压裂/压力泵送

石油工程如何帮助解释火星裂缝之谜

火星车任务期间在火星上发现的天然裂缝可能非常重要,值得将它们带回地球。

jpt_23_natural_fractures_mars2.jpg
美国宇航局好奇号火星探测器拍摄的露头图像显示,轮廓分明的矿脉充满了白色矿物质,被解释为硫酸钙。
资料来源:美国宇航局。

当石油和天然气行业的研究工作因 COVID-19 大流行而放缓时,学术界的许多人被迫寻找新的方法来使自己的研究组合多样化。对于一些人来说,这意味着更深入地研究气候科学和碳管理的主题。

对于迈赫迪·莫赫塔里 (Mehdi Mokhtari) 来说,它还创造了一个利用石油和天然气研究产生的地球科学来帮助探索另一个世界的机会。

路易斯安那大学莱菲特分校石油工程系的副教授最近发表了一项研究,认为美国宇航局应该在计划于未来十年的任务中将火星上的自然断裂的岩石样本带回地球。

这位岩石力学专家和长期的太空探索爱好者表示,这项研究的想法是在他回忆起美国宇航局的好奇号漫游车任务及其发回的破碎岩石图像后产生的。

“裂缝中有这些凹陷和翼状结构,”他谈到在这颗红色星球上发现的裂缝时说道,“我知道它们看起来与我们在一些非常规地层中看到的一些复杂的裂缝模式非常相似。” 这非常有趣,让我想看看是否可以将我们在地球上所知道的与我们在火星上所看到的联系起来。”

但莫赫塔里和他的研究团队最关注的是含有矿物填充裂缝或矿脉的火星岩石,他说这些岩石代表了“火星上过去存在水的线索和证据,当然,美国宇航局正在试图回答一个大问题。”

2012 年,好奇号降落在一个名为盖尔陨石坑的地点,在那里它使用一种名为“hemCam”的工具分析了火星岩石的矿物学。激光光谱仪技术证实,一些裂隙岩石中充满了硫酸钙,大多数人称为石膏。

在地球上,我们知道这种矿化作用通常比主岩裂缝形成的时间晚数百万年。如果这些知识可以通过分析火星上的裂缝来证实,那么它将帮助我们了解水在其古代历史中所扮演的角色,以及可能大部分水的去向。

与此同时,莫赫塔里和其他人正在转向的地方之一是犹他州,据信那里的泥岩露头与近年来在火星上发现的裂隙岩石非常相似。

jpt_23_mars_utah_cores.JPG
(a) 火星黄刀湾羊床部分的“John Klein”钻孔中的矿化细脉,旁边的图像 (b) 显示了犹他州 Moenkopi 泥岩地层的核心。
资料来源:美国宇航局/路易斯安那大学拉斐特分校。

路易斯安那大学拉斐特分校的团队所做的不同之处在于,他们使用数字图像相关(DIC)来研究犹他州露头中发现的裂缝和静脉,以推测它们可能是如何形成的。该大学研究团队几年前率先使用DIC 来研究水力裂缝扩展。

他们的新希望是影响最新的火星任务,其中涉及2020 年登陆 Jezero 陨石坑的毅力号火星车。之所以选择这个地点,是因为人们相信,在亿万年前的某一时刻,这里有一个可能存在生命的大湖。

然而,湖泊最终干涸了,这就是为什么有些人认为火山口周围发现的裂缝实际上是残留的干燥裂缝。莫赫塔里说,这一理论之所以受到关注,是因为该地区的许多裂缝都呈现出多边形形状,这与我们在地球上干涸的湖床上看到的干燥裂缝不同。

其他人认为裂缝是由构造、热变化甚至静水压力造成的。“就像我们使用的水力压裂过程一样,除了来自地层本身之外,这是相似的,”莫赫塔里对后一种理论解释道。

但关键是,在其中一些岩石落入科学家和研究人员手中之前,我们可能无法确定这一切。由于美国宇航局提出的火星样本返回(MSR)任务,这一天预计将在下十年到来。

jpt_23_mars_sample_return.jpg
渲染图展示了多个机器人的概念,这些机器人将收集和发送美国宇航局火星毅力号火星车从火星表面收集的岩石和土壤样本。
资料来源:美国宇航局。

MSR 任务的目标是在 2028 年之前向火星发射一艘航天器,将毅力号收集的样本装载到火星上,然后在 2033 年之前用火箭送回地球。本月,在 NASA 的OSIRIS-Rex成功投放后,这个想法获得了一些先例将从附近小行星表面收集的所谓“原始样本”带到地球。

莫赫塔里表示,如果 NASA 决定在 MSR 任务期间归还一些裂隙岩石,它将需要了解岩石力学及其与检索和保存样本之间关系的石油和天然气专家的帮助。

“这将是一个微妙的项目,因为这些类型的岩石(带有纹理)的抗拉强度是完整样本的三分之一,”他说。换句话说,这些有价值的样本可能会在采集过程中或在运送到新星球的过程中分解。

莫赫塔里表示,好消息是石油和天然气行业及其学术部门在这方面拥有数十年的经验。

“我们的目标是将美国宇航局在火星上所做的事情与我们在石油工程领域所做的事情联系起来,”他说。“他们有很多优秀的地质学家,可以制造漫游车,但我们也知道很多如何取样,对天然裂缝有深入的了解。”

进一步阅读:

Icarus 115760 与火星盖尔陨石坑硫酸钙矿脉相似的陆地机械特性,作者:Ali Ettehadi、Mehdi Mokhtari、Maksym Chuprin、路易斯安那大学拉斐特分校等人。

原文链接/jpt
Fracturing/pressure pumping

How Petroleum Engineering Can Help Explain the Mysteries of Mars Fractures

The natural fractures discovered on Mars during rover missions might be so important that they are worth bringing back to Earth.

jpt_23_natural_fractures_mars2.jpg
An image of an outcrop taken by NASA's Curiosity Mars rover revealed well-defined veins filled with whitish minerals, interpreted as calcium sulfate.
Source: NASA.

When oil and gas industry research efforts slowed down as a result of the COVID-19 pandemic it forced many in academia to look for new ways to diversify their own research portfolios. For some, that meant delving deeper into the topics of climate science and carbon management.

For Mehdi Mokhtari it also created an opportunity to use the earth sciences born from oil and gas research to help explore another world.

The associate professor at the petroleum engineering department of the University of Louisiana at Layfette recently published a study that argues NASA should bring naturally fractured rock samples from Mars back to Earth in a mission planned for next decade.

The rock mechanics expert and longtime space exploration enthusiast said the idea for the study came to him after recalling NASA’s Curiosity rover mission and the images of fractured rocks it sent back.

“There were these dips and wings in the fractures,” he said of the fractures found on the red planet, “and I knew they looked very similar to some of the complex fracture patterns that we see in some unconventional formations. That was very interesting and made me want to see if I could connect what we know here on Earth to what we have seen on Mars.”

But in particular, what Mokhtari and his research team are most focused on are the Mars rocks containing mineral-filled fractures, or veins, which he said represent “clues and evidence about the past presence of water on Mars which is, of course, a big question NASA is trying to answer.”

In 2012, Curiosity landed at a site known as the Gale Crater where it analyzed the minerology of Mars rocks using a tool called the “ChemCam.” The laser-spectrograph technology confirmed that some of the fractured rocks are filled with calcium sulfate, known to most as gypsum.

On Earth, we know that such mineralization often postdates the host rock’s fracture formation by millions of years. If such learnings can be confirmed by analyzing fractures on Mars, then it would help us understand the role water played in its ancient history—and maybe where most of it went.

One of the places Mokhtari and others are turning to in the meantime is Utah where mudstone outcrops are believed to closely resemble the fractured rocks found in recent years on Mars.

jpt_23_mars_utah_cores.JPG
Mineralized veinlets in (a) the ‘John Klein’ drill hole in the Sheepbed member of Yellowknife Bay, Mars next to an image (b) which shows a core of the Moenkopi mudstone formation in Utah.
Source: NASA/University of Louisiana at Lafayette.

What the team from the University of Louisiana at Lafayette is doing differently is using digital image correlation (DIC) to study the fractures and veins found in the Utah outcrops to suggest how they might have formed. The university research team pioneered the use of DIC for studying hydraulic fracture propagation several years ago.

Their new hope is to influence the latest mission on Mars which involves the Perseverance rover that landed in 2020 at the Jezero Crater. The site was chosen because it is believed that at one point eons ago it held a large lake which might have hosted life.

However, the lake eventually dried up which is why some think the fractures found around the crater are really leftover desiccation cracks. Mokhtari said this theory has gained traction because so many of the fractures in the area exhibit the polygonal shape that is distinctive of the desiccation cracks that we see in dry lakebeds on this planet.

Others believe the fractures were created by tectonics, thermal shifts, or even hydraulically due to hydrostatic pressure. “Just like the process we use known as hydraulic fracturing, this is similar except it comes from the formation itself,” explained Mokhtari of the latter theory.

But the key is that we may not know any of this for sure until some of these rocks are in the hands of scientists and researchers. That day is expected to come next decade thanks to NASA’s proposed Mars Sample Return (MSR) mission.

jpt_23_mars_sample_return.jpg
Rendering shows a concept for multiple robots that would collect and send samples of rock and soil collected from the Martian surface by NASA’s Mars Perseverance rover.
Source: NASA.

The goal of the MSR mission is to send a spacecraft to Mars by 2028 where samples collected by Perseverance will be loaded up and then rocketed back to Earth by 2033. The idea gained some precedent just this month after NASA’s OSIRIS-Rex successfully dropped to Earth what were described as “pristine samples” collected from the surface of a nearby asteroid.

Mokhtari said if NASA decides to return some fractured rock during the MSR mission, it will need the help of oil and gas experts who understand rock mechanics and how it relates to retrieving and preserving samples.

"It will be a delicate project because these kinds of rocks—ones with veins—have a tensile strength that is one-third that of a fully intact sample," he said. In other words, these valuable samples might fall apart either while taken or while in transit to their new planet.

Mokhtari said the good news is that the oil and gas industry and its academic wings have decades of experience in this matter.

“My goal here is to link what NASA is doing on Mars with what we can do in petroleum engineering,” he said. “They have a lot of good geologists and can make rovers, but we also know a lot about how to take samples and have a deep understanding of natural fractures.”

For Further Reading:

Icarus 115760 Mechanical Properties of Terrestrial Analogs to Calcium Sulfate Veins on Gale Crater, Mars by Ali Ettehadi, Mehdi Mokhtari, Maksym Chuprin, University of Louisiana at Lafayette, et al.