| DC Field | Value | Language |
|---|---|---|
| dc.contributor.editor | Balogh, André | - |
| dc.contributor.editor | Ksanfomaliti, L. V. | - |
| dc.contributor.editor | Steiger, R. von | - |
| dc.date.accessioned | 2017-04-14T07:30:29Z | - |
| dc.date.available | 2017-04-14T07:30:29Z | - |
| dc.date.issued | 2008 | - |
| dc.identifier.isbn | 978-0-387-77538-8 | - |
| dc.identifier.uri | http://repository.vnu.edu.vn/handle/VNU_123/28760 | - |
| dc.description.abstract | Mercury, the planet closest to the Sun, is different in several respects from the other three terrestrial planets. In appearance, it resembles the heavily cratered surface of the Moon, but its density is high, it has a magnetic field and magnetosphere, but no atmosphere or ionosphere. This book reviews the progress made in Mercury studies since the flybys by Mariner 10 in 1974-75, based on the continued research using the Mariner 10 archive, on observations from Earth, and on increasingly realistic models of its interior evolution. | - |
| dc.format.extent | 460 p. | - |
| dc.language.iso | en | en_US |
| dc.publisher | Springer | en_US |
| dc.rights | © 2008 Springer Science+Business Media, BV | - |
| dc.subject | Physics and Astronomy | en_US |
| dc.subject | Earth Sciences | - |
| dc.subject | Geography | - |
| dc.title | Mercury | en_US |
| dc.type | Book | en_US |
| Appears in Collections: | Khoa học Trái đất, Không gian & Môi trường | |
Readership Map
Content Distribution
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.editor | Balogh, André | - |
| dc.contributor.editor | Ksanfomaliti, L. V. | - |
| dc.contributor.editor | Steiger, R. von | - |
| dc.date.accessioned | 2017-04-14T07:30:29Z | - |
| dc.date.available | 2017-04-14T07:30:29Z | - |
| dc.date.issued | 2008 | - |
| dc.identifier.isbn | 978-0-387-77538-8 | - |
| dc.identifier.uri | http://repository.vnu.edu.vn/handle/VNU_123/28760 | - |
| dc.description.abstract | Mercury, the planet closest to the Sun, is different in several respects from the other three terrestrial planets. In appearance, it resembles the heavily cratered surface of the Moon, but its density is high, it has a magnetic field and magnetosphere, but no atmosphere or ionosphere. This book reviews the progress made in Mercury studies since the flybys by Mariner 10 in 1974-75, based on the continued research using the Mariner 10 archive, on observations from Earth, and on increasingly realistic models of its interior evolution. | - |
| dc.format.extent | 460 p. | - |
| dc.language.iso | en | en_US |
| dc.publisher | Springer | en_US |
| dc.rights | © 2008 Springer Science+Business Media, BV | - |
| dc.subject | Physics and Astronomy | en_US |
| dc.subject | Earth Sciences | - |
| dc.subject | Geography | - |
| dc.title | Mercury | en_US |
| dc.type | Book | en_US |
| Appears in Collections: | Khoa học Trái đất, Không gian & Môi trường | |
