Apparent magnitude
Apparent magnitude (m) is a measure of the brightness of a star or other astronomical object observed from Earth. An object's apparent magnitude depends on its intrinsic luminosity, its distance from Earth, and any extinction of the object's light caused by interstellar dust along the line of sight to the observer. The measurement of apparent magnitude is called photometry. Photometric measurements are made in the ultraviolet, visible, or infrared wavelength bands using standard passband filters belonging to photometric systems such as the UBV system or the Strömgren uvbyβ system.
Apparant magnitudeApparent MagnitudeApparent Visual BrightnessApparent Visual MagnitudeApparent bightnessApparent bolometric magnitudeApparent brightnessApparent luminosityApparent visual magnitudeApparent visual magnitudesFifth magnitude starOptical magnitudePogson's RatioPogson's ratioPogsons ratioRelative magnitudeSecond magnitude starSixth magnitude starStellar magnitudeV magnitudeVisible magnitudeVisual apparent magnitudeVisual magnitude
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(119951)_2002_KX14(137108) 1999 AN10(152680) 1998 KJ9(153814) 2001 WN5(15874) 1996 TL66(163132) 2002 CU11(163348) 2002 NN4(163899)_2003_SD220(177049) 2003 EE16(192642)_1999_RD32(208996)_2003_AZ84(231937) 2001 FO32(237442) 1999 TA10(242450) 2004 QY2(276033) 2002 AJ129(285263) 1998 QE2(308242) 2005 GO21(308635) 2005 YU55(315898) 2008 QD4(33342) 1998 WT24(341843)_2008_EV5(35396) 1997 XF11(357439) 2004 BL86(367789) 2011 AG5(410777)_2009_FD(454101) 2013 BP73(458732) 2011 MD5(471240) 2011 BT15(501647) 2014 SD224(505657)_2014_SR339(523662) 2012 MU2(523671) 2013 FZ27(523764) 2014 WC510(523794)_2015_RR245(529366) 2009 WM1(532037) 2013 FY27(55636) 2002 TX300(55637)_2002_UX25(82075) 2000 YW134(84522)_2002_TC302
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Apparent magnitude
Apparent magnitude (m) is a measure of the brightness of a star or other astronomical object observed from Earth. An object's apparent magnitude depends on its intrinsic luminosity, its distance from Earth, and any extinction of the object's light caused by interstellar dust along the line of sight to the observer. The measurement of apparent magnitude is called photometry. Photometric measurements are made in the ultraviolet, visible, or infrared wavelength bands using standard passband filters belonging to photometric systems such as the UBV system or the Strömgren uvbyβ system.
has abstract
A magnitude aparente (m) de um ...... ver um objeto de magnitude 15.
@pt
Apparent magnitude (m) is a me ...... agnitude is normally intended.
@en
Astronomian, itxurazko magnitu ...... txikiagoa da bere magnitudea.
@eu
Die scheinbare Helligkeit gibt ...... taus hellste Objekt am Himmel.
@de
Hvězdná velikost (zdánlivá mag ...... í hvězdná velikost (viz dále).
@cs
La magnitud aparent d'un astre ...... entre la diferència U-B és l'.
@ca
La magnitud aparente (m) de un ...... rella y una fuente artificial.
@es
La magnitude apparente est une ...... teindre 34 en lumière visible.
@fr
La magnitudine apparente (m) d ...... cetto di magnitudine assoluta.
@it
Magnitudo semu atau Magnitudo ...... parsec jauhnya.
* l
* b
* s
@in
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1.021.814.372
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May 2019
@en
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talk:Apparent magnitude#Main Article Problems
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A magnitude aparente (m) de um ...... 100, ou aproximadamente 2,512.
@pt
Apparent magnitude (m) is a me ...... or the Strömgren uvbyβ system.
@en
Astronomian, itxurazko magnitu ...... txikiagoa da bere magnitudea.
@eu
Die scheinbare Helligkeit gibt ...... ßenklasse oder schlicht Größe.
@de
Hvězdná velikost (zdánlivá mag ...... í hvězdná velikost (viz dále).
@cs
La magnitud aparent d'un astre ...... reduir la magnitud una unitat.
@ca
La magnitud aparente (m) de un ...... un factor alrededor de 2,512.
@es
La magnitude apparente est une ...... aux erreurs d'étalonnage près.
@fr
La magnitudine apparente (m) d ...... o può apparire molto debole se
@it
Magnitudo semu atau Magnitudo ...... parsec jauhnya.
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label
Apparent magnitude
@en
Hvězdná velikost
@cs
Itxurazko magnitude
@eu
Magnitud aparent
@ca
Magnitud aparente
@es
Magnitude aparente
@pt
Magnitude apparente
@fr
Magnitudine apparente
@it
Magnitudo semu
@in
Obserwowana wielkość gwiazdowa
@pl