在最初的9亿年里,最明亮的星系的快速进化
Rychard J Bouwens1, Garth D Illingworth
1UCO/Lick Observatory and Department of Astronomy, University of California Santa Cruz, Santa Cruz, California 95064, USA. bouwens@ucolick.org
Nature
|September 15, 2006
概括
早期的星系形成仍然是神秘的. 这项研究发现,大爆炸后大约7亿年,非常发光的星系是罕见的,这表明宇宙太年轻,无法形成它们.
科学领域:
- 宇宙学的宇宙学是什么?
- 银河系的形成和进化
- 早期宇宙天体物理学 天体物理学
背景情况:
- 大爆炸后的第一个9亿年 (米尔) 的星系形成 (直到红移z ≈6) 在很大程度上是未被探索的.
- 虽然星系样本存在于z ≈ 6,但早期的检测是不确定的,这在理解从第一颗恒星 (z ≈ 12-15) 到z ≈ 6的星系组合方面留下了空白.
研究的目的:
- 为了研究大爆炸后z ≈ 7-8的星系数量,大约700万年.
- 为了确定发光星系在早期宇宙中是否常见或罕见.
主要方法:
- 利用了最深度的近红外和光学成像数据.
- 使用保守和不那么保守的选择标准,搜索了z ≈ 7-8红移的候选星系.
主要成果:
- 在保守的标准下,只有一个候选星系在z ≈7-8发现,而如果没有从z ≈6进化,预计会有十个候选星系.
- 使用不那么保守的标准,发现了四个候选者,而没有进化,预计有17个候选者.
- 这表明非常发光的星系在z ≈ 7-8时是罕见的.
结论:
- 在z ≈ 7-8的发光星系稀缺性表明,宇宙太年轻了,无法通过等级融合形成显著的人口.
- 这些发现暗示早期宇宙中发光星系的数量很少,这挑战了快速星系聚集的模型.
相关概念视频
Speciation Rates
18.8K
Overview
18.8K
What is Evolutionary History?
31.1K
Scientists record evolutionary history by analyzing fossil, morphological, and genetic data. The fossil record documents the history of life on Earth and provides evidence for evolution. However, both fossil and living organisms offer evidence that outlines Earth’s evolutionary history.
31.1K
Gene Duplication and Divergence
6.8K
The seminal work of Ohno in 1970 popularized the idea of gene duplication and divergence. DNA sequence comparison studies reveal that a large portion of the genes in bacteria, archaebacteria, and eukaryotes was generated by gene duplication and divergence, indicating its critical role in evolution.
The duplicated copies of the gene are called Paralogs. Paralogs with similar sequences and functions form a gene family. Across several species, a large number of gene families are...
The duplicated copies of the gene are called Paralogs. Paralogs with similar sequences and functions form a gene family. Across several species, a large number of gene families are...
6.8K
Detection of Black Holes
1.7K
Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
1.7K
Origin of Photosynthesis
112
Photosynthesis represents a fundamental biological process that transformed Earth's atmosphere and paved the way for complex life. Emerging roughly 3.4–3.8 billion years ago, the earliest photosynthetic organisms harnessed light energy to produce organic compounds. These anoxygenic phototrophs used electron donors like hydrogen sulfide (H₂S) or ferrous iron (Fe²⁺), rather than water, and did not release molecular oxygen (O₂) as a byproduct. Various groups, including...
112
Evolution of New Traits in Microbes
199
Microorganisms evolve rapidly due to their large population sizes and short generation times, often exhibiting measurable changes within days under laboratory conditions. Natural selection acts on standing genetic variation, enabling the retention and amplification of beneficial traits that confer fitness advantages in changing environments.Adaptive Pigment Regulation in RhodobacterIn Rhodobacter, a genus of purple non-sulfur bacteria, light-harvesting pigments such as bacteriochlorophyll and...
199


