Analogo solare: differenze tra le versioni

Versione delle 22:38, 10 gen 2024

Versione delle 22:41, 10 gen 2024

Riga 27:

|-

|style="text-align:left;"| [[Epsilon Eridani]]

| {{RA|03|32|55.,9}}

| {{DEC|−09|27|30}}

| 10,5

Riga 36:

|-

|style="text-align:left;"| [[Tau Ceti]]<ref>La metallicità di Tau Ceti è incerta, in alcuni casi è stimata più del 70% rispetto al Sole; in questo caso la stella sarebbe un analogo solare.</ref>

| {{RA|01|44|04.,1}}

| {{DEC|−15|56|15}}

| 11,9

Riga 45:

|-

|style="text-align:left;"| [[Keid]] A

| {{RA|04|15|16.,3}}

| {{DEC|−07|39|10}}

| 16,5

Riga 54:

|-

|style="text-align:left;"| [[82 Eridani]]

| {{RA|03|19|55.,7}}

| {{DEC|−43|04|11.,2}}

| 19,8

| G8V

Riga 63:

|-

|style="text-align:left;"| [[Delta Pavonis]]

| {{RA|20|08|43.,6}}

| {{DEC|−66|10|55}}

| 19,9

Riga 72:

|-

|style="text-align:left;"| [[Gliese 785]]

| {{RA|20|15|17.,4}}

| {{DEC|−27|01|59}}

| 28,8

Riga 90:

|-

|style="text-align:left;"| [[Gliese 86]] A

| {{RA|02|10|25.,9}}

| {{DEC|−50|49|25}}

| 35,2

Riga 99:

|-

|style="text-align:left;"| [[54 Piscium]]

| {{RA|00|39|21.,8}}

| {{DEC|+21|15|02}}

| 36,1

Riga 108:

|-

|style="text-align:left;"| [[V538 Aurigae]]

| {{RA|05|41|20.,3}}

| {{DEC|+53|28|51.,8}}

| 39,9

| K1V

Riga 117:

|-

|style="text-align:left;"| [[HD 14412]]

| {{RA|02|18|58.,5}}

| {{DEC|−25|56|45}}

| 41,3

Riga 126:

|-

|style="text-align:left;"| [[HR 4587]]

| {{RA|12|00|44.,3}}

| {{DEC|-10|26|45.,7}}

| 42,1

|style="background-color:Moccasin;"| G8IV

Riga 135:

|-

|style="text-align:left;"| [[HD 172051]]

| {{RA|18|38|53.,4}}

| {{DEC|−21|03|07}}

| 42,7

Riga 144:

|-

|style="text-align:left;"| [[72 Herculis]]

| {{RA|17|20|39.,6}}

| {{DEC|+32|28|04}}

| 46,9

Riga 153:

|-

|style="text-align:left;"| [[HD 196761]]

| {{RA|20|40|11.,8}}

| {{DEC|−23|46|26}}

| 46,9

Riga 162:

|-

|style="text-align:left;"| [[Nu² Lupi]]

| {{RA|15|21|48.,1}}

| {{DEC|−48|19|03}}

| 47,5