To save content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about saving content to .
To save content items to your Kindle, first ensure no-reply@cambridge.org
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about saving to your Kindle.
Note you can select to save to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
As a star ages, more and more of the hydrogen in its core becomes consumed by fusion into helium. Once this core hydrogen is used up, how does the star react and adjust? Stars at this post-main-sequence stage of life actually start to expand, eventually becoming much brighter giant or supergiant stars, shining with a luminosity that can be thousands or even tens of thousands that of their core-H-burning main sequence. We discuss how such stars reach their stellar end points as planetary nebulae or white dwarfs.
To understand ways we might infer stellar distances, we first consider how we intuitively estimate distance in our everyday world, through apparent angular size, and/or using our stereoscopic vision. We explain a practical, quite direct way to infer distances to relatively nearby stars, namely through the method of trigonometric parallax. This leads to the definition of the astronomical unit and parsec, and the concept of solid angles on the sky, measured in steradians or square degrees.
What are the key physical properties we can aspire to know about a star? In this chapter we consider the properties of stars, identifying first what we can directly observe about a given star: position on the sky, apparent brightness, color/spectrum. When these observations are combined with a clear understanding of some basic physical principles, we can infer many of the key physical properties of stars. We also make a brief aside to discuss ways to get our heads around the enormous distances and timescales we encounter in astrophysics.
This third volume of the award-winning The International Atlas of Mars Exploration picks up the story where Volume 2 left off, after the first Martian year of Curiosity's mission in 2014. Covering the exploration of Mars from 2015 to 2021 and supported by a unique set of detailed annotated maps and graphics, this volume documents the activities of Opportunity, Curiosity, InSight, China's rover Zhurong, and the early activities of Mars 2020. This essential visual reference chronicles the day-to-day operations of each mission, recording future landing site planning, how landing sites were chosen and what happened during each mission. Like the previous volumes, the atlas is accessible to space enthusiasts, but the bibliography and meticulous detail make it a particularly valuable resource for academic researchers and students working in planetary science and planetary mapping.
This section adds details for several past orbiter missions to bring them up to date, and includes the discovery of the Beagle 2 lander apparently intact on the Martian surface.
This section examines planning for missions after Curiosity, including the process of landing site selection. It depicts the activities of NASA’s InSight lander and Perseverance rover, China’s Tianwen-1 lander and Zhurong rover, and orbiting spacecraft including MAVEN, Hope and the Trace Gas Orbiter. Plans for future human exploration of Mars are presented as they were imagined in this period.
A survey of spacecraft results and mission planning for the Martian satellites, Phobos and Deimos, since 2014. Images and other observations by many spacecraft are included, as well as plans for future missions.
We consider solutions that can be obtained via dimensional reduction. We first consider the domain wall, both the perturbative nonrelativistic solution and the exact relativistic solution, first directly in four dimensions, and then show how it can be described via dimensional reduction. Then we consider the cosmic string solution, first directly in four dimensions, and then via dimensional reduction, and finally deriving it at weak field. Finally, we consider the BTZ black hole solution in 2+1 dimensions, deriving it directly, and then show how the BTZ solution and AdS space are continuously related.