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SpaceX首份财报将至：紧盯星链业务与算力开支，千亿解禁能否平稳落地？_我的网站

一 |     财联社7月21日讯（编辑 李莹）SpaceX将公布其上市以来的首份财报。    

    Schematic diagram of Milky Way Photo: Courtesy of Purple Mountain Observatory (PMO)
Chinese astronomers have discovered that the Milky Way is not a simple, smoothly warped disk, but contains widespread "wrinkle-like" structures resembling ripples on a water surface, providing new clues to understanding the galaxy's 3D structure and evolutionary history.
The discovery was made by a research team from the Purple Mountain Observatory (PMO) under the Chinese Academy of Sciences, using data from the "Milky Way Imaging Scroll Painting" (MWISP) survey. The findings were published online titled "Widespread corrugations superimposed on the Galactic warp in the outer CO disk" in the journal Nature Astronomy on August 7.
For decades, astronomers have known that the Milky Way's disk is not perfectly flat. Instead, its outer regions are slightly bent upward on one side and downward on the other - a structure known as a galactic warp.
However, the latest study shows that this large-scale bending is not the whole story. Smaller-scale vertical fluctuations are also embedded within the warped disk, creating a more complicated 3D structure.
"In many illustrations and in the public imagination, the Milky Way looks like a flat vinyl record," Sun Yan, associate researcher at PMO and the first author of the paper, told the Global Times on Tuesday. "In reality, the outer part of the Milky Way is more like a record that has been heated and deformed, with one side lifted and the other side lowered. That is the warp. On top of this large-scale deformation, there are additional smaller waves, which we call corrugations," Sun explained.
Using a more everyday analogy, Sun compared the Milky Way's structure to a sea surface. The warp is like a large swell that changes the overall height of the ocean, while corrugations are smaller waves superimposed on that swell.
"The two structures exist together. In our data analysis, we first removed the large-scale warp model, which allowed us to reveal the smaller wave-like patterns hidden underneath," Sun said.
The research focused on the Milky Way's outer gas disk rather than the more familiar stellar disk. According to Sun, cold molecular gas and stars provide two complementary ways to study the galaxy.
"Molecular gas is a sensitive probe for studying the vertical structure and dynamics of the galactic disk because it is concentrated near the disk plane and responds strongly to disturbances," she said.
Molecular gas is also the raw material for star formation, meaning its distribution is closely connected with the formation of young stars. The researchers traced this gas through carbon monoxide (CO) emission, which can penetrate regions obscured by interstellar dust and provide a different perspective from optical observations of stars.
The breakthrough was made possible by the MWISP survey, conducted using China's 13.7-meter millimeter-wave telescope. 
"MWISP can be understood as giving the Milky Way a large-scale medical examination using millimeter-wave observations," Sun said.
Previous CO surveys were limited in sensitivity and coverage, making it difficult to accurately study the distant outer regions of the galaxy. In contrast, the latest study identified more than 30,000 molecular cloud samples, covering about half of the Milky Way's outer disk and extending to a distance of about 26 kiloparsecs from the Galactic center.
With such a large dataset, researchers were able to first establish a model of the overall warp and then separate subtle structures from the background. The newly identified corrugations have radial wavelengths of about 3.9-7.9 kiloparsecs and vertical amplitudes of about 100-200 parsecs.
The study also identified a corrugation structure extending about 40 kiloparsecs in azimuth at a distance of around 12.7 kiloparsecs from the Galactic center. In some spiral arm regions, vertical displacements can reach approximately 200 parsecs.
The researchers believe these large-scale vertical fluctuations are likely related to "bending waves" triggered by external gravitational disturbances, suggesting that the Milky Way might have experienced more complex interactions during its evolutionary history.
Although the newly discovered structures sound dramatic, they do not have any direct impact on Earth or the solar system. "Humans cannot directly sense these corrugations," Sun said. "Their scales reach thousands or even tens of thousands of light-years, and even if these structures are evolving, such changes would not be directly perceptible on human timescales."
The study focuses on the outer disk of the Milky Way and does not include the region around the solar system. "There is currently no evidence that these structures have any observable influence on Earth's environment," Sun said.
Instead, their significance lies in what they reveal about the past. Like geological layers recording Earth's history, these galactic structures preserve traces of the Milky Way's evolutionary journey, the researchers explained.
Researchers said future studies combining more precise motion measurements and numerical simulations could further reveal the origins of these structures and their role in the long-term evolution of the Milky Way.
。投资者需重点关注财报哪些核心指标？财报公布后解禁的股份会遭到市场抢购，还是出现抛售踩踏？          SpaceX宣布将于2026年8月4日（周二）美股收盘后发布2026年第二季度财报。         这份二季度财报不仅是SpaceX登陆纳斯达克后，市场首次完整窥见公司真实财务基本面的官方窗口，财报落地还将触发金融史上规模巨大的一批内部限售股解禁。

二 |          据SpaceX分阶段限售协议，首批符合解禁条件的内部人士与全体员工所持股份中的20%（合计最高9.115亿股），将在本次二季度财报发布后的第二个交易日解除限售。         按当前每股119.85美元的最新股价测算，本次一次性解禁股份对应的流通市值约1092亿美元，约为SpaceX基础IPO募资总额750亿美元的1.45倍；对比来看，本次新增可流通筹码体量超过IPO对外发行的全部公众流通股，潜在抛压巨大。

三 |          财报核心看点          SpaceX需向市场证明，公司在星舰迭代研发与AI算力基建上的数十亿美元巨额开支，可由星链与发射业务强劲的经营性现金流所覆盖，从而支撑自由现金流的动态平衡。         星链盈利能力与用户增长： 星链是SpaceX商业收入的核心增长引擎。投资者重点应跟踪两大指标：全球新增用户总量与单用户平均收入（ARPU）。         由于星链业务向新兴市场低价下沉，ARPU 存在下滑压力，投资者需要验证：用户规模扩张带来的规模效应能否对冲单价下行，从而持续抬升星链业务的毛利率。

四 |          猎鹰9号发射业务与星舰研发投入： 猎鹰9号成熟的复用发射业务单机毛利率超70%，占据全球商业发射绝大部分份额，是公司稳定的“现金牛”。         然而，整体航天板块的自由现金流与净利润受星舰大额研发支出与资本开支拖累。评估重点在于区分猎鹰常规发射的经营性现金流造血能力，能否有效覆盖星舰的持续投入。         xAI算力基建资本投入：随着SpaceX于2月完成对xAI的收购，AI板块已成为集团当前最大的“现金消耗板块”。2026年一季度，AI 基础设施单季资本开支达77.2亿美元，占集团总资本投入的76%。         目前，市场亟需从财报与更新的招股书中厘清地面超算基地与卫星轨道算力配套的中长期资本支出节奏，并评估Grok大模型在企业级付费与商业化变现上的落地进度。         业绩指引与市场估值匹配度：当前该股估值处于行业高位区间，SpaceX必须交出亮眼的营收增速，同时给出清晰、可持续的现金流兑现路径，才能支撑长期估值逻辑。         业内指出，8月4日将成为SpaceX发展历程中的关键分水岭。若管理层交出强劲经营数据、明确长期业绩指引，且星链毛利率持续改善，市场买盘或足以消化员工与早期投资者集中抛售带来的海量新增流通筹码。         反之，若财报不及市场预期，基本面走弱叠加近1100亿美元新增可流通股份的双重压力，将持续拖累SpaceX整个夏末阶段的股价表现。

五 |          解禁安排细则          第一批次：2026年8月二季度财报发布后第二个交易日，员工与早期投资者所持股份的20%无条件解除限售。         该批次内，一定的价格条件会触发附加批次。若财报披露前连续10个交易日内，有5个交易日股价站稳175.50美元上方，可同步额外解禁10%股份（约4.558亿股）。基于现在的股价情况，业内普遍推断较难触发该附加批次。         第二批次：自IPO上市后第70天（8月21日）起解禁7%股份（约3.2亿股）。

六 |          第三至第六批：2026 年下半年固定间隔分批解锁，分别为上市后 90/105/120/135 天，每批释放7%股份。         （财联社 李莹）。

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