The Local Bubble , or Local Cavity , [3] is a relative cavity in the interstellar medium (ISM) in the Orion Arm of the Milky Way . It contains, among others, the Local Interstellar Cloud , which contains the Solar System , and the G-Cloud . It is at least 300 light years across and is defined by its neutral- hydrogen density of about 0.05 atoms /cm 3 , or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm 3 ), and one sixth that of the Local Interstellar Cloud (0.3 atoms/cm 3 ). [4]
Year | Metadata | Sections | Top Words | First Paragraph |
2018 |
47131 characters 6 sections 5 paragraphs 15 images 70 internal links 23 external links |
bubble 0.551 loop 0.314 local 0.253 lic 0.239 ism 0.214 supernovae 0.198 interstellar 0.195 atoms 0.163 bubbles 0.125 cm3 0.121 cavity 0.113 cloud 0.104 medium 0.100 abuts 0.088 chipsat 0.088 |
The Local Bubble , or Local Cavity , [3] is a relative cavity in the interstellar medium (ISM) in the Orion Arm of the Milky Way . It contains, among others, the Local Interstellar Cloud , which contains the Solar System , and the G-Cloud . It is at least 300 light years across and is defined by its neutral- hydrogen density of about 0.05 atoms /cm 3 , or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm 3 ), and one sixth that of the Local Interstellar Cloud (0.3 atoms/cm 3 ). [4] |
|
2017 |
46171 characters 6 sections 5 paragraphs 14 images 66 internal links 22 external links |
bubble 0.567 loop 0.307 local 0.266 lic 0.234 ism 0.209 supernovae 0.194 interstellar 0.191 atoms 0.159 hot 0.140 bubbles 0.122 cm3 0.118 cavity 0.110 cloud 0.101 medium 0.098 abuts 0.086 |
The Local Bubble , or Local Cavity , [3] is a cavity in the interstellar medium (ISM) in the Orion Arm of the Milky Way . It contains, among others, the Local Interstellar Cloud , which contains the Solar System , and the G-cloud . It is at least 300 light years across and has a neutral- hydrogen density of about 0.05 atoms /cm 3 , or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm 3 ), and one sixth that of the Local Interstellar Cloud (0.3 atoms/cm 3 ). [4] The hot diffuse gas in the Local Bubble emits X-rays . |
|
2016 |
35206 characters 6 sections 5 paragraphs 3 images 64 internal links 20 external links |
bubble 0.569 loop 0.308 local 0.248 lic 0.235 ism 0.210 supernovae 0.195 interstellar 0.192 atoms 0.160 hot 0.141 bubbles 0.123 cm3 0.118 gemini 0.104 cloud 0.102 medium 0.098 abuts 0.087 |
The Local Bubble is a cavity in the interstellar medium (ISM) in the Orion Arm of the Milky Way . It contains, among others, the Local Interstellar Cloud , which contains the Solar System , and the G-cloud . It is at least 300 light years across and has a neutral- hydrogen density of about 0.05 atoms /cm 3 , or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm 3 ), and one sixth that of the Local Interstellar Cloud (0.3 atoms/cm 3 ). [3] The hot diffuse gas in the Local Bubble emits X-rays . |
|
2015 |
35195 characters 6 sections 5 paragraphs 3 images 64 internal links 20 external links |
bubble 0.569 loop 0.308 local 0.248 lic 0.235 ism 0.210 supernovae 0.195 interstellar 0.192 atoms 0.160 hot 0.141 bubbles 0.123 cm3 0.118 gemini 0.104 cloud 0.102 medium 0.098 abuts 0.087 |
The Local Bubble is a cavity in the interstellar medium (ISM) in the Orion Arm of the Milky Way . It contains, among others, the Local Interstellar Cloud , G-cloud , and the Solar System . It is at least 300 light years across and has a neutral- hydrogen density of about 0.05 atoms /cm 3 , or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm 3 ), and one sixth that of the Local Interstellar Cloud (0.3 atoms/cm 3 ). [3] The hot diffuse gas in the Local Bubble emits X-rays . |
|
2014 |
35183 characters 6 sections 5 paragraphs 3 images 64 internal links 20 external links |
bubble 0.569 loop 0.308 local 0.248 lic 0.235 ism 0.210 supernovae 0.195 interstellar 0.192 atoms 0.160 hot 0.141 bubbles 0.123 cm3 0.118 gemini 0.104 cloud 0.102 medium 0.098 abuts 0.087 |
The Local Bubble is a cavity in the interstellar medium (ISM) in the Orion Arm of the Milky Way . It contains, among others, the Local Interstellar Cloud , G-cloud , and the Solar System . It is at least 300 light years across and has a neutral- hydrogen density of about 0.05 atoms /cm 3 , or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm 3 ), and one sixth of the Local Interstellar Cloud (0.3 atoms/cm 3 ). [3] The hot diffuse gas in the Local Bubble emits X-rays . |
|
2013 |
27428 characters 6 sections 5 paragraphs 3 images 55 internal links 14 external links |
bubble 0.562 loop 0.290 local 0.251 ism 0.230 supernovae 0.214 interstellar 0.210 atoms 0.176 hot 0.155 cloud 0.140 bubbles 0.135 cm3 0.130 gemini 0.115 medium 0.108 abuts 0.095 chipsat 0.095 |
The Local Bubble is a cavity in the interstellar medium (ISM) in the Orion Arm of the Milky Way . It contains, among others, the Local Interstellar Cloud and G-cloud . It is at least 300 light years across and has a neutral- hydrogen density of about 0.05 atoms/cm 3 , or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm 3 ), and one sixth of the Local Interstellar Cloud (0.3 atoms/cm 3 ). [1] The hot diffuse gas in the Local Bubble emits X-rays . |
|
2012 |
26435 characters 6 sections 5 paragraphs 3 images 57 internal links 14 external links |
bubble 0.553 loop 0.285 local 0.268 ism 0.226 supernovae 0.210 interstellar 0.207 atoms 0.173 cc 0.158 hot 0.152 cloud 0.137 bubbles 0.132 gemini 0.113 medium 0.106 abuts 0.094 chipsat 0.094 |
The Local Bubble is a cavity in the interstellar medium (ISM) in the Orion Arm of the Milky Way which contains the Local Interstellar Cloud and G-cloud (as well as others). It is at least 300 light years across and has a neutral hydrogen density of about 0.05 atoms per cubic centimetre, or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cc), and one sixth of the Local Fluff , or Local Interstellar Cloud (0.3 atoms/cc). [1] The hot diffuse gas in the Local Bubble emits X-rays . |
|
2011 |
25364 characters 6 sections 5 paragraphs 3 images 54 internal links 13 external links |
bubble 0.515 loop 0.319 local 0.253 ism 0.253 supernovae 0.235 atoms 0.193 cc 0.177 interstellar 0.165 bubbles 0.148 gemini 0.126 abut 0.105 abuts 0.105 chipsat 0.105 hot 0.102 galactic 0.096 |
The Local Bubble is a cavity in the interstellar medium (ISM) of the Orion Arm of the Milky Way . It is at least 300 light years across and has a neutral hydrogen density of about 0.05 atoms per cubic centimetre, or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cc), and half that for the "Local Fluff", or Local Interstellar Cloud (0.1 atoms/cc). The hot diffuse gas in the Local Bubble emits X-rays . |
|
2010 |
15967 characters 4 sections 4 paragraphs 3 images 46 internal links 6 external links |
bubble 0.520 loop 0.345 ism 0.274 local 0.249 atoms 0.209 cc 0.192 supernovae 0.169 bubbles 0.160 interstellar 0.143 gemini 0.136 abut 0.113 abuts 0.113 galactic 0.104 geminga 0.102 scorpii 0.102 |
The Local Bubble is a cavity in the interstellar medium (ISM) of the Orion Arm of the Milky Way . It is at least 300 light years across and has a neutral hydrogen density of about 0.05 atoms per cubic centimetre, or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cc), and half that for the "Local Fluff," or Local Interstellar Cloud (0.1 atoms/cc). The hot diffuse gas in the Local Bubble emits X-rays . |
|
2009 |
16272 characters 5 sections 6 paragraphs 3 images 46 internal links 6 external links |
bubble 0.549 loop 0.340 local 0.270 ism 0.270 atoms 0.206 cc 0.189 supernovae 0.167 bubbles 0.158 gemini 0.134 abuts 0.112 interstellar 0.106 galactic 0.103 geminga 0.101 scorpii 0.101 lic 0.101 |
The Local Bubble is a cavity in the interstellar medium (ISM) of the Orion Arm of the Milky Way . It is at least 300 light years across and has a neutral hydrogen density of about 0.05 atoms per cubic centimetre, or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cc), and half that for the "Local Fluff," or Local Interstellar Cloud (0.1 atoms/cc). The hot diffuse gas in the Local Bubble emits X-rays . The very sparse, hot gas of the Local Bubble is the result of supernovae that exploded within the past two to four million years. [1] The most likely candidate for the remains of this supernova is " Geminga " ("Gemini gamma-ray source"), a pulsar in the constellation Gemini . |
|
2008 |
13152 characters 3 sections 6 paragraphs 2 images 45 internal links 4 external links |
bubble 0.584 loop 0.362 ism 0.287 local 0.235 supernovae 0.178 bubbles 0.168 gemini 0.143 abuts 0.119 atoms 0.109 galactic 0.109 geminga 0.107 scorpii 0.107 lic 0.107 cubic 0.107 pulsar 0.089 |
The Local Bubble is a cavity in the interstellar medium (ISM) of the Orion Arm of the Milky Way . It is at least 300 light years across and has a neutral hydrogen density approximately one tenth of the 0.5 atoms per cubic centimetre average for the ISM in the Milky Way . The hot diffuse gas in the Local Bubble emits X-rays . The very sparse, hot gas of the Local Bubble is the result of supernovae that exploded within the past two to four million years. [1] The most likely candidate for the remains of this supernova is " Geminga " ("Gemini gamma-ray source"), a pulsar in the constellation Gemini . |
|
2007 |
6121 characters 2 sections 7 paragraphs 1 images 20 internal links 4 external links |
bubble 0.559 ism 0.366 loop 0.346 local 0.275 supernovae 0.170 bubbles 0.161 abuts 0.114 atoms 0.105 galactic 0.105 geminga 0.103 scorpii 0.103 lic 0.103 cubic 0.102 template 0.096 fluff 0.091 |
The Local Bubble is a cavity in the interstellar medium (ISM) of the Orion Arm of the Milky Way . It is at least 300 light years across and has a neutral hydrogen density approximately one tenth of the 0.5 atoms per cubic centimetre average for the ISM in the Milky Way . The hot diffuse gas in the Local Bubble emits X-rays . |
|
2006 |
5286 characters 1 sections 8 paragraphs 1 images 16 internal links 4 external links |
loop 0.429 ism 0.425 bubble 0.416 local 0.279 bubbles 0.224 fluff 0.170 supernovae 0.158 atoms 0.146 cubic 0.142 centimetre 0.133 gemini 0.127 abuts 0.106 iii 0.100 galactic 0.097 geminga 0.095 |
The Local Bubble is a cavity in the local interstellar medium (ISM) at least 300 light years across containing a neutral hydrogen density that is approximately one tenth of that of the average ISM in the Milky Way (approximately 0.05 atoms per cubic centimetre , as opposed to 0.5 atoms per cubic centimetre). The hot diffuse gas in the Local Bubble emits X-rays . |
|
2005 |
4469 characters 0 sections 4 paragraphs 1 images 16 internal links 0 external links |
ism 0.539 bubble 0.395 local 0.294 fluff 0.215 loop 0.204 supernovae 0.200 atoms 0.185 cubic 0.180 centimetre 0.168 abuts 0.134 galactic 0.123 density 0.107 scorpius 0.095 bubbles 0.095 plane 0.093 |
The Local Bubble is a cavity in the local interstellar medium (ISM) at least 300 light years across containing a neutral hydrogen density that is approximately one tenth of that of the average ISM in the Milky Way (approximately 0.05 atoms per cubic centimetre , as opposed to 0.5 atoms per cubic centimetre). The hot diffuse gas in the Local Bubble emits X-rays . |
|
2004 |
2787 characters 0 sections 4 paragraphs 0 images 13 internal links 0 external links |
ism 0.539 bubble 0.395 local 0.294 fluff 0.215 loop 0.204 supernovae 0.200 atoms 0.185 cubic 0.180 centimetre 0.168 abuts 0.134 galactic 0.123 density 0.107 scorpius 0.095 bubbles 0.095 plane 0.093 |
The Local Bubble is a cavity in the local interstellar medium (ISM) at least 300 light years across containing a neutral hydrogen density that is approximately one tenth of that of the average ISM in the Milky Way (approximately 0.05 atoms per cubic centimetre , as opposed to 0.5 atoms per cubic centimetre). The hot diffuse gas in the Local Bubble emits X-rays . |