it ideal for discovering distant objects, including potential Planet Nine, by identifying their orbits and movements. Its advanced technology will significantly expand our catalog of outer solar system objects, helping to determine whether Planet Nine exists.

Why was Pluto demoted from being a planet, and how does this relate to the search for Planet Nine?

Pluto was demoted in 2006 after the discovery of Eris, a larger object in the outer solar system. This led astronomers to redefine what qualifies as a planet: it must orbit a star, be spherical due to gravity, and clear its orbit of other debris. Pluto failed the third criterion, as it shares its orbit with other objects. This redefinition sparked the search for Planet Nine, as astronomers began finding other distant objects with unusual orbits, suggesting the gravitational influence of a hidden planet.

What evidence suggests the existence of Planet Nine?

Evidence for Planet Nine comes from the unusual orbits of extreme trans-Neptunian objects (ETNOs) like Sedna. These objects have highly elongated, tilted orbits that differ significantly from the flat plane of the solar system. Their orbits suggest the gravitational influence of a large, unseen object. Additionally, the clustering of these orbits and their alignment point to the possibility of a hidden planet shaping their paths.

What are some alternative explanations for the unusual orbits of distant solar system objects?

Alternative explanations include the possibility that the observed objects are outliers, and more typical objects with normal orbits remain undiscovered. Another theory is that a rogue planet or passing star influenced these orbits long ago. Some astronomers have even proposed the existence of a hidden black hole in the outer solar system, which could gravitationally affect these objects.

How far away could Planet Nine be, and why is it so hard to detect?

Planet Nine could be as far as 700 times the Earth-Sun distance, making it extremely distant and dim. For comparison, Neptune, the farthest official planet, is only 30 times this distance. Even with advanced telescopes like the Vera Rubin Observatory, detecting such a distant and relatively small object (5-10 times Earth's size) remains a significant challenge.

What role does Mike Brown play in the search for Planet Nine?

Mike Brown, a Caltech astronomer, is a key figure in the search for Planet Nine. He discovered Eris, which led to Pluto's demotion, and now advocates for the existence of Planet Nine based on the unusual orbits of distant objects. His work has been instrumental in shaping the debate around both Pluto and the potential discovery of a new planet.

What other scientific questions could the Vera Rubin Observatory help answer?

The Vera Rubin Observatory will aid in detecting potentially hazardous asteroids, studying dark matter, and exploring dark energy. By mapping the movement of objects in the solar system and beyond, it will provide insights into the distribution of dark matter and help refine our understanding of these mysterious cosmic phenomena.

Chapters
This chapter explores the demotion of Pluto from its planetary status in 2006 and how this event led to the hypothesis of Planet Nine. It introduces the discovery of Eris and the subsequent need to define what constitutes a planet, highlighting the criteria that Pluto failed to meet.
  • Pluto's demotion in 2006
  • Discovery of Eris, larger than Pluto
  • New definition of a planet: orbit a star, be round, clear its orbit
  • Pluto's failure to clear its orbit

Shownotes Transcript

Pluto was unseated as our solar system’s ninth planet in 2006. Since then astronomers have found signs that a real ninth planet could be hiding at the edges of our solar system. Clara Moskowitz, senior editor for space and physics, explains how the forthcoming Vera Rubin Observatory could give researchers a way to find the real Planet Nine—if it’s out there.

Recommended reading:

We May Be on the Brink of Finding the Real Planet Nine)

How to Move the World’s Largest Camera from a California Lab to an Andes Mountaintop)

E-mail us at [email protected]) if you have any questions, comments or ideas for stories we should cover!

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Science Quickly is produced by Rachel Feltman, Fonda Mwangi, Kelso Harper, Madison Goldberg and Jeff DelViscio. This episode was hosted by Rachel Feltman with guest Clara Moskowitz, senior editor for space and physics. Our show is edited by Madison Goldberg with fact-checking by Emily Makowski, Shayna Posses and Aaron Shattuck.  The theme music was composed by Dominic Smith.

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